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Cassini >> MIMI

CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE
CO-S-MIMI-4-INCA-CALIB-V1.0	PDS 3 CERTIFIED

Start Time: 2004-01-01 16:00:00 - Stop Time: 2017-09-15 03:28:13

CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE

Citiation Information

Author	Vandegriff J., Kusterer M.B.
Title	CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE
Publisher	NASA Planetary Data System
Publication Year	2018
doi	https://doi.org/10.17189/1519607

Top/ DATA/ IANGAVE0_T/ 2017 /

IANGAVE0_T_2017001_02

Start Time:	2017-001T00:00:13.129	Stop Time:	2017-001T23:58:43.576
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017002_02

Start Time:	2017-002T00:00:13.576	Stop Time:	2017-002T23:58:15.023
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017003_02

Start Time:	2017-003T00:00:22.023	Stop Time:	2017-003T21:56:46.517
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017004_02

Start Time:	2017-004T20:28:55.997	Stop Time:	2017-004T23:59:54.916
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017005_02

Start Time:	2017-005T00:02:01.916	Stop Time:	2017-005T23:59:45.363
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017006_02

Start Time:	2017-006T00:01:15.363	Stop Time:	2017-006T23:59:45.810
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017007_02

Start Time:	2017-007T00:01:15.810	Stop Time:	2017-007T23:59:46.257
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017008_02

Start Time:	2017-008T00:01:16.256	Stop Time:	2017-008T23:59:42.704
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017009_02

Start Time:	2017-009T00:01:12.703	Stop Time:	2017-009T14:51:12.362
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017010_02

Start Time:	2017-010T01:33:43.115	Stop Time:	2017-010T19:37:26.698
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017011_02

Start Time:	2017-011T00:42:26.581	Stop Time:	2017-011T22:34:54.077
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017012_02

Start Time:	2017-012T11:59:54.768	Stop Time:	2017-012T23:59:55.491
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017013_02

Start Time:	2017-013T00:01:25.491	Stop Time:	2017-013T23:58:55.939
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017014_02

Start Time:	2017-014T00:00:25.938	Stop Time:	2017-014T23:58:55.385
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017015_02

Start Time:	2017-015T00:00:25.385	Stop Time:	2017-015T23:58:48.832
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017016_02

Start Time:	2017-016T00:00:56.832	Stop Time:	2017-016T18:00:26.417
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017017_02

Start Time:	2017-017T07:43:27.101	Stop Time:	2017-017T23:37:57.734
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017018_02

Start Time:	2017-018T15:07:28.377	Stop Time:	2017-018T23:59:12.173
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017019_02

Start Time:	2017-019T00:01:20.172	Stop Time:	2017-019T23:58:36.620
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017020_02

Start Time:	2017-020T00:00:44.619	Stop Time:	2017-020T23:59:35.066
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017021_02

Start Time:	2017-021T00:01:05.066	Stop Time:	2017-021T23:59:35.513
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017022_02

Start Time:	2017-022T00:01:05.513	Stop Time:	2017-022T23:59:55.960
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017023_02

Start Time:	2017-023T00:01:25.959	Stop Time:	2017-023T23:59:45.407
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017024_02

Start Time:	2017-024T00:00:45.407	Stop Time:	2017-024T23:58:50.854
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017025_02

Start Time:	2017-025T00:00:58.853	Stop Time:	2017-025T23:28:22.313
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017026_02

Start Time:	2017-026T08:53:23.096	Stop Time:	2017-026T23:58:00.748
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017027_02

Start Time:	2017-027T00:00:07.747	Stop Time:	2017-027T23:58:48.195
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017028_02

Start Time:	2017-028T00:00:56.194	Stop Time:	2017-028T23:59:04.642
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017029_02

Start Time:	2017-029T00:01:11.641	Stop Time:	2017-029T23:58:16.089
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017030_02

Start Time:	2017-030T00:00:24.088	Stop Time:	2017-030T23:59:29.535
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017031_02

Start Time:	2017-031T00:00:44.535	Stop Time:	2017-031T23:59:39.982
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017032_02

Start Time:	2017-032T00:01:47.981	Stop Time:	2017-032T23:59:28.429
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017033_02

Start Time:	2017-033T00:00:58.428	Stop Time:	2017-033T23:59:27.876
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017034_02

Start Time:	2017-034T00:00:57.875	Stop Time:	2017-034T23:59:28.323
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017035_02

Start Time:	2017-035T00:00:58.322	Stop Time:	2017-035T23:59:28.769
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017036_02

Start Time:	2017-036T00:00:58.769	Stop Time:	2017-036T23:59:28.216
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017037_02

Start Time:	2017-037T00:00:58.216	Stop Time:	2017-037T23:58:34.664
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017038_02

Start Time:	2017-038T00:00:41.663	Stop Time:	2017-038T17:21:42.263
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017039_02

Start Time:	2017-039T01:50:28.067	Stop Time:	2017-039T11:24:28.847
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017040_02

Start Time:	2017-040T14:32:53.221	Stop Time:	2017-040T23:58:08.004
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017041_02

Start Time:	2017-041T00:00:16.004	Stop Time:	2017-041T23:59:46.451
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017042_02

Start Time:	2017-042T00:01:16.450	Stop Time:	2017-042T23:59:46.897
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017043_02

Start Time:	2017-043T00:01:16.897	Stop Time:	2017-043T23:59:47.344
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017044_02

Start Time:	2017-044T00:01:17.344	Stop Time:	2017-044T23:59:02.791
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017045_02

Start Time:	2017-045T00:00:32.791	Stop Time:	2017-045T23:59:33.238
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017046_02

Start Time:	2017-046T00:00:33.238	Stop Time:	2017-046T18:45:23.806
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017047_02

Start Time:	2017-047T12:29:25.397	Stop Time:	2017-047T23:58:40.132
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017048_02

Start Time:	2017-048T00:00:49.131	Stop Time:	2017-048T23:58:30.579
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017049_02

Start Time:	2017-049T00:00:00.579	Stop Time:	2017-049T23:59:01.026
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017050_02

Start Time:	2017-050T00:00:31.025	Stop Time:	2017-050T23:59:01.473
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017051_02

Start Time:	2017-051T00:00:31.472	Stop Time:	2017-051T23:59:00.920
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017052_02

Start Time:	2017-052T00:00:45.919	Stop Time:	2017-052T10:37:23.674
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017053_02

Start Time:	2017-053T10:03:18.134	Stop Time:	2017-053T19:39:29.913
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017054_02

Start Time:	2017-054T07:50:45.632	Stop Time:	2017-054T23:58:05.260
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017055_02

Start Time:	2017-055T00:00:14.260	Stop Time:	2017-055T23:58:49.707
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017056_02

Start Time:	2017-056T00:00:19.707	Stop Time:	2017-056T00:51:50.687
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017057_02

Start Time:	2017-057T08:10:51.965	Stop Time:	2017-057T23:58:32.601
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017058_02

Start Time:	2017-058T00:00:02.600	Stop Time:	2017-058T23:58:33.048
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017059_02

Start Time:	2017-059T00:00:03.047	Stop Time:	2017-059T23:59:03.494
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017060_02

Start Time:	2017-060T00:00:18.494	Stop Time:	2017-060T23:58:34.942
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017061_02

Start Time:	2017-061T00:00:04.941	Stop Time:	2017-061T07:36:34.766
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017062_02

Start Time:	2017-062T07:07:06.224	Stop Time:	2017-062T23:59:36.835
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017063_02

Start Time:	2017-063T00:01:06.834	Stop Time:	2017-063T23:58:57.282
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017064_02

Start Time:	2017-064T00:00:27.281	Stop Time:	2017-064T23:58:57.729
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017065_02

Start Time:	2017-065T00:00:27.728	Stop Time:	2017-065T23:59:17.176
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017066_02

Start Time:	2017-066T00:01:25.175	Stop Time:	2017-066T23:59:55.622
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017067_02

Start Time:	2017-067T00:01:25.622	Stop Time:	2017-067T23:59:09.069
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017068_02

Start Time:	2017-068T00:01:17.069	Stop Time:	2017-068T23:57:26.517
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017069_02

Start Time:	2017-069T07:45:27.337	Stop Time:	2017-069T23:58:56.963
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017070_02

Start Time:	2017-070T00:00:26.963	Stop Time:	2017-070T23:54:30.412
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017071_02

Start Time:	2017-071T16:40:58.025	Stop Time:	2017-071T23:58:57.857
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017072_02

Start Time:	2017-072T00:00:27.856	Stop Time:	2017-072T23:58:41.304
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017073_02

Start Time:	2017-073T00:00:11.303	Stop Time:	2017-073T23:59:12.751
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017074_02

Start Time:	2017-074T00:00:12.750	Stop Time:	2017-074T23:58:51.198
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017075_02

Start Time:	2017-075T00:00:06.197	Stop Time:	2017-075T23:59:21.644
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017076_02

Start Time:	2017-076T00:00:51.644	Stop Time:	2017-076T23:58:39.091
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017077_02

Start Time:	2017-077T00:00:09.091	Stop Time:	2017-077T23:59:25.538
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017078_02

Start Time:	2017-078T00:01:10.537	Stop Time:	2017-078T23:58:48.985
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017079_02

Start Time:	2017-079T00:00:33.984	Stop Time:	2017-079T23:59:05.432
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017080_02

Start Time:	2017-080T00:00:50.431	Stop Time:	2017-080T23:59:19.879
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017081_02

Start Time:	2017-081T00:00:19.878	Stop Time:	2017-081T23:59:59.325
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017082_02

Start Time:	2017-082T00:01:29.325	Stop Time:	2017-082T23:08:28.792
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017083_02

Start Time:	2017-083T12:20:29.488	Stop Time:	2017-083T23:58:52.219
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017084_02

Start Time:	2017-084T00:00:22.219	Stop Time:	2017-084T23:34:19.676
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017085_02

Start Time:	2017-085T11:19:50.405	Stop Time:	2017-085T23:29:44.124
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017086_02

Start Time:	2017-086T03:35:14.030	Stop Time:	2017-086T23:59:14.560
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017087_02

Start Time:	2017-087T00:00:44.559	Stop Time:	2017-087T23:59:53.006
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017088_02

Start Time:	2017-088T00:00:53.006	Stop Time:	2017-088T16:07:38.635
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017089_02

Start Time:	2017-089T09:46:10.228	Stop Time:	2017-089T22:42:28.930
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017090_02

Start Time:	2017-090T14:30:59.566	Stop Time:	2017-090T23:59:27.347
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017091_02

Start Time:	2017-091T00:00:57.347	Stop Time:	2017-091T23:59:29.794
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017092_02

Start Time:	2017-092T00:00:59.793	Stop Time:	2017-092T23:59:30.241
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017093_02

Start Time:	2017-093T00:01:00.240	Stop Time:	2017-093T23:59:24.688
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017094_02

Start Time:	2017-094T00:00:54.687	Stop Time:	2017-094T23:59:38.135
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017095_02

Start Time:	2017-095T00:01:08.134	Stop Time:	2017-095T15:45:08.771
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017096_02

Start Time:	2017-096T00:16:46.575	Stop Time:	2017-096T22:39:51.059
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017097_02

Start Time:	2017-097T01:32:58.992	Stop Time:	2017-097T23:59:20.596
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017098_02

Start Time:	2017-098T00:01:24.908	Stop Time:	2017-098T13:18:35.168
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017099_02

Start Time:	2017-099T01:36:35.885	Stop Time:	2017-099T22:08:50.412
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017100_02

Start Time:	2017-100T12:55:52.071	Stop Time:	2017-100T23:58:51.816
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017101_02

Start Time:	2017-101T00:00:21.816	Stop Time:	2017-101T23:58:52.263
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017102_02

Start Time:	2017-102T00:00:22.262	Stop Time:	2017-102T19:13:21.820
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017103_02

Start Time:	2017-103T11:50:23.437	Stop Time:	2017-103T22:35:53.189
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017104_02

Start Time:	2017-104T06:22:53.954	Stop Time:	2017-104T16:54:00.711
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017105_02

Start Time:	2017-105T10:39:47.301	Stop Time:	2017-105T21:57:32.041
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017106_02

Start Time:	2017-106T10:27:18.753	Stop Time:	2017-106T23:59:18.440
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017107_02

Start Time:	2017-107T00:00:48.440	Stop Time:	2017-107T23:59:18.887
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017108_02

Start Time:	2017-108T00:00:48.886	Stop Time:	2017-108T23:59:18.333
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017109_02

Start Time:	2017-109T00:00:48.333	Stop Time:	2017-109T23:59:11.780
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017110_02

Start Time:	2017-110T00:00:26.779	Stop Time:	2017-110T23:11:55.245
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017111_02

Start Time:	2017-111T04:17:56.127	Stop Time:	2017-111T23:59:19.673
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017112_02

Start Time:	2017-112T00:00:49.672	Stop Time:	2017-112T23:59:20.119
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017113_02

Start Time:	2017-113T00:00:50.119	Stop Time:	2017-113T23:59:17.566
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017114_02

Start Time:	2017-114T00:00:47.565	Stop Time:	2017-114T23:59:18.012
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017115_02

Start Time:	2017-115T00:00:48.012	Stop Time:	2017-115T23:59:48.459
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017116_02

Start Time:	2017-116T00:00:48.458	Stop Time:	2017-116T21:00:48.974
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017117_02

Start Time:	2017-117T05:02:49.789	Stop Time:	2017-117T18:00:32.490
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017118_02

Start Time:	2017-118T10:03:33.119	Stop Time:	2017-118T20:58:43.868
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017119_02

Start Time:	2017-119T09:53:14.570	Stop Time:	2017-119T23:59:57.244
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017120_02

Start Time:	2017-120T00:01:27.244	Stop Time:	2017-120T17:32:27.840
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017121_02

Start Time:	2017-121T09:33:28.470	Stop Time:	2017-121T23:59:59.137
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017122_02

Start Time:	2017-122T00:01:29.137	Stop Time:	2017-122T23:58:59.584
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017123_02

Start Time:	2017-123T00:00:14.584	Stop Time:	2017-123T22:21:55.068
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017124_02

Start Time:	2017-124T09:34:55.809	Stop Time:	2017-124T20:29:35.558
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017125_02

Start Time:	2017-125T09:34:36.256	Stop Time:	2017-125T20:30:05.004
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017126_02

Start Time:	2017-126T09:24:05.706	Stop Time:	2017-126T20:57:06.440
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017127_02

Start Time:	2017-127T01:00:36.346	Stop Time:	2017-127T23:59:06.817
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017128_02

Start Time:	2017-128T00:00:36.816	Stop Time:	2017-128T23:59:16.263
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017129_02

Start Time:	2017-129T00:00:31.262	Stop Time:	2017-129T22:56:41.733
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017130_02

Start Time:	2017-130T10:45:42.461	Stop Time:	2017-130T23:58:55.156
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017131_02

Start Time:	2017-131T00:00:25.155	Stop Time:	2017-131T23:58:54.602
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017132_02

Start Time:	2017-132T00:00:24.602	Stop Time:	2017-132T23:59:21.049
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017133_02

Start Time:	2017-133T00:00:51.048	Stop Time:	2017-133T04:15:50.950
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017134_02

Start Time:	2017-134T11:46:52.223	Stop Time:	2017-134T21:42:22.994
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017135_02

Start Time:	2017-135T02:50:52.876	Stop Time:	2017-135T23:59:23.388
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017136_02

Start Time:	2017-136T00:00:38.388	Stop Time:	2017-136T19:47:08.932
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017137_02

IANGAVE0_T_2017138_02

Start Time:	2017-138T08:43:11.080	Stop Time:	2017-138T19:39:53.827
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017139_02

Start Time:	2017-139T09:39:24.505	Stop Time:	2017-139T19:46:30.271
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017140_02

Start Time:	2017-140T08:21:00.981	Stop Time:	2017-140T19:53:30.715
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017141_02

Start Time:	2017-141T12:13:02.339	Stop Time:	2017-141T23:59:32.067
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017142_02

Start Time:	2017-142T00:00:47.067	Stop Time:	2017-142T17:32:32.662
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017143_02

Start Time:	2017-143T03:32:03.432	Stop Time:	2017-143T23:59:19.960
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017144_02

Start Time:	2017-144T00:00:49.959	Stop Time:	2017-144T23:59:06.407
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017145_02

Start Time:	2017-145T00:01:13.406	Stop Time:	2017-145T19:46:08.949
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017146_02

Start Time:	2017-146T08:23:39.657	Stop Time:	2017-146T19:06:40.409
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017147_02

Start Time:	2017-147T08:16:11.105	Stop Time:	2017-147T23:59:10.742
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017148_02

Start Time:	2017-148T00:01:18.741	Stop Time:	2017-148T23:59:11.186
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017149_02

Start Time:	2017-149T00:01:19.186	Stop Time:	2017-149T12:03:51.907
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017150_02

Start Time:	2017-150T02:29:52.573	Stop Time:	2017-150T23:58:57.076
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017151_02

Start Time:	2017-151T00:00:27.076	Stop Time:	2017-151T23:59:01.521
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017152_02

Start Time:	2017-152T00:00:31.520	Stop Time:	2017-152T18:36:00.090
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017153_02

Start Time:	2017-153T01:24:00.933	Stop Time:	2017-153T23:58:30.411
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017154_02

Start Time:	2017-154T00:00:00.410	Stop Time:	2017-154T23:59:15.856
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017155_02

Start Time:	2017-155T00:00:45.855	Stop Time:	2017-155T21:13:54.364
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017156_02

Start Time:	2017-156T08:56:25.093	Stop Time:	2017-156T18:33:29.871
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017157_02

Start Time:	2017-157T07:42:38.567	Stop Time:	2017-157T18:25:24.319
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017158_02

Start Time:	2017-158T18:16:18.767	Stop Time:	2017-158T23:59:03.635
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017159_02

Start Time:	2017-159T00:01:11.634	Stop Time:	2017-159T23:59:46.080
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017160_02

Start Time:	2017-160T00:01:16.079	Stop Time:	2017-160T23:59:46.524
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017161_02

Start Time:	2017-161T00:01:16.524	Stop Time:	2017-161T23:59:46.969
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017162_02

Start Time:	2017-162T00:01:16.969	Stop Time:	2017-162T18:02:19.552
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017163_02

IANGAVE0_T_2017164_02

Start Time:	2017-164T06:42:21.704	Stop Time:	2017-164T17:34:16.453
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017165_02

Start Time:	2017-165T00:52:46.283	Stop Time:	2017-165T23:59:57.749
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017166_02

Start Time:	2017-166T00:01:27.748	Stop Time:	2017-166T23:58:58.194
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017167_02

Start Time:	2017-167T00:00:28.193	Stop Time:	2017-167T23:59:30.639
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017168_02

Start Time:	2017-168T00:00:15.638	Stop Time:	2017-168T22:12:34.125
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017169_02

Start Time:	2017-169T16:12:35.708	Stop Time:	2017-169T23:59:05.528
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017170_02

Start Time:	2017-170T00:00:35.528	Stop Time:	2017-170T17:10:28.131
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017171_02

Start Time:	2017-171T04:10:28.876	Stop Time:	2017-171T23:59:23.418
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017172_02

Start Time:	2017-172T00:00:53.417	Stop Time:	2017-172T23:59:23.863
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017173_02

Start Time:	2017-173T00:00:53.862	Stop Time:	2017-173T23:59:24.308
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017174_02

Start Time:	2017-174T00:00:54.307	Stop Time:	2017-174T23:59:24.753
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017175_02

Start Time:	2017-175T00:00:54.752	Stop Time:	2017-175T23:59:15.198
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017176_02

Start Time:	2017-176T00:00:45.197	Stop Time:	2017-176T23:58:06.643
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017177_02

Start Time:	2017-177T00:00:13.642	Stop Time:	2017-177T10:07:58.408
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017178_02

Start Time:	2017-178T03:28:59.006	Stop Time:	2017-178T14:12:28.758
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017179_02

Start Time:	2017-179T03:52:30.442	Stop Time:	2017-179T16:59:30.139
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017180_02

Start Time:	2017-180T00:46:30.959	Stop Time:	2017-180T23:59:31.422
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017181_02

Start Time:	2017-181T00:00:31.421	Stop Time:	2017-181T19:10:09.978
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017182_02

Start Time:	2017-182T10:08:40.632	Stop Time:	2017-182T23:58:59.312
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017183_02

Start Time:	2017-183T00:00:29.311	Stop Time:	2017-183T20:52:29.828
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017184_02

Start Time:	2017-184T16:13:31.381	Stop Time:	2017-184T23:58:01.202
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017185_02

Start Time:	2017-185T00:00:07.201	Stop Time:	2017-185T01:48:10.159
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017186_02

Start Time:	2017-186T04:54:42.532	Stop Time:	2017-186T23:58:42.091
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017187_02

Start Time:	2017-187T00:00:27.090	Stop Time:	2017-187T22:35:21.568
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017188_02

Start Time:	2017-188T05:12:51.415	Stop Time:	2017-188T23:59:33.981
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017189_02

Start Time:	2017-189T00:01:03.980	Stop Time:	2017-189T23:59:01.426
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017190_02

Start Time:	2017-190T00:00:31.425	Stop Time:	2017-190T23:59:44.870
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017191_02

Start Time:	2017-191T00:01:14.869	Stop Time:	2017-191T23:58:59.312
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017192_02

Start Time:	2017-192T00:01:07.311	Stop Time:	2017-192T23:59:44.754
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017193_02

Start Time:	2017-193T00:01:52.753	Stop Time:	2017-193T23:49:23.200
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017194_02

Start Time:	2017-194T00:06:23.193	Stop Time:	2017-194T23:58:16.638
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017195_02

Start Time:	2017-195T00:00:25.637	Stop Time:	2017-195T01:11:32.610
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017196_02

Start Time:	2017-196T06:01:34.939	Stop Time:	2017-196T15:35:15.717
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017197_02

Start Time:	2017-197T04:26:46.418	Stop Time:	2017-197T23:59:42.964
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017198_02

Start Time:	2017-198T00:01:12.963	Stop Time:	2017-198T23:59:08.406
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017199_02

Start Time:	2017-199T00:00:38.405	Stop Time:	2017-199T23:59:33.848
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017200_02

Start Time:	2017-200T00:01:14.847	Stop Time:	2017-200T20:49:10.364
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017201_02

Start Time:	2017-201T04:52:33.176	Stop Time:	2017-201T15:03:42.940
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017202_02

IANGAVE0_T_2017203_02

Start Time:	2017-203T04:00:08.081	Stop Time:	2017-203T23:59:21.616
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017204_02

Start Time:	2017-204T00:00:51.615	Stop Time:	2017-204T23:58:45.058
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017205_02

Start Time:	2017-205T00:00:15.058	Stop Time:	2017-205T23:58:45.500
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017206_02

Start Time:	2017-206T00:00:15.500	Stop Time:	2017-206T23:59:30.942
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017207_02

Start Time:	2017-207T00:00:45.942	Stop Time:	2017-207T23:59:49.384
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017208_02

Start Time:	2017-208T00:01:19.383	Stop Time:	2017-208T23:58:38.826
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017209_02

Start Time:	2017-209T00:00:08.826	Stop Time:	2017-209T23:58:55.268
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017210_02

Start Time:	2017-210T00:00:25.268	Stop Time:	2017-210T23:58:51.710
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017211_02

Start Time:	2017-211T00:00:21.710	Stop Time:	2017-211T14:29:21.373
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017212_02

Start Time:	2017-212T03:38:22.067	Stop Time:	2017-212T23:59:22.594
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017213_02

Start Time:	2017-213T00:00:22.594	Stop Time:	2017-213T23:58:35.037
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017214_02

Start Time:	2017-214T00:00:44.036	Stop Time:	2017-214T21:37:55.533
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017215_02

Start Time:	2017-215T03:53:40.387	Stop Time:	2017-215T07:33:01.303
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017216_02

Start Time:	2017-216T02:47:02.855	Stop Time:	2017-216T14:27:01.584
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017217_02

Start Time:	2017-217T02:44:02.299	Stop Time:	2017-217T14:25:11.027
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017218_02

Start Time:	2017-218T13:45:12.484	Stop Time:	2017-218T23:58:42.247
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017219_02

Start Time:	2017-219T00:00:12.246	Stop Time:	2017-219T21:39:43.743
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017220_02

Start Time:	2017-220T01:56:43.643	Stop Time:	2017-220T23:58:45.131
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017221_02

Start Time:	2017-221T00:00:15.130	Stop Time:	2017-221T23:58:44.573
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017222_02

Start Time:	2017-222T00:00:14.572	Stop Time:	2017-222T23:59:02.015
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017223_02

Start Time:	2017-223T00:00:32.014	Stop Time:	2017-223T23:59:02.457
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017224_02

Start Time:	2017-224T00:00:32.456	Stop Time:	2017-224T23:59:02.899
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017225_02

Start Time:	2017-225T00:00:47.898	Stop Time:	2017-225T23:59:34.340
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017226_02

Start Time:	2017-226T00:01:04.340	Stop Time:	2017-226T23:59:35.783
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017227_02

Start Time:	2017-227T00:01:20.782	Stop Time:	2017-227T23:59:39.225
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017228_02

Start Time:	2017-228T00:00:39.224	Stop Time:	2017-228T23:59:14.667
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017229_02

Start Time:	2017-229T00:00:29.666	Stop Time:	2017-229T23:59:33.109
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017230_02

Start Time:	2017-230T00:00:33.108	Stop Time:	2017-230T23:59:27.551
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017231_02

Start Time:	2017-231T00:00:27.550	Stop Time:	2017-231T23:59:29.993
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017232_02

Start Time:	2017-232T00:00:29.992	Stop Time:	2017-232T18:07:15.571
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017233_02

Start Time:	2017-233T01:21:46.403	Stop Time:	2017-233T13:02:54.131
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017234_02

Start Time:	2017-234T01:51:54.833	Stop Time:	2017-234T23:59:58.319
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017235_02

Start Time:	2017-235T00:01:28.318	Stop Time:	2017-235T23:59:44.761
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017236_02

Start Time:	2017-236T00:01:51.760	Stop Time:	2017-236T15:04:25.410
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017237_02

Start Time:	2017-237T11:53:26.926	Stop Time:	2017-237T23:58:11.645
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017238_02

Start Time:	2017-238T00:00:19.644	Stop Time:	2017-238T23:58:50.087
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017239_02

Start Time:	2017-239T00:00:05.087	Stop Time:	2017-239T23:59:52.529
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017240_02

Start Time:	2017-240T00:02:00.528	Stop Time:	2017-240T23:58:23.971
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017241_02

Start Time:	2017-241T00:00:31.970	Stop Time:	2017-241T13:51:01.649
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017242_02

Start Time:	2017-242T01:05:32.387	Stop Time:	2017-242T13:58:13.088
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017243_02

Start Time:	2017-243T01:14:14.826	Stop Time:	2017-243T23:59:32.297
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017244_02

Start Time:	2017-244T00:01:39.296	Stop Time:	2017-244T12:49:46.998
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017245_02

Start Time:	2017-245T03:20:06.157	Stop Time:	2017-245T23:34:04.191
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017246_02

Start Time:	2017-246T02:54:50.113	Stop Time:	2017-246T23:58:57.623
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017247_02

Start Time:	2017-247T00:00:27.623	Stop Time:	2017-247T23:59:28.065
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017248_02

Start Time:	2017-248T00:00:58.064	Stop Time:	2017-248T23:58:45.507
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017249_02

Start Time:	2017-249T00:00:15.507	Stop Time:	2017-249T11:44:37.234
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017250_02

Start Time:	2017-250T02:27:37.892	Stop Time:	2017-250T23:59:08.391
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017251_02

Start Time:	2017-251T00:00:38.391	Stop Time:	2017-251T23:59:24.833
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017252_02

Start Time:	2017-252T00:00:09.833	Stop Time:	2017-252T23:59:42.275
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017253_02

Start Time:	2017-253T00:01:12.275	Stop Time:	2017-253T23:59:00.717
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017254_02

Start Time:	2017-254T00:01:10.717	Stop Time:	2017-254T23:59:05.159
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017255_02

Start Time:	2017-255T00:00:35.159	Stop Time:	2017-255T23:59:04.601
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017256_02

Start Time:	2017-256T00:00:34.601	Stop Time:	2017-256T23:59:25.043
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017257_02

Start Time:	2017-257T00:00:25.043	Stop Time:	2017-257T23:59:26.485
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2017258_02

Start Time:	2017-258T00:00:26.485	Stop Time:	2017-258T10:30:28.241
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

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