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LRO CRaTER CDR Flight Data
LRO-L-CRAT-3-CDR-CALIBRATED-V1.0	PDS 3 CERTIFIED

Start Time: 2009-06-29 23:00:00 - Stop Time: 2023-09-30 23:59:59

LRO CRaTER CDR Flight Data

Citiation Information

Top/ DATA/ 2010/ 2010100 /

Start Time:	2010-04-10T00:00:03.22	Stop Time:	2010-04-10T23:59:47.22
Level 1 housekeeping data from CRaTER for year 2010 day 100. Information about the data columns can be found in the format files (.FMT) referenced in the label file (.LBL) associated with this data file. The format files are in the LABEL directory of the online volume. The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) is a stacked detector- absorber cosmic-ray telescope designed to answer key questions to enable future human exploration of the Solar System. CRaTER's primary measurement goal is to measure directly the lineal energy transfer (LET or 'y') spectra caused by space radiation penetrating and interacting with shielding material. Such measured LET spectra are frequently unavailable. In the absence of measurements, numerical models are used to provide estimates of LET--the reliability of the models require experimental measurements to provide a ground truth.

Start Time:	2010-04-10T00:00:00.22	Stop Time:	2010-04-10T23:59:59.22
Level 1 primary science data from CRaTER for year 2010 day 100. Information about the data columns can be found in the format files (.FMT) referenced in the label file (.LBL) associated with this data file. The format files are in the LABEL directory of the online volume. The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) is a stacked detector- absorber cosmic-ray telescope designed to answer key questions to enable future human exploration of the Solar System. CRaTER's primary measurement goal is to measure directly the lineal energy transfer (LET or 'y') spectra caused by space radiation penetrating and interacting with shielding material. Such measured LET spectra are frequently unavailable. In the absence of measurements, numerical models are used to provide estimates of LET--the reliability of the models require experimental measurements to provide a ground truth.

Start Time:	2010-04-10T00:00:00.22	Stop Time:	2010-04-10T23:59:59.22
Level 1 secondary science data from CRaTER for year 2010 day 100. Information about the data columns can be found in the format files (.FMT) referenced in the label file (.LBL) associated with this data file. The format files are in the LABEL directory of the online volume. The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) is a stacked detector- absorber cosmic-ray telescope designed to answer key questions to enable future human exploration of the Solar System. CRaTER's primary measurement goal is to measure directly the lineal energy transfer (LET or 'y') spectra caused by space radiation penetrating and interacting with shielding material. Such measured LET spectra are frequently unavailable. In the absence of measurements, numerical models are used to provide estimates of LET--the reliability of the models require experimental measurements to provide a ground truth.

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