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Lunar Reconnaissance Orbiter >> CRAT
LRO CRaTER DDR Flight Data View Errata Order Volume Toggle viewing into brief mode
LRO-L-CRAT-3/4-DDR-PROCESSED-V1.0 PDS 3      CERTIFIED
Start Time: 2009-06-29 09:00:00 - Stop Time: 2023-09-30 23:59:59
Processed (DDR) flight data from the CRaTER instrument, flown in the Lunar Reconnaissance Orbiter. Includes housekeeping (HK), primary science (PRI), and secondary science (SEC) data of levels 0. Data file names begin with CRAT_L0_xxx, where xxx is HK, PRI or SEC.
Processed (DDR) flight data from the CRaTER instrument, flown in the Lunar Reconnaissance Orbiter. Includes housekeeping (HK), primary science (PRI), and secondary science (SEC) data of levels 0. Data file names begin with CRAT_L0_xxx, where xxx is HK, PRI or SEC.    less ...
Citiation Information
Author Spence, H.E.
TitleLRO CRaTER DDR Flight Data
PublisherNASA Planetary Data System
Publication Year 2019
doi https://doi.org/10.17189/1519729
Top/ DATA/ 2011/ 2011260 / click here to download folders and files
CRAT_L2_HK_2011260_V01
Start Time: 2011-09-17T00:00:00.28 Stop Time: 2011-09-17T23:59:44.29
Level 2 housekeeping data from CRaTER for year 2011 day 260.
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.
CRAT_L2_PRI_2011260_V01
Start Time: 2011-09-17T00:00:00.28 Stop Time: 2011-09-17T23:59:59.29
Level 2 primary science data from CRaTER for year 2011 day 260.
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.
CRAT_L2_SEC_2011260_V01
Start Time: 2011-09-17T00:00:00.28 Stop Time: 2011-09-17T23:59:59.29
Level 2 secondary science data from CRaTER for year 2011 day 260.
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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