Data Set Information
DATA_SET_NAME ROSETTA-ORBITER X SREM 2 CRUISE 5 V1.0
DATA_SET_ID RO-X-SREM-2-CR5-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION
Data Set Overview : This data set contains 'raw' SREM count rate data (1/s), converted from the equivalent SREM Level 0 CDF products, which are provided in the EXTRAS directory. Note that the CDF processing levels differ from the CODMAC definition used within these PDS data sets. The SREM CDF Level 0 data are equivalent to the PDS CODMAC Level 2 data while the SREM CDF Level 2 data are equivalent to the PDS CODMAC Level 5 data. Associated standard deviations are also provided within each data product, calculated as the square root of the count rate values. These data are useful for determining the energetic particle environment experienced by the Standard Radiation Environment Monitor onboard the Rosetta Orbiter. Processing : These are 'raw' count rate data converted directly from the equivalent SREM Level 0 CDF data. No additional processing has been completed. Standard deviations are provided within each data product, along side the data, and are calculated as the square root of the count rate values. Data : One data product is provided per day of measurement. Data products are named according to the following convention: SREM_L_YYYYMMDD.EXT Where:  is the CODMAC processing level (2 for the count rate data and 5 for the derived proton and electron flux data). YYYMMDD is the date of the observation. EXT is the file extension (TAB for the ASCII data table and LBL for the detached PDS label file). All data products are formatted as plain ASCII tables and have an associated detached PDS label. The CODMAC Level 2 data are given as count rates (1/s) for each of the 15 SREM energy bins, and their associated standard deviations (calculated as square root of the count rate). Measurements are time tagged at the middle of the time interval (centered). The following table provides a list of the 15 SREM channels and the corresponding energy ranges of detected protons and electrons. |:|:|:|:|:| | SREM | Proton Energy [Mev] | Electron Energy [MeV] | |------|----------|----------|----------|------------| | Bin | Emin | Emax | Emin | Emax | |:|:|:|:|:| | TC1 | 27 | infinity | 2.00 | infinity | |------|----------|----------|----------|------------| | S12 | 26 | infinity | 2.08 | infinity | |------|----------|----------|----------|------------| | S13 | 27 | infinity | 2.23 | infinity | |------|----------|----------|----------|------------| | S14 | 24 | 542 | 3.20 | infinity | |------|----------|----------|----------|------------| | S15 | 23 | 434 | 8.18 | infinity | |:|:|:|:|:| | TC2 | 49 | infinity | 2.80 | infinity | |------|----------|----------|----------|------------| | S25 | 48 | 270 | - | - | |------|----------|----------|----------|------------| | C1 | 43 | 86 | - | - | |------|----------|----------|----------|------------| | C2 | 52 | 278 | - | - | |------|----------|----------|----------|------------| | C3 | 76 | 450 | - | - | |------|----------|----------|----------|------------| | C4 | 164 | infinity | 8.10 | infinity | |:|:|:|:|:| | TC3 | 12 | infinity | 0.80 | infinity | |------|----------|----------|----------|------------| | S32 | 12 | infinity | 0.75 | infinity | |------|----------|----------|----------|------------| | S33 | 12 | infinity | 1.05 | infinity | |------|----------|----------|----------|------------| | S34 | 12 | infinity | 2.08 | infinity | |:|:|:|:|:| Table Extracted from [SANDBERGETAL2012] The LBL file contains metadata with information about the instrument, mission, any important instrument parameters or measurement parameters, start and stop time of the measurement, and the pointer to the TAB object. The data table is structured as follows: - A first row with text headers defining the corresponding SREM channel and standard deviation for each column in the subsequent table. - The data table (called SREM_COUNT_RATES_TABLE) with each row containing the following columns: Time: A time tag per measurement, at the center of the observation. Count Rates: 15 count rates values (one per channel). Standard Deviations: 15 standard deviation values (one per count rate) calculated as the square root of the count rates. IMPORTANT NOTES: - As noted above, the time values provided mark the center time of the observation. - The PDS keyword MISSING_CONSTANT, which is provided in every LBL file, indicates the value (-1.0E31) used in the data table if no measurement data is available. Any zero values in the data tables are real measurements. Software : No software is provided with this data set. All products are provided as plain ASCII tables and can be read using the standard freely available NASAView and ReadPDS software packages. Media/Format : The data set will be delivered and kept online.
DATA_SET_RELEASE_DATE 2020-12-01T00:00:00.000Z
START_TIME 2009-12-14T12:00:24.161Z
STOP_TIME 2010-05-16T11:55:28.120Z
MISSION_NAME INTERNATIONAL ROSETTA MISSION
MISSION_START_DATE 1995-03-01T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME CALIBRATION
TARGET_TYPE CALIBRATION
INSTRUMENT_HOST_ID RO
INSTRUMENT_NAME STANDARD RADIATION ENVIRONMENT MONITOR
INSTRUMENT_ID SREM
INSTRUMENT_TYPE PARTICLE DETECTOR
NODE_NAME Small Bodies
ARCHIVE_STATUS LOCALLY ARCHIVED
CONFIDENCE_LEVEL_NOTE
All data have been reviewed by the SREM team to check for data set completeness and screened for non-physical values such as negative energy. No obvious errors have been found in the data at this time. Data have also been passed through two Rosetta independent science reviews, and all items raised have been addressed.
CITATION_DESCRIPTION H. Evans, P. Nieminen, I. Sandberg, I. Daglis, and M. Taylor, ROSETTA-ORBITER X SREM 2 CRUISE 5 V1.0, RO-X-SREM-2-CR5-V1.0, ESA Planetary Science Archive and NASA Planetary Data System, 2020.
ABSTRACT_TEXT This data set contains count rates (1/s) as measured by the Standard Radiation Environment Monitor (SREM) instrument on the Rosetta spacecraft, along with their standard deviations. These are CODMAC Level 2 Experiment Data Record data, and provide a measure of the radiation in the spacecraft environment during the CRUISE 5 mission phase.
PRODUCER_FULL_NAME M. BARTHELEMY, F. VALLEJO, D. HEATHER
SEARCH/ACCESS DATA
  • SBN Comet Website