Data Set Information
|
DATA_SET_NAME |
ROSETTA-ORBITER 67P SREM 2 ESCORT 2
MTP015 V1.0
|
DATA_SET_ID |
RO-X-SREM-2-ESC2-MTP015-V1.0
|
NSSDC_DATA_SET_ID |
|
DATA_SET_TERSE_DESCRIPTION |
This data set contains SREM count rates
(1/s), converted from the equivalent
SREM Level 0 CDF products.
|
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 |
2015-04-08T12:00:33.783Z
|
STOP_TIME |
2015-05-02T08:01:25.984Z
|
MISSION_NAME |
INTERNATIONAL ROSETTA MISSION
|
MISSION_START_DATE |
1995-03-01T12:00:00.000Z
|
MISSION_STOP_DATE |
N/A (ongoing)
|
TARGET_NAME |
67P/CHURYUMOV-GERASIMENKO 1 (1969 R1)
|
TARGET_TYPE |
COMET
|
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 67P SREM 2 ESCORT 2
MTP015 V1.0,
RO-X-SREM-2-ESC2-MTP015-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. The primary target is comet 67P/Churyumov-Gerasimenko.
These are CODMAC Level 2 Experiment Data Record data, and provide a
measure of the radiation in the spacecraft environment during the
Medium Term Plan 15 period of the ESCORT 2 mission phase.
|
PRODUCER_FULL_NAME |
M. BARTHELEMY, F. VALLEJO, D. HEATHER
|
SEARCH/ACCESS DATA |
SBN Comet Website
|