Data Set Information
DATA_SET_NAME JUNO JUPITER SRU COUNT RATE TABLE 5 L2 V1.0
DATA_SET_ID JNO-J-SRU-COUNTRATE-TABLE-5-L2-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION
Data Set Overview : This data set contains count rate tables derived from the Juno Stellar Reference Unit (SRU) EDR images. This data set uses the Committee on Data Management and Computation (CODMAC) data level numbering system. The SRU count rate tables are considered Level 5 or Derived Data (equivalent to NASA Level 1C).  Processing : SRU count rate tables are produced in '.CSV' format and consist of comma-delimited values. Data :  SRU count rate tables (CRTs) contain derived electron count rates from  a series of SRU images acquired during an orbit. The process by which  these are derived is explained in the Software Interface Specification  (SIS): Stellar Reference Unit Standard Data Products. Typically these SRU  images are taken near perijove. Image processing includes geometric  correction, star identification and removal, hot pixel removal, and count  rate detection. One of two methods of count rate quantification is used,  depending on the noise level observed in the image. Details of this  processing are described in the SIS. One count rate table (CRT) will be produced for each orbit. Within one  orbit's table, each row will represent the derived count rate from  one SRU image. The count rate values are derived from one of the two  measurement techniques described in the SIS, indicated by a valid value  in either column 4 or 5. The measurement technique will be chosen based  on the overall radiation-induced noise level of that image.  There are six fields in the table. The columns are as follows: SCET (UTC)  corresponding to midpoint of SRU image exposure; SCLK corresponding to  midpoint of SRU image exposure (following conversion from the native  format provided in the Event Verification Record (EVR) which telemeters  the SRU-generated image time tag); Identification number of the SRU that  the image was taken with; Detected count rate ('cluster' counts per  square cm of CCD area per second), if valid; Derived rate of deposited  noise signal ('DN' per pixel per second), if valid; Derived count rate  per square cm of CCD area per second using one of the previous methods  that is valid. Column 4 or 5 will have a value of 1.0E-31 if that  measurement technique is not valid; in that case the other column will  have a valid value. Each table product has two parts: the table itself with the extension  of 'CSV' and a detached label with an extension of 'LBL'.  Refer to the Stellar Reference Unit Standard Data Products Software  Interface Specification (SIS) for further details on these data products.
DATA_SET_RELEASE_DATE 3000-01-01T00:00:00.000Z
START_TIME 2016-01-01T12:00:00.000Z
STOP_TIME N/A (ongoing)
MISSION_NAME JUNO
MISSION_START_DATE 2011-08-05T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME JUPITER
TARGET_TYPE PLANET
INSTRUMENT_HOST_ID JNO
INSTRUMENT_NAME STELLAR REFERENCE UNIT
INSTRUMENT_ID SRU
INSTRUMENT_TYPE CAMERA
NODE_NAME Imaging
ARCHIVE_STATUS PRE PEER REVIEW
CONFIDENCE_LEVEL_NOTE
NULL
CITATION_DESCRIPTION Daubar, I., JUNO JUPITER SRU COUNT RATE TABLE 5 L2 V1.0, JNO-J-SRU-COUNTRATE-TABLE-5-L2-V1.0, NASA Planetary Data System, 2022. https://doi.org/10.17189/649d-ch52
ABSTRACT_TEXT NULL
PRODUCER_FULL_NAME INGRID DAUBAR
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