Data Set Information
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DATA_SET_NAME |
JNO J JED 3 CDR V1.0
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DATA_SET_ID |
JNO-J-JED-3-CDR-V1.0
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NSSDC_DATA_SET_ID |
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DATA_SET_TERSE_DESCRIPTION |
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DATA_SET_DESCRIPTION |
Data Set Overview : The data set consists of calibrated observations, also known as CDRs. For all the CDR products there is a detached PDS label file that describes the contents of one data file. Each label file will have the same base name as the data file it is describing, with the extension .LBL to denote a label file. The label file defines the start time and end of the observation, product creation time, and the structure of the ASSCI tables. Each data product is identified within the PDS label by a STANDARD_DATA_PRODUCT_ID value, shown in parentheses in the table below. Instrument Overview : The JEDI sensors consists of a 60-mm diameter, hockey puck-like cylinder, in which a start foil and stop foil, wrapped around opposite curved sides of the cylinder, constitute the TOF chamber. The detectors are arranged so that each detector senses the events within a given range of incidence angles. Each of the 6 detector modules is composed of 4 pixels: large and small ion and large and small electron. See the INSTRUMENT.CAT file for more information. Calibration Overview : This data set is calibrated; it provides the instrument team's best available interpretation of the measured data at the time of release. This understanding is evolving and it is expected that the calibration process will change and improve with subsequent releases. Parameters : The timing parameters in the CDRs are identical to those in the EDRs. See JEDI_J_EDR_DS.CAT file for a short description or the JEDI SIS for more detailed information. In addition to the timing parameters and the uncalibrated counts, and calibrated counts per second and intensity spectra, for each data record in the CDR, we include ephemeris attitude and pitch angle information for the convenience of the end user. We also include a subset of the basic rate information so the end user can obtain an understanding of the level of activity in the instrument system as this will affect the instrument performance. The additional quantities are, in brief: : Spacecraft Position - X, Y, and Z in the POS frame (POS : JSE for observations at Jupiter). Planetary Position - Latitude and Longitude in the LOC frame (LOC: IAU_JUPITER for observations at Jupiter). Look Direction - Unit Vector X, Y, and Z of the 'look direction' of the negative of the incident particle velocity vector for each telescope. Pitch Angle (1 column per telescope : 6 columns) - The angle between the incident particle velocity vector and the local magnetic field. which of these values are present depends on the data type, see JEDI SIS for details: SSD0-SSD5 - Number of pulses on the Solid State Energy detector for telescope number 0-5 VEP (Valid Events Processed) - Number of events actually processed by the flight software VEE (Valid Energy Events) - Total number of events in all SSD (Energy) detectors. Start0, Stop0 - Number of pulses on the end of the Start or Stop anode nearest to look direction 0. VTOFXE - Number of valid TOFxE events counted. VTOFXPH - Number of valid TOFxPH events counted. Data : The JUNO JEDI CDR data set products are the same as described in JEDI_J_EDR_DS.CAT.
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DATA_SET_RELEASE_DATE |
2024-06-11T00:00:00.000Z
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START_TIME |
2016-07-06T10:04:14.000Z
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STOP_TIME |
2023-11-23T11:59:58.000Z
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MISSION_NAME |
JUNO
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MISSION_START_DATE |
2011-08-05T12:00:00.000Z
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MISSION_STOP_DATE |
N/A (ongoing)
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TARGET_NAME |
JUPITER
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TARGET_TYPE |
PLANET
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INSTRUMENT_HOST_ID |
JNO
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INSTRUMENT_NAME |
JUPITER ENERGETIC-PARTICLE DETECTOR INSTRUMENT
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INSTRUMENT_ID |
JEDI
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INSTRUMENT_TYPE |
ENERGETIC PARTICLE DETECTOR
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NODE_NAME |
Planetary Plasma Interactions
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ARCHIVE_STATUS |
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CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview : The JUNO JEDI CDR data are, at the present time, calibrated simply by multiplying by a factor, determined for each individual telescope and pixel, which captures the efficiency and geometric factor for that detector. The underlying counts per second rate has not been adjusted for background or instrument saturation effects. These are strictly preliminary calibrations at this time. Review : The JUNO JEDI CDR were reviewed internally by the JEDI team prior to release to the PDS. PDS also performed an external review of the JEDI EDR. Data Coverage and Quality : Data reported are the calibrated data for the time period: 2013-279T00:00:00 through 2014-104T23:59:59 Limitations : The calibrations applied to the data both in terms of efficiency factors and energy descrimination are still preliminary. Instrument team calibration efforts are ongoing.
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CITATION_DESCRIPTION |
B. Mauk (APL), JEDI CALIBRATED (CDR) DATA JNO J JED 3 CDR V1.0, NASA Planetary Data System, 2024, DOI: 10.17189/1519713.
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ABSTRACT_TEXT |
Abstract : This data set consists of the JUNO JEDI (Jupiter Energetic-Particle Detector) calibrated observations, also known as CDRs. The system is made up of 3 instrument subsystems (pucks) aligned in three directions on the spinning JUNO spacecraft. The pucks each have 6 look directions (telescopes) with a time of flight (TOF) and a deposited energy detection (SSD) system. In addition, the pulse height of the signal in the TOF system can be used for energy measurement. The instruments can be operated in a variety of modes, differing in the way they use and combine these measurements. More details are available in the INSTRUMENT.CAT file and the JEDI SIS. The CDRs are organized in files covering one day of spacecraft event time (SCET). There are potentially 10 different files per puck, corresponding to the available data gathering modes: HIERSESP, HIERSISP, HIERSTOFXER, HIERSTOFXPHR, LOERSESP, LOERSISP, LOERSTOFXER, LOERSTOFXPHR, NONPTOFXER, NONPTOFXPHR. Depending on how the pucks are operated, not all data types will be available for all pucks for any particular time range. All the measured quantities present in the uncalibrated data files (EDRs) are present here in three forms: counts per accumulation (the same numbers as in the EDRs), counts per second (this number may be corrected for instrument saturation and background), intensity (counts per second per steradian per cm2 per keV). Additional support quantities are also included for the convenience or enlightenment of the end user.
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PRODUCER_FULL_NAME |
BARRY MAUK
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SEARCH/ACCESS DATA |
Planetary Plasma Interactions Website
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