The Parker Solar Probe, PSP, Digital Fields Board, DFB, is responsible for conditioning, digitization, and processing signals from the five voltage sensors and four search coil magnetometers, SCM, over a frequency range from DC to approximately 60 kHz, as well as production of a calibration signal delivered to the SCM. These nine analog inputs are processed by the DFB into twenty five digital data streams, which are then used to produce a range of time domain and spectral domain data products.
Version:2.3.1
The Parker Solar Probe, PSP, Digital Fields Board, DFB, is responsible for conditioning, digitization, and processing signals from the five voltage sensors and four search coil magnetometers, SCM, over a frequency range from DC to approximately 60 kHz, as well as production of a calibration signal delivered to the SCM. These nine analog inputs are processed by the DFB into twenty five digital data streams, which are then used to produce a range of time domain and spectral domain data products.
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | ProjectScientist | spase://SMWG/Person/Nicola.J.Fox | |||
2. | PrincipalInvestigator | spase://SMWG/Person/Stuart.D.Bale | |||
3. | MetadataContact | spase://SMWG/Person/Lee.Frost.Bargatze |
NSSDC Master Catalog Listing for the Parker Solar Probe FIELDS Suite, NSSDCA/COSPAR ID: 2018-065A-01