2.3.1 spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/DFB Parker Solar Probe, PSP, FIELDS Suite, Digital Fields Board, DFB, Instrument Solar Probe Plus, SPP, FIELDS Suite, Digital Fields Board, DFB, Instrument 2020-03-16T12:34:56.789Z 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. Please acknowledge NASA, Stuart D. Bale, the PSP FIELDS Instrument Suite Principal Investigator, and Nicola J. Fox, the PSP Project Scientist. spase://SMWG/Person/Nicola.J.Fox ProjectScientist spase://SMWG/Person/Stuart.D.Bale PrincipalInvestigator spase://SMWG/Person/Lee.Frost.Bargatze MetadataContact Parker Solar Probe FIELDS Suite NSSDCA Master Catalog Listing https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2018-065A-01 NSSDC Master Catalog Listing for the Parker Solar Probe FIELDS Suite, NSSDCA/COSPAR ID: 2018-065A-01 Platform Parker Solar Probe Mission 2018-08-12T07:31:00.000Z spase://SMWG/Observatory/ParkerSolarProbe