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PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage,...
PSP FIELDS Digital Fields Board (DFB), XXX ⨯ YYY cross spectra data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe... -
PSP FIELDS Digital Fields Board (DFB) Searchcoil Magnetometer, SCM, Burst...
PSP FIELDS Digital Fields Board (DFB), Differential Voltage data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe... -
PSP FIELDS Digital Fields Board (DFB) Differential Voltage Burst Waveform,...
PSP FIELDS Digital Fields Board (DFB), Differential Voltage data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe... -
PSP FIELDS Digital Fields Board (DFB) AC-coupled Searchcoil Magnetometer,...
PSP FIELDS Digital Fields Board, DFB, SCMulfhg data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see... -
PSP FIELDS Digital Fields Board (DFB) AC-coupled Searchcoil Magnetometer,...
PSP FIELDS Digital Fields Board, DFB, SCMumfhg data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see... -
PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V3-V4...
PSP FIELDS Digital Fields Board, DFB, dV34 data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see... -
PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V1-V2...
PSP FIELDS Digital Fields Board, DFB, dV12 data: The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see... -
PSP FIELDS Antenna Electronics Board (AEB) Housing Keeping Data
PSP FIELDS Antenna Electronics Board (AEB) Housing Keeping Data. -
ACE Wind Genesis IMP 8 Impact Parameters
ACE Wind Genesis IMP 8 - Earth impact parameters (IP). IP is the minimal distance by which a plasma element seen at one body misses being seen by a second body. Cf.... -
ISEE 3 - IMP 8 Impact Parameters
ISEE 3 - IMP 8 - Earth impact parameters (IP). IP is the minimal distance by which a plasma element seen at one body misses being seen by a second body. Cf.... -
PUNCH Level 3 WFI-3 Polarized F-Corona Model
PUNCH Level 3 polarized F-corona model derived from Wide Field Imager 3 (WFI-3) observations and represented in the PUNCH mosaic frame as an MZP (Minus, Zero, and Plus)... -
PUNCH Level 3 WFI-2 Polarized F-Corona Model
PUNCH Level 3 polarized F-corona model derived from Wide Field Imager 2 (WFI-2) observations and represented in the PUNCH mosaic frame as an MZP (Minus, Zero, and Plus)... -
PUNCH Level 3 WFI-1 Polarized F-Corona Model
PUNCH Level 3 polarized F-corona model derived from Wide Field Imager 1 (WFI-1) observations and represented in the PUNCH mosaic frame as an MZP (Minus, Zero, and Plus)... -
Polar Visible Imaging System (VIS) Low Resolution Camera Images, Calibrated,...
Instrument Functional Description: The VIS Instrument is a Set of three Low Light Level Cameras. Two of these Cameras share primary and some secondary Optics and are designed to... -
Polar Visible Imaging System (VIS) Earth Camera Images, Calibrated (E0), 4 min Data
Instrument Functional Description: The VIS Instrument is a Set of three Low Light Level Cameras. Two of these Cameras share primary and some secondary Optics and are designed to... -
Polar TIMAS K2 Mass Spectral Data
Mass spectra count rates for survey purposes only from the POLAR TIMAS instrument. The mass spectral data product consists of 64 mass steps covering the full detector range, for... -
Polar TIMAS K1 Key Parameter data
H+, O+, He+ and He++ number fluxes for survey purposes only Reference:E.G. Shelley et al., The Toroidal Imaging Mass-Angle Spectrograph (TIMAS) for the Polar Mission, Sp. Sci.... -
Polar TIMAS H2 Level 1 Ion Upflowing Fluxes Data
H+, O+, He+ and He++ upflowing fluxes and statistical uncertainties processed by the TIMAS science team.These data were used in preparing several papers, see Information URLs.... -
Polar TIMAS H0 High-resolution Level 1 Data
Mass resolved ion energy angle spectra covering nearly the full 4pi solid angle and the energy range 15 eV/q to 33 eV/q. H+, O+, He+ and He++ number fluxes and statistical... -
Polar Plasma Wave Instrument (PWI), Wideband Receiver (WBR) 4.016...
PWI>Plasma Wave Instrument Reference: Gurnett, D.A. et al, The Polar Plasma Wave Instrument, Space Science Reviews, Vol. 71, pp. 597-622, 1995. donald-gurnett@uiowa.edu An...