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Mars Science Laboratory (MSL), Radiation Assessment Detector (RAD), Level 1...
The Mars Science Laboratory (MSL) Radiation Assessment Detector (RAD) Level 1 observational counter data product contains time-tagged instrument housekeeping and observation... -
IMP 8 Cosmic Ray Nuclear Composition (CRNC) 15-min PHA and coincidence mode counts
This 15-min-resolution data set consists of 5 count rates from the Low Energy Telescope, 8 count rates for the main telescope (MT), 4 counts of pulse height analyzed events in... -
IMP 8 CPME 5-min rates and fluxes
IMP 8 CPME electron, proton, alpha particle and Z>2 count rates and fluxes at 5-min and lower resolutions -
Mars Science Laboratory (MSL), Radiation Assessment Detector (RAD), Level 2...
Mars Science Laboratory Radiation Assessment Detector (RAD) Level 2 observation data for Mars surface operations. The record contains quality-filtered variables, identified by... -
IMP 8 CRNC Hourly Count Rates
Hourly count rates from U.Chi/UNH IMP 8 experiment, 9 each proton and alpha channels 11-95 MeV/n, 3 electron channels 0.7-50 MeV, 2 each CNO and Z>8 channels -
Mars Science Laboratory (MSL), Radiation Assessment Detector (RAD), Level 1...
The Mars Science Laboratory (MSL) Radiation Assessment Detector (RAD) Level 1 observational counter data product contains time-tagged instrument housekeeping and observation... -
Mars Science Laboratory (MSL), Radiation Assessment Detector (RAD), Level 2...
Mars Science Laboratory Radiation Assessment Detector (RAD) Level 2 observation data for Mars surface operations. The record contains quality-filtered variables, identified by... -
Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) High Flux...
This Data Set contains 10 min Average Spin-Averaged and Sectored Counting Rate based Nominal Fluxes of Energetic Proton and Heavier Nuclei from the Ulysses COSPIN High Flux... -
TRACERS 1 Analyzer of Cusp Electrons (ACE) Differential Energy Flux and...
The ACE L2 data consist of raw measured counts and calibrated differential energy fluxes as a function of anode angle and calibrated energy. Counts are accumulated in 21...