2.3.1 spase://CNES/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp prime parameters : protons Cluster 2 Prime Parameter RAPID Data 2015-10-19T15:51:46Z The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. For more details of the Cluster mission, the spacecraft, and its instruments, see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159, and the included article RAPID: The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which this information was obtained. spase://SMWG/Person/Peter.W.Daly TechnicalContact NSSDC Master Catalog listing for Cluster II Salsa Research with Adaptive Particle Imaging Detectors (RAPID) http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06 This site provides information concerning the Cluster II Salsa Research with Adaptive Particle Imaging Detectors Instrument. spase://SMWG/Repository/CNES/CDPP-AMDA Online Restricted AMDA at CDPP http://amda.cdpp.eu NetCDF NASA, Dr. Berend Wilken CSA Calibrated Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data Calibrated spase://CNES/Instrument/CDPP-AMDA/Cluster2/RAPID EnergeticParticles 2001-01-01T00:00:03Z 2006-12-31T23:59:58Z PT4S Earth.Magnetosheath Earth.Magnetosphere Earth.Magnetosphere.Magnetotail Earth.Magnetosphere.Main Earth.Magnetosphere.Polar Earth.Magnetosphere.RadiationBelt Earth.NearSurface.AuroralRegion Earth.NearSurface.Ionosphere Earth.NearSurface.Plasmasphere Earth.NearSurface.PolarCap Heliosphere.NearEarth 4 second magnetosphere auroral region polar cap cusp bow shock solar wind magnetosheath Cluster magnetotail lobe diff flux c2_rap_p Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution phys.flux.density;phys.count;phys.atmol.ionStage PT4S 1/cm^2_sr_s_keV Spectrogram -1.0000e+31 Proton Scalar EnergyFlux