2.3.0 spase://ESA/NumericalData/Cluster-Rumba/RAPID/PrimeParameter/PT4S Cluster-Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data Cluster 1 Prime Parameter RAPID Data 2021-04-27T17:52:14Z 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. NASA, Dr. Berend Wilken, European Space Agency spase://SMWG/Person/Berend.Wilken PrincipalInvestigator spase://SMWG/Person/Joseph.F.Fennell CoInvestigator spase://SMWG/Person/J.Bernard.Blake CoInvestigator spase://SMWG/Person/Finn.Soraas CoInvestigator spase://SMWG/Person/Bengt.K.G.Hultqvist CoInvestigator spase://SMWG/Person/Richard.D.Belian CoInvestigator spase://SMWG/Person/Theodore.Allan.Fritz CoInvestigator spase://SMWG/Person/Axel.Korth CoInvestigator spase://SMWG/Person/Hans.Borg CoInvestigator spase://SMWG/Person/Pekka.J.Tanskanen CoInvestigator spase://SMWG/Person/Gerhard.Kremser CoInvestigator spase://SMWG/Person/David.S.Hall CoInvestigator spase://SMWG/Person/Stein.Ullaland CoInvestigator spase://SMWG/Person/Daniel.N.Baker CoInvestigator spase://SMWG/Person/Fritz.O.Gliem CoInvestigator spase://SMWG/Person/Peter.W.Daly CoInvestigator spase://SMWG/Person/Susan.M.P.McKenna-Lawlor CoInvestigator spase://SMWG/Person/Stefano.A.Livi CoInvestigator spase://SMWG/Person/Kalevi.Mursula CoInvestigator spase://SMWG/Person/Manuel.Grande CoInvestigator spase://SMWG/Person/James.M.Weygand MetadataContact NSSDC Master Catalog listing for Cluster II Rumba Research with Adaptive Particle Imaging Detectors (RAPID) https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2000-045A-06 This site provides information concerning the Cluster II Rumba Research with Adaptive Particle Imaging Detectors Instrument. spase://SMWG/Observatory/Cluster-Rumba ObservedBy spase://VMO/NumericalData/Cluster2-Rumba/RAPID/PrimeParameter/4S spase://VMO/NumericalData/Cluster-Rumba/RAPID/PrimeParameter/4S spase://VSPO/NumericalData/Cluster-Rumba/RAPID/PrimeParameter/PT4S spase://SMWG/Repository/NASA/GSFC/SPDF/CDAWeb Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/cluster/c1/pp/rap/ Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) data HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/cluster/c1/pp/rap/ In CDF via HTTP from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=C1_PP_RAP&index=sp_phys C1_PP_RAP CDF NASA, Dr. Berend Wilken spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi C1_PP_RAP Web Service to this product using the HAPI interface. CSV NASA, Dr. Berend Wilken Calibrated Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data Calibrated 1 spase://SMWG/Instrument/Cluster-Rumba/RAPID EnergeticParticles 2000-12-09T00:00:00 -P3M Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000 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 Half Sample Time Interval Half_interval__C1_PP_RAP Half width of measurement interval PT4S ms 1.0e-3>s -1.0000e+31 Other Universal Time Epoch__C1_PP_RAP Universal Time in data cell: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000. PT4S ms 1.0e-3>s Epoch -1.0000e+31 Temporal Status Status__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors status at spin time resolution PT4S 0 255 255 Other Electron Flux (E>50 keV) J_e_lo__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux for electrons with energies greater than 50 keV at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(e,lo) 100 10000000 0 2.0000e+9 -1.0000e+31 Electron Scalar EnergyFlux Electron Flux (E>95 keV) J_e_hi__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux for electrons with energies greater than 95 keV at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(e,hi) 100 10000000 0 2.0000e+9 -1.0000e+31 Electron Scalar EnergyFlux Proton Flux (E>28 keV) J_p_lo__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors proton flux for protons with energies greater than 28 keV at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(p,lo) 100 10000000 0 2.0000e+9 -1.0000e+31 Proton Scalar EnergyFlux Proton Flux (E>92 keV) J_p_hi__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors proton flux for protons with energies greater than 92 keV at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(p,lo) 100 10000000 0 2.0000e+9 -1.0000e+31 Proton Scalar EnergyFlux Helium Flux (E>138 kev) J_He_lo__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors helium flux for helium with energies greater than 138 keV at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(He,lo) 100 10000000 0 2.0000e+9 -1.0000e+31 AlphaParticle Scalar EnergyFlux Helium Flux (E>172 kev) J_He_hi__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors helium flux for helium with energies greater than 172 keV at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(He,hi) 100 10000000 0 2.0000e+9 -1.0000e+31 AlphaParticle Scalar EnergyFlux Ion Flux (m>4, E>84 kev) J_hvy_lo__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors ion flux for ions with energies greater than 84 keV and atomic mass greater than 4 at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(m>4,lo) 100 10000000 0 2.0000e+9 -1.0000e+31 Ion Scalar EnergyFlux Ion Flux (m>4, E>414 kev) J_hvy_hi__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors ion flux for ions with energies greater than 414 keV and atomic mass greater than 4 at spin time resolution PT4S 1/(cm^2 s sr) 1.e4>m^-2 s^-1 sr^-1 J(m>4,hi) 100 10000000 0 2.0000e+9 -1.0000e+31 Ion Scalar EnergyFlux Field-Aligned Electron Anisotropy A_e_par__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors field-aligned electron anisotropy at spin time resolution PT4S A(e) -1 1 -1 1 -1.0000e+31 Other Field-Aligned Proton Anisotropy A_p_par__C1_PP_RAP Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors field-aligned proton anisotropy at spin time resolution PT4S A(e) -1 1 -1 1 -1.0000e+31 Other