2.2.6 spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad HIA pad Cluster 3 Prime Parameter CIS data 2015-10-19T15:51:45Z This instrument (CIS: Cluster Ion Spectrometry) is capable of obtaining full 3D ion distributions with high time resolution (in one spacecraft spin) and mass-per-charge resolution. The experiment consists of two different instruments, a Hot Ion Analyzer (HIA) and a time-of-flight Ion Composition and Distribution Function analyzer (CODIF). Extensive on-board processing is done, within its dual-processor Data Processing System (DPS). CODIF determines the distributions of the major ion species with energies from spacecraft potential to 40 KeV/charge with an angular resolution of 22.5 x 10.25 degrees and with two different sensitivities. The CODIF instrument uses electrostatic deflection to select by energy per charge, with subsequent time-of-flight analysis. The sensor primarily covers the energy range 0.02-40 KeV/charge, but with additional pre-acceleration for energies below 25 eV/charge, the range is extended to energies as low as the spacecraft potential. The HIA does not measure mass, but extends the dynamic range to the highest ion fluxes, and has angular resolution capability of 5.6 x 5.6 degrees for ion-beam and solar-wind measurements. The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. 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 The Cluster Ion Spectrometry Experiment, by H. Reme et al., from which this information was obtained. NASA, Prof. Henri Reme, European Space Agency spase://SMWG/Person/Henri.Reme PrincipalInvestigator spase://SMWG/Person/Elena.Budnik TechnicalContact NSSDC Master Catalog listing for Cluster II Samba Cluster Ion Spectrometry (CIS) http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02 This site provides information concerning the Cluster II Samba Cluster Ion Spectrometry Instrument. spase://SMWG/Observatory/Cluster-Samba ObservedBy spase://SMWG/Repository/CDPP/AMDA Online Open AMDA at CDPP http://amda.cdpp.eu NetCDF NASA, Prof. Henri Reme IRAP Calibrated Cluster II Samba Prime Parameter Cluster Ion Spectrometry (CIS) Data Calibrated 1 spase://CDPP/Instrument/AMDA/Cluster-Samba/CIS IonComposition 2001-01-31T01:02:10Z 2009-11-11T08:17:05Z 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 Pitch angle distribution c3_hia_pad pos.posAng PT4S cnts/(cm2 s sr Kev) Spectrogram Other Pitch angle distribution : sum over all energies c3_hia_pad_angle pos.posAng PT4S cnts/(cm2 s sr Kev) Spectrogram Other Energy distribution : sum over all pitch angles c3_hia_pad_energy pos.posAng PT4S cnts/(cm2 s sr Kev) Spectrogram Other