From 72806b1a2e6e04ab13afad9ac945571b9acb5131 Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Thu, 10 Mar 2016 18:34:36 +0100 Subject: [PATCH] work --- NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp.xml | 269 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_.xml | 269 ----------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp.xml | 269 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp_.xml | 273 --------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- 4 files changed, 538 insertions(+), 542 deletions(-) create mode 100644 NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp.xml delete mode 100644 NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_.xml create mode 100644 NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp.xml delete mode 100644 NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp_.xml diff --git a/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp.xml b/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp.xml new file mode 100644 index 0000000..2f28ba6 --- /dev/null +++ b/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp.xml @@ -0,0 +1,269 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp + + prime parameters + Cluster 1 Prime Parameter CIS data + 2015-10-19T09:53:45Z + 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 Rumba Cluster Ion Spectrometry (CIS) + http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02 + This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument. + + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + AMDA at CDPP + http://amda.cdpp.eu + + NetCDF + NASA, Prof. Henri Reme + + CSDS-CNES + Calibrated + Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data + Calibrated + 1 + spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-CODIF + IonComposition + + + 2001-01-10T14:54:04Z + 2012-11-29T14:30:14Z + + 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 + + h+ density + c1_h_dens + Cluster II Rumba Prime Parameter Cluster Ion Spectrometry CODIF H number density at spin time resolution + phys.density;phys.atmol.ionStage + PT4S + cm^-3 + 1.0e6>m^-3 + + TimeSeries + H n(HIA) + 0.0010 + 1000 + + 0.0010 + 1000 + -1.0000e+31 + + Ion + Scalar + NumberDensity + + + + o+ density + c1_o_dens + Cluster II Rumba Prime Parameter Cluster Ion Spectrometry CODIF O number density at spin time resolution + phys.density;phys.atmol.ionStage + PT4S + cm^-3 + 1.0e6>m^-3 + + TimeSeries + O n(HIA) + 0.0010 + 1000 + + 0.0010 + 1000 + -1.0000e+31 + + Ion + Scalar + NumberDensity + + + + h+ v_gse + c1_h_v + Cluster II Rumba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution + phys.veloc;phys.atmol.ionStage + PT4S + km/s + 1.0e3>m s^-1 + + Cartesian + GSE + + + TimeSeries + -2000 + 2000 + + + 3 + + vx + Component.I + 1 + c1_h_v(0) + + + vy + Component.J + 2 + c1_h_v(1) + + + vz + Component.K + 3 + c1_h_v(2) + + + -2000 + 2000 + -1.0000e+31 + + Ion + Vector + Velocity + + + + h+ v_gsm + c1_h_v_gsm + Cluster II Rumba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution + phys.veloc;phys.atmol.ionStage + PT4S + km/s + 1.0e3>m s^-1 + + Cartesian + GSM + + + TimeSeries + -2000 + 2000 + + + 3 + + vx + Component.I + 1 + c1_h_v_gsm(0) + + + vy + Component.J + 2 + c1_h_v_gsm(1) + + + vz + Component.K + 3 + c1_h_v_gsm(2) + + + -2000 + 2000 + -1.0000e+31 + + Ion + Vector + Velocity + + + + h+ |v| + c1_h_vtot + Cluster Rumba Fluxgate Magnetometer Velocity magnitude at spin time resolution + phys.veloc;phys.atmol.ionStage + PT4S + nT + + TimeSeries + + -1.0000e+31 + + Ion + Magnitude + Velocity + + + + h+ temperature + c1_h_t + phys.temperature;phys.atmol.ionStage + PT4S + eV + + TimeSeries + + + 2 + + t_para + Parallel + 1 + c1_h_t(0) + -1.0000e+31 + + T(HIA)_par + + + + t_perp + Perpendicular + 2 + c1_h_t(1) + -1.0000e+31 + + T(HIA)_perp + + + + + Ion + Array + Temperature + + + + diff --git a/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_.xml b/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_.xml deleted file mode 100644 index df8452b..0000000 --- a/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_.xml +++ /dev/null @@ -1,269 +0,0 @@ - - - 2.2.6 - - spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_ - - CODIF prime parametres - Cluster 1 Prime Parameter CIS data - 2015-10-19T09:53:45Z - 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 Rumba Cluster Ion Spectrometry (CIS) - http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02 - This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument. - - - - spase://SMWG/Repository/CDPP/AMDA - Online - Open - - AMDA at CDPP - http://amda.cdpp.eu - - NetCDF - NASA, Prof. Henri Reme - - CSDS-CNES - Calibrated - Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data - Calibrated - 1 - spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-CODIF - IonComposition - - - 1970-01-01T00:00:00Z - 1970-01-01T00:00:00Z - - 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 - - H Density - c1_h_dens - Cluster II Rumba Prime Parameter Cluster Ion Spectrometry CODIF H number density at spin time resolution - phys.density;phys.atmol.ionStage - PT4S - cm^-3 - 1.0e6>m^-3 - - TimeSeries - H n(HIA) - 0.0010 - 1000 - - 0.0010 - 1000 - -1.0000e+31 - - Ion - Scalar - NumberDensity - - - - O Density - c1_o_dens - Cluster II Rumba Prime Parameter Cluster Ion Spectrometry CODIF O number density at spin time resolution - phys.density;phys.atmol.ionStage - PT4S - cm^-3 - 1.0e6>m^-3 - - TimeSeries - O n(HIA) - 0.0010 - 1000 - - 0.0010 - 1000 - -1.0000e+31 - - Ion - Scalar - NumberDensity - - - - H Velocity GSE - c1_h_v - Cluster II Rumba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution - phys.veloc;phys.atmol.ionStage - PT4S - km/s - 1.0e3>m s^-1 - - Cartesian - GSE - - - TimeSeries - -2000 - 2000 - - - 3 - - Vx GSE - Component.I - 1 - c1_h_v(0) - - - Vy GSE - Component.J - 2 - c1_h_v(1) - - - Vz GSE - Component.K - 3 - c1_h_v(2) - - - -2000 - 2000 - -1.0000e+31 - - Ion - Vector - Velocity - - - - H Velocity GSM - c1_h_v_gsm - Cluster II Rumba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution - phys.veloc;phys.atmol.ionStage - PT4S - km/s - 1.0e3>m s^-1 - - Cartesian - GSM - - - TimeSeries - -2000 - 2000 - - - 3 - - Vx GSM - Component.I - 1 - c1_h_v_gsm(0) - - - Vy GSM - Component.J - 2 - c1_h_v_gsm(1) - - - Vz GSM - Component.K - 3 - c1_h_v_gsm(2) - - - -2000 - 2000 - -1.0000e+31 - - Ion - Vector - Velocity - - - - Velocity magnitude - c1_h_vtot - Cluster Rumba Fluxgate Magnetometer Velocity magnitude at spin time resolution - phys.veloc;phys.atmol.ionStage - PT4S - nT - - TimeSeries - - -1.0000e+31 - - Ion - Magnitude - Velocity - - - - Temperature - c1_h_t - phys.temperature;phys.atmol.ionStage - PT4S - eV - - TimeSeries - - - 2 - - Hot Ion Parallel Temperature - Parallel - 1 - c1_h_t(0) - -1.0000e+31 - - T(HIA)_par - - - - Hot Ion Perpendicular Temperature - Perpendicular - 2 - c1_h_t(1) - -1.0000e+31 - - T(HIA)_perp - - - - - Ion - Array - Temperature - - - - diff --git a/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp.xml b/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp.xml new file mode 100644 index 0000000..328f70c --- /dev/null +++ b/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp.xml @@ -0,0 +1,269 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp + + prime parameters + 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/Repository/CDPP/AMDA + Online + Open + + AMDA at CDPP + http://amda.cdpp.eu + + NetCDF + NASA, Prof. Henri Reme + + CSDS-CNES + Calibrated + Cluster II Samba Prime Parameter Cluster Ion Spectrometry (CIS) Data + Calibrated + 1 + spase://CDPP/Instrument/AMDA/Cluster-Samba/CIS-CODIF + IonComposition + + + 2001-01-09T17:50:48Z + 2009-12-15T14:42:52Z + + 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 + + h+ density + c3_h_dens + Cluster II Samba Prime Parameter Cluster Ion Spectrometry CODIF H number density at spin time resolution + phys.density;phys.atmol.ionStage + PT4S + cm^-3 + 1.0e6>m^-3 + + TimeSeries + H n(HIA) + 0.0010 + 1000 + + 0.0010 + 1000 + -1.0000e+31 + + Ion + Scalar + NumberDensity + + + + o+ density + c3_o_dens + Cluster II Samba Prime Parameter Cluster Ion Spectrometry CODIF O number density at spin time resolution + phys.density;phys.atmol.ionStage + PT4S + cm^-3 + 1.0e6>m^-3 + + TimeSeries + O n(HIA) + 0.0010 + 1000 + + 0.0010 + 1000 + -1.0000e+31 + + Ion + Scalar + NumberDensity + + + + h+ v_gse + c3_h_v + Cluster II Samba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution + phys.veloc;phys.atmol.ionStage + PT4S + km/s + 1.0e3>m s^-1 + + Cartesian + GSE + + + TimeSeries + -2000 + 2000 + + + 3 + + vx + Component.I + 1 + c3_h_v(0) + + + vy + Component.J + 2 + c3_h_v(1) + + + vz + Component.K + 3 + c3_h_v(2) + + + -2000 + 2000 + -1.0000e+31 + + Ion + Vector + Velocity + + + + h+ v_gsm + c3_h_v_gsm + Cluster II Samba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution + phys.veloc;phys.atmol.ionStage + PT4S + km/s + 1.0e3>m s^-1 + + Cartesian + GSM + + + TimeSeries + -2000 + 2000 + + + 3 + + vx + Component.I + 1 + c3_h_v_gsm(0) + + + vy + Component.J + 2 + c3_h_v_gsm(1) + + + vz + Component.K + 3 + c3_h_v_gsm(2) + + + -2000 + 2000 + -1.0000e+31 + + Ion + Vector + Velocity + + + + h+ |v| + c3_h_vtot + Cluster Samba Fluxgate Magnetometer Velocity magnitude at spin time resolution + phys.veloc;phys.atmol.ionStage + PT4S + nT + + TimeSeries + + -1.0000e+31 + + Ion + Magnitude + Velocity + + + + h+ temperature + c3_h_t + phys.temperature;phys.atmol.ionStage + PT4S + eV + + TimeSeries + + + 2 + + t_para + Parallel + 1 + c3_h_t(0) + -1.0000e+31 + + T(HIA)_par + + + + t_perp + Perpendicular + 2 + c3_h_t(1) + -1.0000e+31 + + T(HIA)_perp + + + + + Ion + Array + Temperature + + + + diff --git a/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp_.xml b/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp_.xml deleted file mode 100644 index 710d9e8..0000000 --- a/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp_.xml +++ /dev/null @@ -1,273 +0,0 @@ - - - 2.2.6 - - spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/CIS-CODIF/clust3-cis-prp_ - - Cluster II Samba Prime Parameter Cluster Ion Spectrometry (CIS) CODIF Data - 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 - - CSDS-CNES - Calibrated - Cluster II Samba Prime Parameter Cluster Ion Spectrometry (CIS) Data - Calibrated - 1 - spase://CDPP/Instrument/AMDA/Cluster-Samba/CIS - IonComposition - - - 1970-01-01T00:00:00Z - 1970-01-01T00:00:00Z - - 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 - - H Density - c3_h_dens - Cluster II Samba Prime Parameter Cluster Ion Spectrometry CODIF H number density at spin time resolution - phys.density;phys.atmol.ionStage - PT4S - cm^-3 - 1.0e6>m^-3 - - TimeSeries - H n(HIA) - 0.0010 - 1000 - - 0.0010 - 1000 - -1.0000e+31 - - Ion - Scalar - NumberDensity - - - - O Density - c3_o_dens - Cluster II Samba Prime Parameter Cluster Ion Spectrometry CODIF O number density at spin time resolution - phys.density;phys.atmol.ionStage - PT4S - cm^-3 - 1.0e6>m^-3 - - TimeSeries - O n(HIA) - 0.0010 - 1000 - - 0.0010 - 1000 - -1.0000e+31 - - Ion - Scalar - NumberDensity - - - - H Velocity - c3_h_v - Cluster II Samba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution - phys.veloc;phys.atmol.ionStage - PT4S - km/s - 1.0e3>m s^-1 - - Cartesian - GSE - - - TimeSeries - -2000 - 2000 - - - 3 - - Vx GSE - Component.I - 1 - c3_h_v(0) - - - Vy GSE - Component.J - 2 - c3_h_v(1) - - - Vz GSE - Component.K - 3 - c3_h_v(2) - - - -2000 - 2000 - -1.0000e+31 - - Ion - Vector - Velocity - - - - H Velocity - c3_h_v_gsm - Cluster II Samba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution - phys.veloc;phys.atmol.ionStage - PT4S - km/s - 1.0e3>m s^-1 - - Cartesian - GSM - - - TimeSeries - -2000 - 2000 - - - 3 - - Vx GSM - Component.I - 1 - c3_h_v_gsm(0) - - - Vy GSM - Component.J - 2 - c3_h_v_gsm(1) - - - Vz GSM - Component.K - 3 - c3_h_v_gsm(2) - - - -2000 - 2000 - -1.0000e+31 - - Ion - Vector - Velocity - - - - Velocity magnitude - c3_h_vtot - Cluster Samba Fluxgate Magnetometer Velocity magnitude at spin time resolution - phys.veloc;phys.atmol.ionStage - PT4S - nT - - TimeSeries - - -1.0000e+31 - - Ion - Magnitude - Velocity - - - - Temperature - c3_h_t - phys.temperature;phys.atmol.ionStage - PT4S - eV - - TimeSeries - - - 2 - - Hot Ion Parallel Temperature - Parallel - 1 - c3_h_t(0) - -1.0000e+31 - - T(HIA)_par - - - - Hot Ion Perpendicular Temperature - Perpendicular - 2 - c3_h_t(1) - -1.0000e+31 - - T(HIA)_perp - - - - - Ion - Array - Temperature - - - - -- libgit2 0.21.2