diff --git a/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml b/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml index 5050726..e67b639 100644 --- a/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml +++ b/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml @@ -4,19 +4,16 @@ spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad - pitch angle distribution - + PAD + 2D Pitch-Angle/Energy distribution 2015-10-19T10:51:45Z - 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 + Pitch-angle distributions (PADs) are given in particle flux units, as a function of the particle energy and pitch-angle (2D distributions), and their resolution is in 16 angular sectors covering the pitch angle range from 0° to 180°. + PADs are calculated for HIA magnetospheric modes. The dataset is provided with 31 energy bins resolution + Principal Investigator: Dr. Iannis Dandouras - spase://SMWG/Person/Henri.Reme + spase://CDPP/Person/Jannis.Dandouras 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 @@ -32,11 +29,10 @@ http://amda.cdpp.eu NetCDF - NASA, Prof. Henri Reme - IRAP + CSA Calibrated - Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data + C1_CP_CIS-HIA_PAD_HS_MAG_IONS_PF Calibrated 1 spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA @@ -71,46 +67,49 @@ magnetotail lobe - Pitch angle distribution + 2D pitch-angle/energy distribution c1_hia_pad - - pos.posAng + Hot ion pitch angle distribution + PT4S cnts/(cm2 s sr Kev) Spectrogram - - Other - + + Ion + NumberFlux + - Pitch angle distribution : sum over all energies + 1D pitch-angle distribution : sum over energies c1_hia_pad_angle - - pos.posAng + Hot ion pitch angle distribution (sum over all energy bins) + PT4S cnts/(cm2 s sr Kev) Spectrogram - - Other - + + Ion + NumberFlux + - Energy distribution : sum over all pitch angles + 1D energy distribution : sum over PA c1_hia_pad_energy - - pos.posAng + Hot ion pitch angle distribution (sum over all angle bins) + PT4S cnts/(cm2 s sr Kev) Spectrogram - - Other - + + Ion + NumberFlux + diff --git a/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-mom.xml b/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-mom.xml index 38f9e63..b409094 100644 --- a/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-mom.xml +++ b/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-mom.xml @@ -43,7 +43,7 @@ CSA Calibrated - c3_CP_CIS-HIA_ONBOARD_MOMENTS + C3_CP_CIS-HIA_ONBOARD_MOMENTS Calibrated 1 spase://CDPP/Instrument/AMDA/Cluster-Samba/CIS-HIA diff --git a/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml b/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml index 04cd552..f9deb28 100644 --- a/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml +++ b/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml @@ -1,27 +1,24 @@ - + 2.2.6 spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad - pitch angle distribution - Pitch-Angle Distribution - 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 + PAD + 2D Pitch-Angle/Energy distribution + 2016-10-19T10:51:45Z + Pitch-angle distributions (PADs) are given in particle flux units, as a function of the particle energy and pitch-angle (2D distributions), and their resolution is in 16 angular sectors covering the pitch angle range from 0° to 180°. + PADs are calculated for HIA magnetospheric modes. The dataset is provided with 31 energy bins resolution + Principal Investigator: Dr. Iannis Dandouras - spase://SMWG/Person/Henri.Reme + spase://CDPP/Person/Jannis.Dandouras PrincipalInvestigator - - - spase://SMWG/Person/Elena.Budnik - TechnicalContact - NSSDC Master Catalog listing for Cluster II Samba Cluster Ion Spectrometry (CIS) + 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 Samba Cluster Ion Spectrometry Instrument. - + This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument. + spase://SMWG/Repository/CDPP/AMDA @@ -29,22 +26,21 @@ Open AMDA at CDPP - http://amda.cdpp.eu - + http://amda.cdpp.eu + NetCDF - NASA, Prof. Henri Reme - IRAP + CSA Calibrated - + C3_CP_CIS-HIA_PAD_HS_MAG_IONS_PF Calibrated 1 - spase://CDPP/Instrument/AMDA/Cluster-Samba/CIS-HIA + spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA ThermalPlasma 2001-01-31T01:02:10Z - 2009-11-11T08:17:05Z + 2009-11-11T08:17:05Z PT4S @@ -69,48 +65,51 @@ magnetosheath Cluster magnetotail - lobe + lobe - Pitch angle distribution + 2D pitch-angle/energy distribution c3_hia_pad - - pos.posAng + Hot ion pitch angle distribution + PT4S cnts/(cm2 s sr Kev) Spectrogram - - Other - + + Ion + NumberFlux + - Pitch angle distribution : sum over all energies + 1D pitch-angle distribution : sum over energies c3_hia_pad_angle - - pos.posAng + Hot ion pitch angle distribution (sum over all energy bins) + PT4S cnts/(cm2 s sr Kev) Spectrogram - - Other - + + Ion + NumberFlux + - - Energy distribution : sum over all pitch angles + + 1D energy distribution : sum over PA c3_hia_pad_energy - - pos.posAng + Hot ion pitch angle distribution (sum over all angle bins) + PT4S cnts/(cm2 s sr Kev) Spectrogram - - Other - + + Ion + NumberFlux + -- libgit2 0.21.2