diff --git a/Instrument/AMDA/Geotail/EPIC.xml b/Instrument/AMDA/Geotail/EPIC.xml index 159e0cf..7dcfc25 100644 --- a/Instrument/AMDA/Geotail/EPIC.xml +++ b/Instrument/AMDA/Geotail/EPIC.xml @@ -7,9 +7,9 @@ EPIC Energetic Particles and Ion Composition instrument 2017-02-04T12:34:56.789 - The Energetic Particles and Ion Composition (EPIC) instrument (block diagram) is actually composed of two separate sensor and processing assemblies. - * The STICS assembly (Supra-Thermal Ion Composition Spectrometer) uses a quadrispherical electrostatic analyzer followed by a foil/solid state detector time-of-flight (TOF) telecope to measure charge state, mass and energy of ions with energies of 30 - 230 keV/charge. It uses an electrostatic analyzer with a geometry factor of 0.05 cm**2 sr, time of flight and energy analysis. - * The ICS assembly (Ion Composition Subsystem) measures mass and energy properties of energetic ions with energies of less than 50 keV to 3 MeV. It uses a pair of collimators with sweeping magnets to reject electrons, followed by TOF and energy analysis, with a geometry factor of 0.2 cm**2 sr. A thin foil/solid state detector electron telescope measures electrons higher than 30 keV. + The Energetic Particles and Ion Composition (EPIC) instrument is actually composed of two separate sensor and processing assemblies. + * The STICS assembly (Supra-Thermal Ion Composition Spectrometer) uses a quadrispherical electrostatic analyzer followed by a foil/solid state detector time-of-flight (TOF) telecope to measure charge state, mass and energy of ions with energies of 30 - 230 keV/charge. It uses an electrostatic analyzer with a geometry factor of 0.05 cm^2 sr, time of flight and energy analysis. + * The ICS assembly (Ion Composition Subsystem) measures mass and energy properties of energetic ions with energies of less than 50 keV to 3 MeV. It uses a pair of collimators with sweeping magnets to reject electrons, followed by TOF and energy analysis, with a geometry factor of 0.2 cm^2 sr. A thin foil/solid state detector electron telescope measures electrons higher than 30 keV. spase://SMWG/Person/Donald.J.Williams diff --git a/Instrument/AMDA/Geotail/LEP.xml b/Instrument/AMDA/Geotail/LEP.xml index a0a4bb5..628ba01 100644 --- a/Instrument/AMDA/Geotail/LEP.xml +++ b/Instrument/AMDA/Geotail/LEP.xml @@ -20,10 +20,6 @@ spase://SMWG/Person/Donald.H.Fairfield Scientist - - spase://SMWG/Person/Jan.Merka - MetadataContact - The Geotail Low Energy Particle Experiment (LEP) http://www.darts.isas.ac.jp/stp/geotail/jgg_lep.pdf diff --git a/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml index 19c956a..34770ef 100644 --- a/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml +++ b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml @@ -4,21 +4,24 @@ spase://CDPP/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed - ED : electron flux - Electron Detector : + ED : electron flux : E > 34 keV + Electron Detector : electron integral flux : E > 34 keV 2017-02-12T10:48:29Z - *'directionward' (tailward, etc) : the correspondinf sector is taken + *'directionward' (tailward, etc) : the corresponding sector is taken * Sectors (degrees) : 0., 45., 90., 135., 180., 225., 270., 315.; - - - + + spase://CDPP/Person/Stuart.Nyland + DataProducer + + + spase://CDPP/Person/Elena.Budnik + TechnicalContact + - - - - + + @@ -32,7 +35,7 @@ CDF - + JHU/APL spase://CDPP/Instrument/AMDA/Geotail/EPIC EnergeticParticles @@ -42,19 +45,18 @@ PT3S - Comet - - + Earth.Magnetosphere + - integral flux : E > 34 keV + e- flux gtl_edhigh_av - - - - - + 1/(cm**2-s-sr-kev) + + Electron + NumberFlux + - + diff --git a/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh.xml b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh.xml new file mode 100644 index 0000000..4c98fd4 --- /dev/null +++ b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh.xml @@ -0,0 +1,67 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh + + P2 : proton flux + P2 : proton flux : 58 - 77 keV : averaged over two heads + 2017-02-12T10:48:29Z + + + + spase://CDPP/Person/Stuart.Nyland + DataProducer + + + spase://CDPP/Person/Elena.Budnik + TechnicalContact + + + + + + + + gtl-ics-high + PartOf + ICS : high resolution : profile + + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + AMDA at CDPP + http://amda.cdpp.eu + + CDF + + + JHU/APL + spase://CDPP/Instrument/AMDA/Geotail/EPIC + EnergeticParticles + + + 1992-10-18T00:01:17Z + 2010-12-31T23:57:50Z + + PT6S + + Earth.Magnetosphere + + + + proton flux + gtl_phigh_av + + + 1/(cm**2-s-sr-kev) + + Proton + NumberFlux + + + + diff --git a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml index db5c8a0..eecd59e 100644 --- a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml +++ b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml @@ -22,14 +22,6 @@ spase://SMWG/Person/Donald.H.Fairfield Scientist - - spase://SMWG/Person/Jan.Merka - MetadataContact - - - spase://SMWG/Person/Elena.Budnik - TechnicalContact - The Geotail Low Energy Particle Experiment (LEP) http://www.darts.isas.ac.jp/stp/geotail/jgg_lep.pdf diff --git a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml index 85fc644..c82e21e 100644 --- a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml +++ b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml @@ -17,14 +17,6 @@ spase://SMWG/Person/Donald.H.Fairfield Scientist - - spase://SMWG/Person/Jan.Merka - MetadataContact - - - spase://SMWG/Person/Elena.Budnik - TechnicalContact - The Geotail Low Energy Particle Experiment (LEP) http://www.darts.isas.ac.jp/stp/geotail/jgg_lep.pdf diff --git a/Person/Stuart.Nyland.xml b/Person/Stuart.Nyland.xml new file mode 100644 index 0000000..0ffb5c6 --- /dev/null +++ b/Person/Stuart.Nyland.xml @@ -0,0 +1,10 @@ + + + 2.2.0 + + spase://CDPP/Person/Stuart.Nyland + Dr. Stuart Nyland + Applied Physics Laboratory, Johns Hopkins University + Stu.Nylund@jhuapl.edu + + -- libgit2 0.21.2