CDPP / CNES

Commit 25d26c84ede553efc9b51fbdf9954a2d8b318549

Authored by Quentin Brzustowski
1 parent 2a1ad25f
Exists in master and in 11 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

Created dataset Geotail CPI-SWA

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Instrument/CDPP-AMDA/Geotail/CPI.xml 0 → 100644
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  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Geotail/CPI</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>CPI</ResourceName>
  8 + <AlternateName>Geotail Comprehensive Plasma Instrumentation</AlternateName>
  9 + <ReleaseDate>2019-05-05T12:34:56.789</ReleaseDate>
  10 + <Description>
  11 + The objective of the Comprehensive Plasma Instrumentation (CPI) investigation is to make comprehensive observations
  12 + of the three-dimensional velocity distribution functions of electrons and positive ions, with identification of ion species.
  13 + The instrument contains three sets of quadrispherical analyzers with channel electron multipliers.
  14 + These three obtain three-dimensional measurements for hot plasma and solar wind electrons, for solar wind ions,
  15 + and for positive-ion composition measurements. The positive-ion composition measurement of the Ion Composition
  16 + (IC) analyzer includes five miniature imaging mass spectrometers at the exit aperture of the analyzer, and covers
  17 + masses from 1 to 550 u/Q at 100 eV, and 1 to 55 u/Q at 10 keV. The Hot Plasma (HP) analyzer measures electrons and ions
  18 + in the range 1-50,000 eV/Q. The Solar Wind (SW) analyzer measures ions from 150 to 7,000 eV/Q.
  19 + Sequencing of the energy analyzers and mass spectrometers, and other control functions, are provided by two microprocessors.
  20 + </Description>
  21 + <Contact>
  22 + <PersonID>spase://SMWG/Person/Louis.A.Frank</PersonID>
  23 + <Role>PrincipalInvestigator</Role>
  24 + </Contact>
  25 + <InformationURL>
  26 + <Name>NSSDC's Master Catalog</Name>
  27 + <URL>https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1992-044A-04</URL>
  28 + <Description>Information about the Comprehensive Plasma Instrument</Description>
  29 + </InformationURL>
  30 + </ResourceHeader>
  31 + <InstrumentType>QuadrisphericalAnalyser</InstrumentType>
  32 + <InvestigationName>CPI on GEOTAIL</InvestigationName>
  33 + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Geotail</ObservatoryID>
  34 + </Instrument>
  35 +</Spase>
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NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl_cpi_swa.xml 0 → 100644
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  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Geotail/CPI/gtl-cpi-swa</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>SWA</ResourceName>
  8 + <AlternateName>Solar Wind Analyser</AlternateName>
  9 + <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
  10 + <Description>
  11 + The Solar Wind Analyzer (SWA) of the Comprehensive Plasma Instrumentation (CPI) on Geotail is a quadrispherical plasma analyzer
  12 + that measures three-dimensional fluxes of ions in the range 150-7,000 eV/Q.
  13 + Version 6 data processing replaced version 5 processing for data after March 10,
  14 + 2006, when the CPI team started using 64 energy steps per spectrum instead of
  15 + the previously used 32 steps per spectrum. The change was made to ensure that
  16 + even for very cold flows, the spectrum would have a sufficient number of
  17 + significant points to derive moments. The change resulted in 96s spectra and
  18 + 96s-resolution moments, vs. 48s previously.
  19 + </Description>
  20 + <Acknowledgement>In any publications, the use of the Geotail data should be acknowledged"</Acknowledgement>
  21 + <Contact>
  22 + <PersonID>spase://SMWG/Person/Louis.A.Frank</PersonID>
  23 + <Role>PrincipalInvestigator</Role>
  24 + </Contact>
  25 + <Contact>
  26 + <PersonID>spase://SMWG/Person/William.R.Paterson</PersonID>
  27 + <Role>GeneralContact</Role>
  28 + </Contact>
  29 + </ResourceHeader>
  30 + <AccessInformation>
  31 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  32 + <Availability>Online</Availability>
  33 + <AccessRights>Open</AccessRights>
  34 + <AccessURL>
  35 + <Name>AMDA at CDPP</Name>
  36 + <URL>http://amda.cdpp.eu</URL>
  37 + </AccessURL>
  38 + <Format>NetCDF</Format>
  39 + <Encoding>None</Encoding>
  40 + <Acknowledgement>Data provider DARTS at Institute of Space and Astronautical Science, JAXA in Japan</Acknowledgement>
  41 + </AccessInformation>
  42 + <ProviderName>CDAweb</ProviderName>
  43 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Geotail/CPI</InstrumentID>
  44 + <MeasurementType>EnergeticParticles</MeasurementType>
  45 + <TemporalDescription>
  46 + <TimeSpan>
  47 + <StartDate>1992-09-28T00:00:02Z</StartDate>
  48 + <StopDate>2019-06-26T23:59:28Z</StopDate>
  49 + </TimeSpan>
  50 + <Cadence>PT96S</Cadence>
  51 + </TemporalDescription>
  52 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
  53 + <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  54 + <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
  55 + <Parameter>
  56 + <Name>v_gse</Name>
  57 + <ParameterKey>gtl_cpi_swa_v</ParameterKey>
  58 + <Description>Ion bulk flow velocity (H+ only in solar wind) in GSE cartesian coordinates</Description>
  59 + <Units>km/s</Units>
  60 + <CoordinateSystem>
  61 + <CoordinateRepresentation>Cartesian</CoordinateRepresentation>
  62 + <CoordinateSystemName>GSE</CoordinateSystemName>
  63 + </CoordinateSystem>
  64 + <RenderingHints>
  65 + <DisplayType>TimeSeries</DisplayType>
  66 + </RenderingHints>
  67 + <Structure>
  68 + <Size>3</Size>
  69 + <Element>
  70 + <Name>vx</Name>
  71 + <Qualifier>Component.I</Qualifier>
  72 + <Index>1</Index>
  73 + <ParameterKey>gtl_cpi_swa_v(0)</ParameterKey>
  74 + </Element>
  75 + <Element>
  76 + <Name>vy</Name>
  77 + <Qualifier>Component.J</Qualifier>
  78 + <Index>2</Index>
  79 + <ParameterKey>gtl_cpi_swa_v(1)</ParameterKey>
  80 + </Element>
  81 + <Element>
  82 + <Name>vz</Name>
  83 + <Qualifier>Component.K</Qualifier>
  84 + <Index>3</Index>
  85 + <ParameterKey>gtl_cpi_swa_v(2)</ParameterKey>
  86 + </Element>
  87 + </Structure>
  88 + </Parameter>
  89 + <Parameter>
  90 + <Name>density</Name>
  91 + <ParameterKey>gtl_cpi_swa_n</ParameterKey>
  92 + <Description>Ion number density</Description>
  93 + <Caveats>Assuming no helium (0.3 - several hundred) if the density is less than 0.3/cc the higher moments (VEL,TEMP) shall not be used because of the poor counting statistics.</Caveats>
  94 + <Units>/cc</Units>
  95 + <RenderingHints>
  96 + <DisplayType>TimeSeries</DisplayType>
  97 + </RenderingHints>
  98 + </Parameter>
  99 + <Parameter>
  100 + <Name>temerature</Name>
  101 + <ParameterKey>gtl_cpi_swa_t</ParameterKey>
  102 + <Description>Ion average kinetic temperature</Description>
  103 + <Units>eV</Units>
  104 + <RenderingHints>
  105 + <DisplayType>TimeSeries</DisplayType>
  106 + </RenderingHints>
  107 + </Parameter>
  108 + </NumericalData>
  109 +</Spase>
... ...