From 4aaf7e34d29e376640c2137783ac48c75ace5801 Mon Sep 17 00:00:00 2001 From: Quentin Brzustowski <quentin.brzustowski@irap.omp.eu> Date: Fri, 7 Feb 2020 17:24:21 +0100 Subject: [PATCH] corrected mistake _ => - --- NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl-cpi-swa.xml | 109 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl_cpi_swa.xml | 109 ------------------------------------------------------------------------------------------------------------- 2 files changed, 109 insertions(+), 109 deletions(-) create mode 100644 NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl-cpi-swa.xml delete mode 100644 NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl_cpi_swa.xml diff --git a/NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl-cpi-swa.xml b/NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl-cpi-swa.xml new file mode 100644 index 0000000..102ee73 --- /dev/null +++ b/NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl-cpi-swa.xml @@ -0,0 +1,109 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.3.1</Version> + <NumericalData> + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Geotail/CPI/gtl-cpi-swa</ResourceID> + <ResourceHeader> + <ResourceName>SWA</ResourceName> + <AlternateName>Solar Wind Analyser</AlternateName> + <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate> + <Description> + The Solar Wind Analyzer (SWA) of the Comprehensive Plasma Instrumentation (CPI) on Geotail is a quadrispherical plasma analyzer + that measures three-dimensional fluxes of ions in the range 150-7,000 eV/Q. + Version 6 data processing replaced version 5 processing for data after March 10, + 2006, when the CPI team started using 64 energy steps per spectrum instead of + the previously used 32 steps per spectrum. The change was made to ensure that + even for very cold flows, the spectrum would have a sufficient number of + significant points to derive moments. The change resulted in 96s spectra and + 96s-resolution moments, vs. 48s previously. + </Description> + <Acknowledgement>In any publications, the use of the Geotail data should be acknowledged"</Acknowledgement> + <Contact> + <PersonID>spase://SMWG/Person/Louis.A.Frank</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <Contact> + <PersonID>spase://SMWG/Person/William.R.Paterson</PersonID> + <Role>GeneralContact</Role> + </Contact> + </ResourceHeader> + <AccessInformation> + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> + <Availability>Online</Availability> + <AccessRights>Open</AccessRights> + <AccessURL> + <Name>AMDA at CDPP</Name> + <URL>http://amda.cdpp.eu</URL> + </AccessURL> + <Format>NetCDF</Format> + <Encoding>None</Encoding> + <Acknowledgement>Data provider DARTS at Institute of Space and Astronautical Science, JAXA in Japan</Acknowledgement> + </AccessInformation> + <ProviderName>CDAweb</ProviderName> + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Geotail/CPI</InstrumentID> + <MeasurementType>EnergeticParticles</MeasurementType> + <TemporalDescription> + <TimeSpan> + <StartDate>1992-09-28T00:00:02Z</StartDate> + <StopDate>2019-06-26T23:59:28Z</StopDate> + </TimeSpan> + <Cadence>PT96S</Cadence> + </TemporalDescription> + <ObservedRegion>Earth.Magnetosheath</ObservedRegion> + <ObservedRegion>Earth.Magnetosphere</ObservedRegion> + <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion> + <Parameter> + <Name>v_gse</Name> + <ParameterKey>gtl_cpi_swa_v</ParameterKey> + <Description>Ion bulk flow velocity (H+ only in solar wind) in GSE cartesian coordinates</Description> + <Units>km/s</Units> + <CoordinateSystem> + <CoordinateRepresentation>Cartesian</CoordinateRepresentation> + <CoordinateSystemName>GSE</CoordinateSystemName> + </CoordinateSystem> + <RenderingHints> + <DisplayType>TimeSeries</DisplayType> + </RenderingHints> + <Structure> + <Size>3</Size> + <Element> + <Name>vx</Name> + <Qualifier>Component.I</Qualifier> + <Index>1</Index> + <ParameterKey>gtl_cpi_swa_v(0)</ParameterKey> + </Element> + <Element> + <Name>vy</Name> + <Qualifier>Component.J</Qualifier> + <Index>2</Index> + <ParameterKey>gtl_cpi_swa_v(1)</ParameterKey> + </Element> + <Element> + <Name>vz</Name> + <Qualifier>Component.K</Qualifier> + <Index>3</Index> + <ParameterKey>gtl_cpi_swa_v(2)</ParameterKey> + </Element> + </Structure> + </Parameter> + <Parameter> + <Name>density</Name> + <ParameterKey>gtl_cpi_swa_n</ParameterKey> + <Description>Ion number density</Description> + <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> + <Units>/cc</Units> + <RenderingHints> + <DisplayType>TimeSeries</DisplayType> + </RenderingHints> + </Parameter> + <Parameter> + <Name>temperature</Name> + <ParameterKey>gtl_cpi_swa_t</ParameterKey> + <Description>Ion average kinetic temperature</Description> + <Units>eV</Units> + <RenderingHints> + <DisplayType>TimeSeries</DisplayType> + </RenderingHints> + </Parameter> + </NumericalData> +</Spase> diff --git a/NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl_cpi_swa.xml b/NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl_cpi_swa.xml deleted file mode 100644 index 899d1b4..0000000 --- a/NumericalData/CDPP-AMDA/GEOTAIL/CPI/gtl_cpi_swa.xml +++ /dev/null @@ -1,109 +0,0 @@ -<?xml version="1.0" encoding="UTF-8"?> -<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"> - <Version>2.3.1</Version> - <NumericalData> - <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Geotail/CPI/gtl-cpi-swa</ResourceID> - <ResourceHeader> - <ResourceName>SWA</ResourceName> - <AlternateName>Solar Wind Analyser</AlternateName> - <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate> - <Description> - The Solar Wind Analyzer (SWA) of the Comprehensive Plasma Instrumentation (CPI) on Geotail is a quadrispherical plasma analyzer - that measures three-dimensional fluxes of ions in the range 150-7,000 eV/Q. - Version 6 data processing replaced version 5 processing for data after March 10, - 2006, when the CPI team started using 64 energy steps per spectrum instead of - the previously used 32 steps per spectrum. The change was made to ensure that - even for very cold flows, the spectrum would have a sufficient number of - significant points to derive moments. The change resulted in 96s spectra and - 96s-resolution moments, vs. 48s previously. - </Description> - <Acknowledgement>In any publications, the use of the Geotail data should be acknowledged"</Acknowledgement> - <Contact> - <PersonID>spase://SMWG/Person/Louis.A.Frank</PersonID> - <Role>PrincipalInvestigator</Role> - </Contact> - <Contact> - <PersonID>spase://SMWG/Person/William.R.Paterson</PersonID> - <Role>GeneralContact</Role> - </Contact> - </ResourceHeader> - <AccessInformation> - <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> - <Availability>Online</Availability> - <AccessRights>Open</AccessRights> - <AccessURL> - <Name>AMDA at CDPP</Name> - <URL>http://amda.cdpp.eu</URL> - </AccessURL> - <Format>NetCDF</Format> - <Encoding>None</Encoding> - <Acknowledgement>Data provider DARTS at Institute of Space and Astronautical Science, JAXA in Japan</Acknowledgement> - </AccessInformation> - <ProviderName>CDAweb</ProviderName> - <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Geotail/CPI</InstrumentID> - <MeasurementType>EnergeticParticles</MeasurementType> - <TemporalDescription> - <TimeSpan> - <StartDate>1992-09-28T00:00:02Z</StartDate> - <StopDate>2019-06-26T23:59:28Z</StopDate> - </TimeSpan> - <Cadence>PT96S</Cadence> - </TemporalDescription> - <ObservedRegion>Earth.Magnetosheath</ObservedRegion> - <ObservedRegion>Earth.Magnetosphere</ObservedRegion> - <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion> - <Parameter> - <Name>v_gse</Name> - <ParameterKey>gtl_cpi_swa_v</ParameterKey> - <Description>Ion bulk flow velocity (H+ only in solar wind) in GSE cartesian coordinates</Description> - <Units>km/s</Units> - <CoordinateSystem> - <CoordinateRepresentation>Cartesian</CoordinateRepresentation> - <CoordinateSystemName>GSE</CoordinateSystemName> - </CoordinateSystem> - <RenderingHints> - <DisplayType>TimeSeries</DisplayType> - </RenderingHints> - <Structure> - <Size>3</Size> - <Element> - <Name>vx</Name> - <Qualifier>Component.I</Qualifier> - <Index>1</Index> - <ParameterKey>gtl_cpi_swa_v(0)</ParameterKey> - </Element> - <Element> - <Name>vy</Name> - <Qualifier>Component.J</Qualifier> - <Index>2</Index> - <ParameterKey>gtl_cpi_swa_v(1)</ParameterKey> - </Element> - <Element> - <Name>vz</Name> - <Qualifier>Component.K</Qualifier> - <Index>3</Index> - <ParameterKey>gtl_cpi_swa_v(2)</ParameterKey> - </Element> - </Structure> - </Parameter> - <Parameter> - <Name>density</Name> - <ParameterKey>gtl_cpi_swa_n</ParameterKey> - <Description>Ion number density</Description> - <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> - <Units>/cc</Units> - <RenderingHints> - <DisplayType>TimeSeries</DisplayType> - </RenderingHints> - </Parameter> - <Parameter> - <Name>temerature</Name> - <ParameterKey>gtl_cpi_swa_t</ParameterKey> - <Description>Ion average kinetic temperature</Description> - <Units>eV</Units> - <RenderingHints> - <DisplayType>TimeSeries</DisplayType> - </RenderingHints> - </Parameter> - </NumericalData> -</Spase> -- libgit2 0.21.2