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NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-cht.xml 5.34 KB
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<?xml version="1.0" encoding="UTF-8"?>
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<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://www.spase-group.org/data/schema/spase-2.4.1.xsd">
  <Version>2.4.1</Version>
  <NumericalData>
    <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-cht</ResourceID>
    <ResourceHeader>
      <ResourceName>channel T</ResourceName>
      <AlternateName>Protons TOF only</AlternateName>
      <ReleaseDate>2022-09-02T12:54:26Z</ReleaseDate>
      <Description>         
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             Ion composition mode channel T. In this TOF only mode, all ions are counted as protons. The available spectras are obtained by summing 80 directions by wedges of 10 detectors into producing 8 data with 8 looking directions.
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             * Species : Protons
             * Nb of energy Bins : 32
             * Energy range : 30 keV - 47.318 MeV
             * Nb of looking directions : 80
         </Description>
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      <Acknowledgement>
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             Please acknowledge the National Aeronautics and Space Administration, NASA
         </Acknowledgement>
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      <Contact>
        <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <Contact>
        <PersonID>spase://SMWG/Person/Eric.R.Christian</PersonID>
        <Role>DeputyPI</Role>
      </Contact>
      <InformationURL>
        <Name>PSP/ISoIS Energetic Particle Data - User Guide</Name>
        <URL>https://spdf.sci.gsfc.nasa.gov/pub/data/psp/isois/ISOIS_Data_Glossary.pdf</URL>
      </InformationURL>
      <InformationURL>
        <Name>Parker Solar Probe Mission Instrument web page, JPL</Name>
        <URL>http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments</URL>
      </InformationURL>
      <Association>
        <AssociationID>psp_loic_wedge</AssociationID>
        <AssociationType>PartOf</AssociationType>
        <Note>ion composition mode : wedges</Note>
      </Association>
    </ResourceHeader>
    <AccessInformation>
         <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
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            <Name>CDPP/AMDA HAPI Server</Name>
            <URL>http://amda.irap.omp.eu/service/hapi</URL>
            <Style>HAPI</Style>
            <Description>Web Service to this product using the HAPI interface.</Description>
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         </AccessURL>
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         <Format>CSV</Format>
         <Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
      </AccessInformation>
    <AccessInformation>
         <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <Name>CDPP/AMDA Web application</Name>
            <URL>http://amda.cdpp.eu</URL>
            <Description>Access to Data via CDPP/AMDA Web application.</Description>
         </AccessURL>
         <Format>CSV</Format>
         <Format>VOTable</Format>
         <Format>CDF</Format>
         <Format>PNG</Format>
         <Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
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      </AccessInformation>
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    <ProviderName>SPDF</ProviderName>
    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/epiLo</InstrumentID>
    <MeasurementType>EnergeticParticles</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2018-09-28T00:10:54Z</StartDate>
        <StopDate>2019-10-10T11:15:04Z</StopDate>
      </TimeSpan>
      <CadenceMin>PT20S</CadenceMin>
      <CadenceMax>PT1800S</CadenceMax>
    </TemporalDescription>
    <ObservedRegion>Heliosphere.Inner</ObservedRegion>
    <ObservedRegion>Sun.Corona</ObservedRegion>
    <Parameter>
      <Name>h+ flux : 2D</Name>
      <ParameterKey>psp_loic_THf</ParameterKey>
      <Description>
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               Proton flux on 8 wedges
           </Description>
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      <Units>1/cm²/sr/s/(MeV/nuc)</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>h+ count rate : 2D</Name>
      <ParameterKey>psp_loic_THcr</ParameterKey>
      <Description>
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             Protons count rate on 8 wedges
         </Description>
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      <Units>counts/sec</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleQuantity>CountRate</ParticleQuantity>
      </Particle>
    </Parameter>
  </NumericalData>
</Spase>