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NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omr.xml 5.24 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-omr</ResourceID>
    <ResourceHeader>
      <ResourceName>channel R</ResourceName>
      <AlternateName>Ion Composition mode, Omnidirectional, channel R : High Time Resolution Protons</AlternateName>
      <ReleaseDate>2022-09-02T12:54:12Z</ReleaseDate>
      <Description>         
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             Ion composition mode channel R. The available spectra are obtained by summing over all directions.
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             * Species : Protons
             * Nb of energy Bins : 16
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             * Energy range : 62 keV - 8.32 MeV
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             * Nb of looking directions : 80
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         </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_omni</AssociationID>
        <AssociationType>PartOf</AssociationType>
        <Note>ion composition mode : omni</Note>
      </Association>
    </ResourceHeader>
    <AccessInformation>
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      <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
      <AccessURL>
        <Name>CDPP/AMDA HAPI Server</Name>
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        <URL>https://amda.irap.omp.eu/service/hapi</URL>
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        <Style>HAPI</Style>
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        <ProductKey>psp-loic-omr</ProductKey>
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        <Description>Web Service to this product using the HAPI interface.</Description>
      </AccessURL>
      <Format>CSV</Format>
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      <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 https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</Acknowledgement>
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    </AccessInformation>
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    <AccessInformation>
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      <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
      <AccessURL>
        <Name>CDPP/AMDA Web application</Name>
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        <URL>https://amda.cdpp.eu</URL>
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        <Description>Access to Data via CDPP/AMDA Web application.</Description>
      </AccessURL>
      <Format>CSV</Format>
      <Format>VOTable</Format>
      <Format>CDF</Format>
      <Format>PNG</Format>
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      <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 https://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>2018-09-28T00:01:54Z</StartDate>
        <StopDate>2019-10-10T11:15:04Z</StopDate>
      </TimeSpan>
      <CadenceMin>PT5S</CadenceMin>
      <CadenceMax>PT600S</CadenceMax>
    </TemporalDescription>
    <ObservedRegion>Heliosphere.Inner</ObservedRegion>
    <ObservedRegion>Sun.Corona</ObservedRegion>
    <Parameter>
      <Name>h+ flux</Name>
      <ParameterKey>psp_omic_RHf</ParameterKey>
      <Description>
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               Proton omnidirectional flux
           </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+ countrate</Name>
      <ParameterKey>psp_omic_RHcr</ParameterKey>
      <Description>
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             Protons omnidirectional count rate
         </Description>
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      <Units>cnts/sec</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleQuantity>CountRate</ParticleQuantity>
      </Particle>
    </Parameter>
  </NumericalData>
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</Spase>