<?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://www.spase-group.org/data/schema/spase-2.4.1.xsd">
  <Version>2.4.1</Version>
  <NumericalData>
    <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.1</ResourceID>
    <ResourceHeader>
      <ResourceName>sunward flow</ResourceName>
      <AlternateName>Electron HighEnergy ( 38-96 MeV ) / He3 / He4 From Antisun Direction ( mean Parker spiral )</AlternateName>

      <ReleaseDate>2024-05-20T03:04:16Z</ReleaseDate>

      <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. 

              
HET  measures the upper part of the energetic particle spectrum. It is equipped with several solid 
state detectors and a BGO crystal to provide identification of particle species from the relative energy
deposited in the different detectors. Thus, HET  measures count rates for different ion species, as
well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
Anti-Sun, North and South)

Parameter ID uses Detector looking directon.
          </Description>

      <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
      <Contact>
        <PersonID>spase://CNES/Person/CDPP-AMDA/J.Rodrigues-Pacheco</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <InformationURL>
        <Name>SolO Archive Support Data</Name>
        <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>

      </InformationURL>

      <Association>
        <AssociationID>solo-epd-het.1</AssociationID>
        <AssociationType>PartOf</AssociationType>
        <Note>L2 : e- 38-96 MeV / he3 / he4 flux</Note>
      </Association>
    </ResourceHeader>
    <AccessInformation>

      <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
      <AccessURL>
        <Name>CDPP/AMDA HAPI Server</Name>

        <URL>https://amda.irap.omp.eu/service/hapi</URL>

        <Style>HAPI</Style>

        <ProductKey>so-het-anti.1</ProductKey>

        <Description>Web Service to this product using the HAPI interface.</Description>
      </AccessURL>
      <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 https://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>https://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 https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</Acknowledgement>

    </AccessInformation>

    <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
    <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
    <MeasurementType>EnergeticParticles</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2020-05-13T00:00:03Z</StartDate>

        <StopDate>2024-02-29T23:59:59Z</StopDate>

      </TimeSpan>
      <CadenceMin>PT5S</CadenceMin>
      <CadenceMax>PT30S</CadenceMax>
    </TemporalDescription>
    <ObservedRegion>Heliosphere.Inner</ObservedRegion>
    <ObservedRegion>Sun.Corona</ObservedRegion>
    <Parameter>
      <Name>e- HE flux: sunward</Name>
      <ParameterKey>solo_het_asun_eheflux</ParameterKey>
      <Description>Electron flux in 38 - 96 MeV energy range</Description>

      <Units>1/(s cm^2 sr MeV)</Units>

      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>e- HE flux unc: sunward</Name>
      <ParameterKey>solo_het_asun_eheunc</ParameterKey>
      <Description>Uncertainty in electron flux</Description>

      <Units>1/(s cm^2 sr MeV)</Units>

      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>he3 flux: sunward</Name>
      <ParameterKey>solo_het_asun_he3flux</ParameterKey>
      <Description>He3 flux</Description>

      <Units>1/(s cm^2 sr MeV)</Units>

      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Structure>
        <Size>9</Size>
      </Structure>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>he3 flux unc: sunward</Name>
      <ParameterKey>solo_het_asun_he3unc</ParameterKey>
      <Description>Uncertainty in He3 flux</Description>

      <Units>1/(s cm^2 sr MeV)</Units>

      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Structure>
        <Size>9</Size>
      </Structure>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>he4 flux: sunward</Name>
      <ParameterKey>solo_het_asun_he4flux</ParameterKey>
      <Description>He4 flux</Description>

      <Units>1/(s cm^2 sr MeV)</Units>

      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Structure>
        <Size>15</Size>
      </Structure>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>he4 flux unc: sunward</Name>
      <ParameterKey>solo_het_asun_he4unc</ParameterKey>
      <Description>Uncertainty in He4 flux</Description>

      <Units>1/(s cm^2 sr MeV)</Units>

      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Structure>
        <Size>15</Size>
      </Structure>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>quality flag: sunward</Name>
      <ParameterKey>solo_het_asun_1_qf</ParameterKey>
      <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>

      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Support>
        <SupportQuantity>DataQuality</SupportQuantity>
      </Support>
    </Parameter>
  </NumericalData>

</Spase>