<?xml version="1.0" encoding="UTF-8"?>

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  <Version>2.4.1</Version>
  <NumericalData>
    <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/MAG/so-mag-rtnhr</ResourceID>
    <ResourceHeader>
      <ResourceName>0.1 sec : rtn</ResourceName>
      <AlternateName>Magnetic Field in RTN : 0.1 sec</AlternateName>

      <ReleaseDate>2024-05-15T03:09:08Z</ReleaseDate>

      <Description>Publication quality. Take note of Quality Flag and refer to SOL-MAG-DPDD for exceptions ( see SolO Archive Support Data)</Description>
      <Acknowledgement>Solar Orbiter magnetometer data was provided by Imperial College London and supported by the UK Space Agency</Acknowledgement>
      <Contact>
        <PersonID>spase://CNES/Person/CDPP-AMDA/Tim.Horbury</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <InformationURL>
        <Name>SolO home page at Imperial College</Name>
        <URL>https://www.imperial.ac.uk/space-and-atmospheric-physics/research/missions-and-projects/space-missions/solar-orbiter/</URL>

      </InformationURL>

      <InformationURL>
        <Name>SolO Archive Support Data</Name>
        <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>

      </InformationURL>

      <Association>
        <AssociationID>solo-mag-l2</AssociationID>
        <AssociationType>PartOf</AssociationType>
        <Note>L2</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-mag-rtnhr</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>MAG-RTN-NORMAL</ProviderResourceName>
    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/MAG</InstrumentID>
    <MeasurementType>MagneticField</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2020-04-15T00:00:00Z</StartDate>

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

      </TimeSpan>
      <Cadence>PT0.1S</Cadence>
    </TemporalDescription>
    <ObservedRegion>Heliosphere.Inner</ObservedRegion>
    <ObservedRegion>Sun.Corona</ObservedRegion>
    <Caveats>Flag setting: 

           * 0: Bad data; 
           * 1: Known problems use at your own risk; 
           * 2: Survey data, possibly not publication quality; 
           * 3: Good for publication subject to PI approval; 
           * 4: Excellent data which has received special treatment; refer SOL-MAG-DPDD for more information on how these flags are generated."</Caveats>

    <Parameter>
      <Name>b_rtn</Name>
      <ParameterKey>solo_b_rtn_hr</ParameterKey>

      <UCD>phys.magField</UCD>
      <Units>nT</Units>
      <UnitsConversion>1e-9&gt;T</UnitsConversion>
      <CoordinateSystem>
        <CoordinateRepresentation>Cartesian</CoordinateRepresentation>
        <CoordinateSystemName>RTN</CoordinateSystemName>
      </CoordinateSystem>
      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Structure>
        <Size>3</Size>
        <Element>
          <Name>br</Name>
          <Qualifier>Component.I</Qualifier>
          <Index>1</Index>
          <ParameterKey>solo_b_rtn_hr(0)</ParameterKey>
        </Element>
        <Element>
          <Name>bt</Name>
          <Qualifier>Component.J</Qualifier>
          <Index>2</Index>
          <ParameterKey>solo_b_rtn_hr(1)</ParameterKey>
        </Element>
        <Element>
          <Name>bn</Name>
          <Qualifier>Component.K</Qualifier>
          <Index>3</Index>
          <ParameterKey>solo_b_rtn_hr(2)</ParameterKey>
        </Element>
      </Structure>
      <Field>
        <Qualifier>Vector</Qualifier>
        <Qualifier>Component.I</Qualifier>
        <Qualifier>Component.J</Qualifier>
        <Qualifier>Component.K</Qualifier>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
    </Parameter>
    <Parameter>
      <Name>|b|</Name>
      <ParameterKey>solo_b_rtn_hr_tot</ParameterKey>
      <Description>

              Magnetic field magnitude 
          </Description>

      <UCD>phys.magField</UCD>
      <Units>nT</Units>
      <UnitsConversion>1e-9&gt;T</UnitsConversion>
      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Field>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
    </Parameter>
    <Parameter>
      <Name>phi</Name>
      <ParameterKey>solo_b_rtn_hr_phi</ParameterKey>
      <Description>

              Magnetic field phi angle 
          </Description>

      <UCD>phys.magField</UCD>
      <Units>degrees</Units>
      <UnitsConversion>1e-9&gt;T</UnitsConversion>
      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Field>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
    </Parameter>
    <Parameter>
      <Name>theta</Name>
      <ParameterKey>solo_b_rtn_hr_theta</ParameterKey>
      <Description>

              Magnetic field theta angle
          </Description>

      <UCD>phys.magField</UCD>
      <Units>degrees</Units>
      <UnitsConversion>1e-9&gt;T</UnitsConversion>
      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Field>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
    </Parameter>
    <Parameter>
      <Name>quality</Name>
      <ParameterKey>solo_b_rtn_hr_qf</ParameterKey>
      <Description>

               Flag setting: 0: Bad data; 1: Known problems use at your own risk; 2: Survey data, possibly 
               not publication quality; 3: Good for publication subject to PI approval; 4: Excellent data which has received special treatment
           </Description>

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

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