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  <Version>2.2.6</Version>
  <NumericalOutput>
    <ResourceID>spase://CNES/NumericalOutput/CDPP-AMDA/KT17/b_kt17</ResourceID>
    <ResourceHeader>
      <ResourceName>KT17 along s/c orbit</ResourceName>
      <ReleaseDate>2023-02-17T00:00:00Z</ReleaseDate>

      <Description>Magnetic field along S/C orbit at Mercury is being real-time calculated.

                   S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. 
         
                   KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
      </Description>
      <Acknowledgement>James, M. K. - KT17 (v1.0.0) - https://github.com/mattkjames7/KT17/releases/tag/v1.0.0</Acknowledgement>
      <Contact>
        <PersonID>spase://CNES/Person/CDPP-AMDA/Haje.Korth</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <Contact>
        <PersonID>spase://CNES/Person/CDPP-AMDA/M.K.James</PersonID>
        <Role>TechnicalContact</Role>
      </Contact>
      <InformationURL>
        <Name>Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154.</Name>
        <URL>https://doi.org/10.1002/2017GL074699</URL>
        <Description>Model description</Description>
      </InformationURL>
      <InformationURL>
        <Name>James, M. K. - KT17 (v1.0.0)</Name>
        <URL>https://github.com/mattkjames7/KT17/releases/tag/v1.0.0</URL>
        <Description>Software</Description>
      </InformationURL>
      <InformationURL>
        <Name>Anderson, B. J., Johnson, C. L., and Korth, H. (2013), A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data, Geochem. Geophys. Geosyst., 14, 3875– 3886</Name>
        <URL>https://doi.org/10.1002/ggge.20242</URL>
        <Description>Disturbance index description</Description>
      </InformationURL>
    </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>b_kt17</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>

    <SimulationRunID>spase://CNES/SimulationRun/CDPP-AMDA/KT17/KT17Run</SimulationRunID>
    <MeasurementType>MagneticField</MeasurementType>
    <TemporalDescription>
      <TimeSpan>

        <StartDate>1970-01-01T00:00:00Z</StartDate>
        <StopDate>2030-01-01T00:00:00Z</StopDate>

      </TimeSpan>

      <Cadence>PT1M</Cadence>

    </TemporalDescription>
    <SimulatedRegion>Mercury</SimulatedRegion>
    <Caveats/>
    <InputResourceID/>
    <Parameter>
      <Name>b msm @@orbit@@</Name>
      <ParameterKey>b_kt17_model</ParameterKey>
      <Description/>
      <Units>nT</Units>
      <Structure>
        <Size>3</Size>
        <Element>
          <Name>bx</Name>
          <Qualifier>Component.I</Qualifier>
          <Index>1</Index>
          <ParameterKey>b_kt17_model(0)</ParameterKey>
          <ValidMin/>
          <ValidMax/>
        </Element>
        <Element>
          <Name>by</Name>
          <Qualifier>Component.J</Qualifier>
          <Index>2</Index>
          <ParameterKey>b_kt17_model(1)</ParameterKey>
          <ValidMin/>
          <ValidMax/>
        </Element>
        <Element>
          <Name>bz</Name>
          <Qualifier>Component.K</Qualifier>
          <Index>3</Index>
          <ParameterKey>b_kt17_model(2)</ParameterKey>
          <ValidMin/>
          <ValidMax/>
          <FillValue/>
        </Element>
      </Structure>
      <Field>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
    </Parameter>
    <Parameter>
      <Name>|b|</Name>
      <ParameterKey>b_kt17_model_tot</ParameterKey>
      <Description>Scalar magnitude of the magnetic field in nT</Description>
      <UCD>phys.magField</UCD>
      <Units>nT</Units>
      <UnitsConversion>1e-9&gt;T</UnitsConversion>
      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Field>
        <Qualifier>Magnitude</Qualifier>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
    </Parameter>
  </NumericalOutput>
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