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  <Version>2.4.1</Version>
  <NumericalData>
    <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ULYSSES/SWICS/ulys-swi-rat</ResourceID>
    <ResourceHeader>
      <ResourceName>abundance ratios</ResourceName>

      <ReleaseDate>2020-06-24T16:09:54Z</ReleaseDate>

      <Description> Selected charge states and abundance ratios : 

                Alpha particle speed: Repeated from previous archive for comparison. - C6+/C5+
                and O7+/O6+ ratios: These two ratios are essentially redundant, with the former
                being ~10 times higher than the latter on average. At high values the O ratio is
                more reliable (because C5+ is getting rare) whereas at low values the C ratio is
                preferable (because O7+ gets rare). Low ratios are indicative of fast streams. -
                Fe/O abundance ratio: This is a proxy for the strength of the FIP fractionation
                if divided by the solar Fe/O ratio of ~0.05. - Average charge state of Fe:
                Weighted average of all charge states from Fe6+ to Fe16+, normally between 9 and
                12 both in slow and in fast wind. High values are a good CME indicator. - Number
                of instrument cycles that were accumulated to obtain the 3-hour average value.
                Each instrument cycle takes 13 minutes, so values of 12-14 are normal, whereas
                low values should be considered as a warning.</Description>

      <Contact>
        <PersonID>spase://SMWG/Person/Rudolf.Von.Steiger</PersonID>
        <Role>DataProducer</Role>
      </Contact>
      <InformationURL>
        <Name>Instrument and data portal at Cosmos</Name>
        <URL>https://www.cosmos.esa.int/web/ulysses/swics-instrument</URL>
      </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>ulys-swi-rat</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>ESA</ProviderName>
    <ProviderResourceName>uswimatbYY.dat</ProviderResourceName>
    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Ulysses/SWICS</InstrumentID>
    <MeasurementType>ThermalPlasma</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>1990-12-07T20:02:48Z</StartDate>
        <StopDate>2009-06-29T06:15:49Z</StopDate>
      </TimeSpan>
      <Cadence>PT3H</Cadence>
    </TemporalDescription>
    <ObservedRegion>Heliosphere</ObservedRegion>
    <Parameter>
      <Name>C6+/C5+ ratio</Name>
      <ParameterKey>ulys_swi_crat</ParameterKey>
      <Description>ratio of carbon 6+ to 5+</Description>

      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>ChargeState</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>O7+/O6+ ratio</Name>
      <ParameterKey>ulys_swi_orat</ParameterKey>
      <Description>ratio of oxygen 7+ to 6+</Description>

      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>ChargeState</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Fe/O ratio</Name>
      <ParameterKey>ulys_swi_ferat</ParameterKey>
      <Description>abundance ratio of iron to oxygen</Description>

      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>ChargeState</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Fe charge</Name>
      <ParameterKey>ulys_swi_fech</ParameterKey>
      <Description>average charge state of iron in e- = 1.6022e-19 C</Description>
      <Units>e-</Units>
      <RenderingHints>
        <DisplayType>TimeSeries</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>ChargeState</ParticleQuantity>
      </Particle>
    </Parameter>
  </NumericalData>

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