<?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/ACE/SWEPAM/ace-swepam-stea</ResourceID>
    <ResourceHeader>

      <ResourceName>e- pitch angle : 272 eV</ResourceName>

      <AlternateName>ACE SWEPAM electron pitch angle data at 272eV</AlternateName>

      <ReleaseDate>2021-02-24T17:49:56Z</ReleaseDate>

      <Description>These data files contain suprathermal electron pitch angle distribution functions (s^3 cm^-6) at 272 eV from the ACE/SWEPAM-E instrument. The energy channel is ~12% wide, centered at 272 eV. Pitch angle bins are 9 degrees wide, and run from 0 to 180 degrees (so 0-9, 9-18, 18-27 degrees, etc.).

The break between the core and suprathermal electrons is generally around 70 eV at 1 AU, but varies around this value, at times exceeding 100 eV. Electrons at 272 eV are generally well within the suprathermal range, and the distribution at this energy typically shows very little contribution from the core population. The measured count rates at 272 eV energy provide excellent statistical significance. In addition, because of the high count rates, very few artifacts (for example due to sunlight contamination) are seen in the data at this energy.

The data are in the solar wind frame, and have been corrected for the spacecraft potential. The spacecraft potential determination requires measurement of the lower energy electrons, and so the potentials calcuated at these times have been interpolated to the times of the suprathermal electron measurements. Transformation to the solar wind frame requires interpolation of the measurements (each at a different energy in the solar wind frame) to the desired energy (272 eV).

Also note that the detector gains on the SWEPAM-E instrument change over time, including both slowly decreasing gains and abrupt increases when the instrument voltages are increased. The use of these data for long-term studies of the distribution function amplitudes is therefore strongly discouraged.</Description>

      <Acknowledgement>Please acknowledge the ACE/SWEPAM instrument team and the ACE Science Center. 
      The following would be an appropriate acknowledgement: “We thank the ACE SWEPAM instrument team and the ACE Science Center for providing the ACE data.”  We would appreciate preprints/reprints of your papers when they become available. 
      </Acknowledgement>
      <Contact>

        <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>

        <Role>CoInvestigator</Role>
      </Contact>
      <Contact>

        <PersonID>spase://SMWG/Person/Ruth.Skoug</PersonID>
        <Role>TechnicalContact</Role>

      </Contact>

      <InformationURL>

        <URL>http://www.srl.caltech.edu/ACE/ASC/DATA/level3/swepam/</URL>

      </InformationURL>
      <InformationURL>

        <Name>The ACE Science Center</Name>
        <URL>http://www.srl.caltech.edu/ACE/ASC/index.html</URL>
        <Description>The ACE Science Center website</Description>

      </InformationURL>
      <InformationURL>

        <Name>Plots</Name>
        <URL>http://www.srl.caltech.edu/ACE/ASC/DATA/level3/swepam/swepam_pa_summary.cgi?LATEST=1</URL>
        <Description>Plots</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>ace-swepam-stea</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>CalTech</ProviderName>

    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/ACE/SWEPAM</InstrumentID>
    <MeasurementType>ThermalPlasma</MeasurementType>
    <TemporalDescription>

      <TimeSpan>

        <StartDate>1997-12-16T00:00:52Z</StartDate>
        <StopDate>2017-07-25T23:57:35Z</StopDate>
      </TimeSpan>
      <Cadence>PT60S</Cadence>
    </TemporalDescription>
    <ObservedRegion>Heliosphere</ObservedRegion>
    <ObservedRegion>Heliosphere.NearEarth</ObservedRegion>
    <Parameter>

      <Name>e- pitch angle : 272 eV</Name>
      <ParameterKey>ace_swepam_stea_epa</ParameterKey>

      <Units>s^3 cm^-6</Units>
      <RenderingHints>

        <DisplayType>Spectrogram</DisplayType>

      </RenderingHints>

      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>

    </Parameter>
  </NumericalData>
</Spase>