<?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/MESSENGER/EPS/mess-eps-spec</ResourceID>
    <ResourceHeader>
      <ResourceName>pitch-angle distribution</ResourceName>
      <ReleaseDate>2019-06-11T16:04:45Z</ReleaseDate>
      <Description>The particle measurements are averaged in 120-second bins. 

                Pitch angle bins are 11.25 degrees wide, and run from 0 to 180 degrees. 
                          
                Please note that the D03 detector on EPS has a very high background and is 
                not useable for any science data product.</Description>

      <Contact>
        <PersonID>spase://SMWG/Person/George.Ho</PersonID>
        <Role>DataProducer</Role>
      </Contact>
      <InformationURL>
        <Name>Data product PDS description</Name>
        <URL>https://pds-ppi.igpp.ucla.edu/data/MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/DOCUMENT/DDR_SIS/EPPS_DDR_SIS.HTM</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>mess-eps-spec</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>

    <ProcessingLevel>Calibrated</ProcessingLevel>
    <ProviderName>PDS</ProviderName>
    <ProviderResourceName>MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM</ProviderResourceName>
    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/MESSENGER/EPS</InstrumentID>
    <MeasurementType>EnergeticParticles</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2011-03-23T00:00:00Z</StartDate>
        <StopDate>2015-04-30T23:59:58Z</StopDate>
      </TimeSpan>
      <Cadence>PT120S</Cadence>
    </TemporalDescription>
    <ObservedRegion>Mercury</ObservedRegion>
    <Caveats>EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel.  

            The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). 
            Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. 
            Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products.
        </Caveats>

    <Parameter>
      <Name>countrate</Name>
      <ParameterKey>mes_eps_pad</ParameterKey>

      <Units>cnts/s</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Structure>
        <Size>16</Size>
      </Structure>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>EnergyFlux</ParticleQuantity>
      </Particle>
    </Parameter>
  </NumericalData>

</Spase>