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   <Version>2.3.1</Version>
   <NumericalData>

      <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/SPI/psp-spi-asp</ResourceID>

      <ResourceHeader>

          <ResourceName>spectrograms</ResourceName>

          <AlternateName>SWEAP SPANAi Level 3 spectrogramms</AlternateName>      

          <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
         <Description>

             This data set provides spectra of the energy flux versus Energy, Elevation and Azimuth angle  in RTN coordinates.

         </Description>
         <Acknowledgement>
             Please acknowledge the NASA Parker Solar Probe Mission and SWEAP team 
             led by Justin Kasper for use of data.
         </Acknowledgement>
         <Contact>
           <PersonID>spase://SMWG/Person/Justin.C.Kasper</PersonID>
           <Role>PrincipalInvestigator</Role>
         </Contact>
          <Contact>
              <PersonID>spase://SMWG/Person/Davin.Larson</PersonID>
              <Role>DeputyPI</Role>
          </Contact>

          <Association>
              <AssociationID>psp-spi-alpha</AssociationID>
              <AssociationType>PartOf</AssociationType>

              <Note>alphas</Note>

          </Association>

          <InformationURL>
              <Name>Investigation Publication</Name>
              <URL>https://link.springer.com/article/10.1007%2Fs11214-015-0206-3</URL>
              <Description>
                  Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus
              </Description>
         </InformationURL>
      </ResourceHeader>
      <AccessInformation>
         <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <Name>AMDA at CDPP</Name>
            <URL>
                http://amda.cdpp.eu
            </URL>
         </AccessURL>
         <Format>Text</Format>
         <Acknowledgement>
                AMDA is a science analysis system provided by the Centre de Donnees de la 
                Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and 
                Universite Paul Sabatier, Toulouse
         </Acknowledgement>
      </AccessInformation>
      <ProviderName>SPDF</ProviderName> 
       <ProviderResourceName>psp/sweap/spi/l3/spi_sf0a_mom_inst/</ProviderResourceName>
      <ProviderAcknowlegment> 
          Please acknowledge the CDAWeb team at GSFC/SPDF.</ProviderAcknowlegment>
      <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/SPI</InstrumentID>
      <MeasurementType>ThermalPlasma</MeasurementType>
      <TemporalDescription>
         <TimeSpan>
            <StartDate>2018-09-02T00:00:12Z</StartDate>
             <StopDate>2025-08-12T23:59:55Z</StopDate>
         </TimeSpan>
          <CadenceMin>PT0.2S</CadenceMin>
          <CadenceMax>PT30S</CadenceMax>
      </TemporalDescription>
      <ObservedRegion>Heliosphere.Inner</ObservedRegion>
      <ObservedRegion>Sun.Corona</ObservedRegion>

       <Parameter>

           <Name>he++ eflux/ener</Name>

           <ParameterKey>psp_spi_aee</ParameterKey>
           <Description>
               Differential Energy Flux vs Energy
           </Description>

           <Units>eV/cm**2-s-ster-eV</Units>

           <RenderingHints>

               <DisplayType>Spectrogram</DisplayType>

           </RenderingHints>
       </Parameter>
       <Parameter>

           <Name>he++ eflux/theta</Name>

           <ParameterKey>psp_spi_aeth</ParameterKey>
           <Description>

               Differential Energy Flux vs Elevation Instrument Coordinates

           </Description>

           <Units>eV/cm**2-s-ster-eV</Units>

           <RenderingHints>

               <DisplayType>Spectrogram</DisplayType>

           </RenderingHints>
       </Parameter>
       <Parameter>

           <Name>he++ eflux/phi</Name>

           <ParameterKey>psp_spi_aeph</ParameterKey>
           <Description>

               Differential Energy Flux vs Azimuth Instrument Coordinates

           </Description>

           <Units>eV/cm**2-s-ster-eV</Units>

           <RenderingHints>

               <DisplayType>Spectrogram</DisplayType>

           </RenderingHints>
       </Parameter>
       
</NumericalData>
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