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NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min.xml 5.94 KB
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<?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_3_0.xsd">
   <Version>2.3.0</Version>
   <NumericalData>
      <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min</ResourceID>
      <ResourceHeader>
          <ResourceName>HET 1min</ResourceName>
          <AlternateName>High Energy Telescope 1 min rate</AlternateName>      
          <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
         <Description>         
             The HET is a cylinder containing a central stack of detector disks and two single detector disks, 
             one at each end. The individual detectors in the central stack have thicknesses of 1000 microns. 
             Three of the detectors in the central stack comprise two 1000-micron disks connected to act as single 
             2000 micron detectors. The end detector disks are 500 microns thick. The front end detector and the 
             outermost detectors at each end of the central stack are each divided into five active elements, 
             a central bulls-eye and four quadrants, each of equal area. Which active area hit on different disks 
             gives directional information on the particle. An outer annular segment of each detector acts as an 
             anti-coincidence shield to detect particles that exit the cylinder before passing through all the detectors. 
             The HET covers electrons up to approximately 6 MeV and protons and heavy ions to at least 100 MeV/n. 
             The lower range overlaps the high end of the Low Energy Telescopes. 
             The measurements are divided into two different sides of the instrument, A and B
         </Description>
         <Acknowledgement>
             Please acknowledge the National Aeronautics and Space Administration, NASA
         </Acknowledgement>
         <Contact>
           <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>
           <Role>PrincipalInvestigator</Role>
         </Contact>
          <Contact>
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              <PersonID>spase://SMWG/Person/Eric.R.Christian</PersonID>
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              <Role>DeputyPI</Role>
          </Contact>
          <InformationURL>
           <Name>PSP/ISoIS Energetic Particle Data - User Guide</Name>
              <URL>https://spdf.sci.gsfc.nasa.gov/pub/data/psp/isois/ISOIS_Data_Glossary.pdf</URL>
         </InformationURL>
         <InformationURL>
            <Name>Parker Solar Probe Mission Instrument web page, JPL</Name>
             <URL>http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments</URL>
         </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> 
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      <ProviderAcknowlegment> 
          Please acknowledge the CDAWeb team at GSFC/SPDF.</ProviderAcknowlegment>
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      <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/epiHi</InstrumentID>
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      <MeasurementType>EnergeticParticles</MeasurementType>
      <TemporalDescription>
         <TimeSpan>
            <StartDate>2018-09-02T00:00:12Z</StartDate>
             <StopDate>2025-08-12T23:59:55Z</StopDate>
         </TimeSpan>
         <Cadence>PT60S</Cadence>
      </TemporalDescription>
      <ObservedRegion>Heliosphere.Inner</ObservedRegion>
      <ObservedRegion>Sun.Corona</ObservedRegion>
      <Parameter>
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         <Name>h+ flux side A</Name>
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         <ParameterKey>psp_het_1min_AHf</ParameterKey>
         <Description>
             Proton flux side A
         </Description>
         <Units>1/cm²/sr/s/(MeV/nuc)</Units>
         <RenderingHints>
              <DisplayType>Spectrogram</DisplayType>
         </RenderingHints>
          <Particle>
              <ParticleQuantity>EnergyFlux</ParticleQuantity>
          </Particle>
      </Parameter>
       <Parameter>
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           <Name>h+ flux side B</Name>
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           <ParameterKey>psp_het_1min_BHf</ParameterKey>
           <Description>
               Proton flux side B
           </Description>
           <Units>1/cm²/sr/s/(MeV/nuc)</Units>
           <RenderingHints>
               <DisplayType>Spectrogram</DisplayType>
           </RenderingHints>
           <Particle>
               <ParticleQuantity>EnergyFlux</ParticleQuantity>
           </Particle>
       </Parameter>
       <Parameter>
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           <Name>he flux side A</Name>
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           <ParameterKey>psp_het_1min_AHef</ParameterKey>
           <Description>
               Helium flux side A
           </Description>
           <Units>1/cm²/sr/s/(MeV/nuc)</Units>
           <RenderingHints>
               <DisplayType>Spectrogram</DisplayType>
           </RenderingHints>
           <Particle>
               <ParticleQuantity>EnergyFlux</ParticleQuantity>
           </Particle>
       </Parameter>
       <Parameter>
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           <Name>he flux side B</Name>
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           <ParameterKey>psp_het_1min_BHef</ParameterKey>
           <Description>
               Helium flux side B
           </Description>
           <Units>1/cm²/sr/s/(MeV/nuc)</Units>
           <RenderingHints>
               <DisplayType>Spectrogram</DisplayType>
           </RenderingHints>
           <Particle>
               <ParticleQuantity>EnergyFlux</ParticleQuantity>
           </Particle>
       </Parameter>
</NumericalData>
</Spase>