<?xml version="1.0" encoding="UTF-8"?>
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  <Version>2.0.0</Version>
  <Instrument>
    <ResourceID>spase://SMWG/Instrument/ISEE3/HECR</ResourceID>
    <ResourceHeader>
      <ResourceName>High-Energy Cosmic Rays</ResourceName>
      <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
      <Description>This experiment was designed to determine the isotopic abundance in the primary cosmic rays for hydrogren through nickel. The instrument used a 10-element solid-state particle telescope consisting of lithium-drifted silicon detectors. Energy ranges measured ran from approximately 20 to approximately 500 MeV/nucleon.  The direction of incident nuclei was obtained from a six-plane drift chamber with 2-deg resolution.</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/Mark.E.Wiedenbeck</PersonID>
        <Role>PrincipalInvestigator</Role>
</Contact>
      <InformationURL>
        <Name>NSSDC's Master Catalog</Name>
        <URL>https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1978-079A-05</URL>
        <Description>Information about the HECR instrument on the ISEE 3 mission.</Description>
</InformationURL>
</ResourceHeader>
    <InstrumentType>EnergeticParticleInstrument</InstrumentType>
    <InvestigationName>High-Energy Cosmic Rays</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/ISEE3</ObservatoryID>
</Instrument>
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