<?xml version="1.0" encoding="UTF-8"?>
<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_1_0.xsd">
  <Version>2.1.0</Version>
  <Instrument>
    <ResourceID>spase://SMWG/Instrument/Wind/SMS</ResourceID>
    <ResourceHeader>
      <ResourceName>Solar Wind and Suprathermal Ion Composition Experiment (SMS)</ResourceName>
      <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
      <Description>The Wind SMS instrument suite is composed of three separate instruments.

          * The SupraThermal Ion Composition Spectrometer (STICS) determines the mass, mass per charge, and energy for ions in the energy range of 6-230 keV/e.
          * The high resolution mass spectrometer (MASS) determines elemental and isotopic abundances from 0.5 to 12 keV/e.
          * Finally, the Solar Wind Ion Composition Spectrometer (SWICS) determines mass, charge, and energy for ions in the energy range of 0.5 to 30 keV/e. The SWICS "stop" MCP experienced a failure resulting in reduced capabilities for this instrument.</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/George.Gloeckler</PersonID>
        <Role>PrincipalInvestigator</Role>
</Contact>
      <InformationURL>
        <Name>Wind spacecraft SMS Documentation</Name>
        <URL>https://link.springer.com/article/10.1007/BF00751327</URL>
        <Description>The Space Science Reviews paper describing the Wind SMS instrument suite.</Description>
</InformationURL>
</ResourceHeader>
    <InstrumentType>EnergeticParticleInstrument</InstrumentType>
    <InvestigationName>Solar Wind and Suprathermal Ion Composition Experiment (SMS)</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/Wind</ObservatoryID>
</Instrument>
</Spase>
