<?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_0_0.xsd">
  <Version>2.0.0</Version>
  <Instrument>
    <ResourceID>spase://SMWG/Instrument/Ulysses/DUST</ResourceID>
    <ResourceHeader>
      <ResourceName>Cosmic Dust (GRU/DUST)</ResourceName>
      <AlternateName>DUST</AlternateName>
      <AlternateName>GRU</AlternateName>
      <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
      <Description>The objectives of this investigation are to study particulate matter with masses between 5.E-19 and 5.E-10 g in the heliosphere; to determine its physical and dynamical properties as a function of ecliptic latitude and heliocentric distance; and to investigate its interaction with other interplanetary/interstellar phenomena such as solar radiation, solar wind, heliospheric magnetic field, and interstellar neutral gas. The instrument is a multicoincidence plasma impact detector which measures mass, speed, flight direction and electric charge of individual dust particles. The instrument has a mass of 3.75 kg and uses 2.0 W of power. The data rate in 8 bps.</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/Eberhard.Grun</PersonID>
        <Role>PrincipalInvestigator</Role>
</Contact>
      <InformationURL>
        <Name>NSSDC's Master Catalog</Name>
        <URL>https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1990-090B&amp;ex=7</URL>
        <Description>Information about the Cosmic Dust (GRU/DUST) experiment on the Ulysses mission.</Description>
</InformationURL>
</ResourceHeader>
    <InstrumentType>DustDetector</InstrumentType>
    <InvestigationName>Cosmic Dust (GRU/DUST) on Ulysses</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/Ulysses</ObservatoryID>
</Instrument>
</Spase>
