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  <Version>2.2.0</Version>
  <Instrument>
    <ResourceID>spase://SMWG/Instrument/Akebono/SMS</ResourceID>
    <ResourceHeader>
      <ResourceName>Suprathermal Mass Spectrometer(SMS)</ResourceName>
      <ReleaseDate>2011-02-23T17:36:22Z</ReleaseDate>
      <Description>The Akebono Suprathermal Mass Spectrometer (SMS) 
is a radio-frequency ion mass spectrometer. It is designed to measure 
the mass composition and velocity distribution (mass-per-charge, 
energy-per-charge and angular distribution in the spacecraft 
spin-plane) of thermal and suprathermal (0.1-4000 eV/q) ions in the 
ionosphere and magnetosphere. It consists of a retarding potential 
analyzer, a 3-stage modified Bennett ion mass spectrometer, and a 
micro-channel plate detector. It can sample ions at 256 mass steps 
over the 1-80 AMU/q mass range, and 256 retarding potential steps 
in the 0.1-25.6V range, and 16 suprathermal energy steps in the 
100-4000 V range. It operates in a number of fast scan and mass 
scan operational modes.
For a detailed description of the SMS instrument and its operation, 
please see B. A. Whalen, J. R. Burrows, A. W. Yau, E. E. Budzinski, 
A. M. Pilon, I. Iwamoto, K. Marubashi, S. Watanabe, H. Mori, and 
E. Sagawa, The suprathermal ion mass spectrometer (SMS) onboard 
the EXOS?D satellite. J. Geomag. Geoelectr. 42, 511-536, 1990 and 
A. W. Yau, E. Drakou, M. J. Greffen, D. J. Knudsen, and E. Sagawa, 
Radio-frequency ion mass spectrometer measurements of thermal ion 
composition, velocity, and temperature: the EXOS-D Suprathermal 
Mass Spectrometer, Geophys. Monogr. Ser., 102, 307-312, 1998.  See also
http://www.darts.isas.jaxa.jp/akbn/readme/readme.sms.txt</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/Andrew.W.Yau</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
    </ResourceHeader>
    <InstrumentType>MassSpectrometer</InstrumentType>
    <InvestigationName>Suprathermal Mass Spectrometer (SMS)</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/Akebono</ObservatoryID>
  </Instrument>
</Spase>
