<?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_2_1.xsd">
  <Version>2.2.1</Version>
  <Instrument>
    <ResourceID>spase://SMWG/Instrument/SESAME/FPI</ResourceID>
    <ResourceHeader>
      <ResourceName>SESAME Fabry-Perot Interferometer</ResourceName>
      <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
      <Description>The SESAME FPI (Satellite Experiments Simultaneous with Antarctic MEasurements Fabry-Perot Interferometer) measured Doppler shifts by imaging the wavelengths of oxygen emissions with high resolution and precision. The instrument comprised of five optical components: a scanning mirror that viewed in the 4 cardinal directions at 30 deg elevation; an etalon that consisted of a pair of quartz plates; a 1-m focal length Cassegrain telescope; a 1-nm filter wheel and an imaging photon detector. The experiment contributed to the understanding of airglow and auroral processes in the thermosphere.</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/J.R.Dudeney</PersonID>
        <Role>PrincipalInvestigator</Role>
</Contact>
      <InformationURL>
        <Name>Project Overview</Name>
        <URL>https://link.springer.com/article/10.1007%2FBF00751348</URL>
        <Description>Information about SESAME</Description>
</InformationURL>
</ResourceHeader>
    <InstrumentType>Interferometer</InstrumentType>
    <InvestigationName>Fabry-Perot Interferometer on SESAME</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/SESAME</ObservatoryID>
</Instrument>
</Spase>
