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   <Version>2.5.0</Version>
   <Instrument>
      <ResourceID>spase://IUGONET/Instrument/NIPR/Aurora/SYO/ATV</ResourceID>
      <ResourceHeader>
         <ResourceName>All-sky TV camera (ATV) at Syowa Station, Antarctica.</ResourceName>
         <ReleaseDate>2013-05-14T12:00:00</ReleaseDate>
         <Description>The all-sky television camera (ATV) is a panchromatic high-sensitivity camera recording all-sky auroral images at 30 frames/sec. Until JARE39 (the 39th Japanese Antarctic Research Expedition), a silicon intensifier target (SIT) tube had been used as a light-receiving element. During JARE40, the light-receiving element was changed to a night viewer (Hamamatsu C3100R) and an analog CCD camera, and the installation location was moved from a roof to an optical dark room. The light receiving section consists of a fish eye lens (Fisheye-Nikkor 8mm, F2.8), the night viewer, a relay lens, and the CCD analog camera (Tokyo Electronics CS8300 or Hamamatsu C3077-70). CCD images are recorded at a video rate of 30 frames/sec using S-VHS (until JARE45) or a HDD/DVD recorder (after JARE46).</Description>
         <Contact>
            <PersonID>spase://IUGONET/Person/Akira.Kadokura</PersonID>
            <Role>PrincipalInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://IUGONET/Person/Natsuo.Sato</PersonID>
            <Role>CoInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://IUGONET/Person/Yuka.Sato</PersonID>
            <Role>MetadataContact</Role>
         </Contact>
      </ResourceHeader>
      <InstrumentType>Imager</InstrumentType>
      <InvestigationName>Auroral Observation at Syowa Station</InvestigationName>
      <ObservatoryID>spase://IUGONET/Observatory/NIPR/misc/SYO</ObservatoryID>
   </Instrument>
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