<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema  http://www.spase-group.org/data/schema/spase-2_7_0.xsd">
   <Version>2.7.0</Version>
   <NumericalData>
      <ResourceID>spase://ESA/NumericalData/SOHO/EIT/EUV195/Level1/PT12M</ResourceID>
      <NamingAuthority>ESA</NamingAuthority>
      <ResourceType>NumericalData</ResourceType>
      <ResourceHeader>
         <ResourceName>SOHO EIT 195 Level1 FITS Data</ResourceName>
         <ReleaseDate>2020-07-07T21:15:19Z</ReleaseDate>
         <RevisionHistory>
            <RevisionEvent>
               <ReleaseDate>2024-04-17T00:08:46</ReleaseDate>
               <Note>Updated ResourceID to include fits data processing level; Updated Contact</Note>
            </RevisionEvent>
            <RevisionEvent>
               <ReleaseDate>2024-05-22T00:08:46</ReleaseDate>
               <Note>Updated PublicationInfo</Note>
            </RevisionEvent>
            <RevisionEvent>
               <ReleaseDate>2024-06-07T00:08:46</ReleaseDate>
               <Note>Changed the NamingAuthority from NASA to ESA</Note>
            </RevisionEvent>
            <RevisionEvent>
               <ReleaseDate>2025-04-03T00:08:46</ReleaseDate>
               <Note>Updated the wavelength.</Note>
            </RevisionEvent>
            <RevisionEvent>
               <ReleaseDate>2025-06-11T14:45:53</ReleaseDate>
               <Note>Added HelioViewerID to Extension</Note>
            </RevisionEvent>
            <RevisionEvent>
               <ReleaseDate>2025-07-25T00:08:46</ReleaseDate>
               <Note>Updated HelioViewerID</Note>
            </RevisionEvent>
         </RevisionHistory>
         <Description>The SOHO/EIT 195 å Level 1 FITS Data. The Extreme ultraviolet Imaging Telescope (EIT) is an extreme ultraviolet imaging telescope, that will return EUV images of the sun in one of four wavelengths. Its normal incidence multilayer-coated optics will select spectral emission lines from Fe IX (171 å), Fe XII (195 å), Fe XV (284 å), and He II (304 å) to provide sensitive temperature diagnostics in the range from 0.06 MK to 3 MK. The EIT has provided wide-field images of the corona and transition region on the solar disc and up to 1.5 Rs above the solar limb. The telescope has a 45 x 45 arcmin field of view and 2.6 arcsec pixels which provide approximately 5-arcsec spatial resolution. The EIT probes the coronal plasma on a global scale, as well as the underlying cooler and turbulent atmosphere, providing the basis for comparative analyses with observations from both the ground and other SOHO instruments.

This information is from the EIT instrument paper by Delaboudiniere et al. (1995).</Description>
         <PublicationInfo>
            <Authors>The EIT Consortium: Institut d'Astrophysique Spatiale (France); Institut d'Optique Théorique et Appliqueé (France); Naval Research Laboratory (USA); Lockheed Martin Solar and Astrophysics Laboratory (USA); NASA Goddard Space Flight Center (USA); Obvservatoire Royale de Belgique (Belgium); Centre Spatiale de Liège (Belgium); Laboratoire d'Astronomie Spatiale (France)</Authors>
            <PublicationDate>2023-11-22T00:00:00</PublicationDate>
            <PublishedBy>SOHO Science Archive at the European Space Astronomy Centre</PublishedBy>
         </PublicationInfo>
         <Contact>
            <PersonID>spase://SMWG/Person/Frederic.Auchere</PersonID>
            <Role>PrincipalInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://SMWG/Person/Jean-Pierre.Delaboudiniere</PersonID>
            <Role>FormerPI</Role>
         </Contact>
         <Contact>
            <PersonID>spase://SMWG/Person/Jack.Ireland</PersonID>
            <Role>HostContact</Role>
         </Contact>
         <Contact>
            <PersonID>spase://SMWG/Person/Seiji.Yashiro</PersonID>
            <Role>MetadataContact</Role>
         </Contact>
         <InformationURL>
            <Name>EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission</Name>
            <URL>https://doi.org/10.1007/BF00733432</URL>
            <Description>The EIT Instrument paper</Description>
         </InformationURL>
         <PriorID>spase://VSPO/NumericalData/P_SOHO_HDR_EIT_INTENS</PriorID>
         <PriorID>spase://VSPO/NumericalData/SOHO/EIT/PT12M</PriorID>
         <PriorID>spase://NASA/NumericalData/SOHO/EIT/PT12M</PriorID>
         <PriorID>spase://NASA/NumericalData/SOHO/EIT/Level1/PT12M</PriorID>
         <PriorID>spase://ESA/NumericalData/SOHO/EIT/Level1/PT12M</PriorID>
      </ResourceHeader>
      <AccessInformation>
         <RepositoryID>spase://ESA/Repository/SOHOScienceArchive</RepositoryID>
         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <Name>SOHO Science Archive</Name>
            <URL>https://ssa.esac.esa.int/ssa/#/pages/search</URL>
            <Style>Search</Style>
         </AccessURL>
         <Format>FITS</Format>
         <Encoding>GZIP</Encoding>
      </AccessInformation>
      <AccessInformation>
         <RepositoryID>spase://SMWG/Repository/SDAC</RepositoryID>
         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <Name>SOHO/EIT Data Archive at NASA/SDAC</Name>
            <URL>https://umbra.nascom.nasa.gov/pub/eit/l1/</URL>
         </AccessURL>
         <Format>FITS</Format>
      </AccessInformation>
      <AccessInformation>
         <RepositoryID>spase://SMWG/Repository/SDAC</RepositoryID>
         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <Name>Virtual Solar Observatory</Name>
            <URL>https://www.virtualsolar.org/</URL>
         </AccessURL>
         <Format>FITS</Format>
      </AccessInformation>
      <ProviderProcessingLevel>CALIBRATED</ProviderProcessingLevel>
      <InstrumentID>spase://SMWG/Instrument/SOHO/EIT</InstrumentID>
      <MeasurementType>ImageIntensity</MeasurementType>
      <TemporalDescription>
         <TimeSpan>
            <StartDate>1996-01-02T19:12:07</StartDate>
            <RelativeStopDate>-P1M</RelativeStopDate>
         </TimeSpan>
         <Cadence>PT12M</Cadence>
      </TemporalDescription>
      <ObservedRegion>Sun</ObservedRegion>
      <ObservedRegion>Sun.Chromosphere</ObservedRegion>
      <ObservedRegion>Sun.Corona</ObservedRegion>
      <Parameter>
         <Name>EUV Intensity</Name>
         <Cadence>PT12M</Cadence>
         <CoordinateSystem>
            <CoordinateRepresentation>Cartesian</CoordinateRepresentation>
            <CoordinateSystemName>HPC</CoordinateSystemName>
         </CoordinateSystem>
         <Wave>
            <WaveType>Photon</WaveType>
            <WaveQuantity>Intensity</WaveQuantity>
            <WavelengthRange>
               <Low>195</Low>
               <High>195</High>
               <Units>Angstrom</Units>
            </WavelengthRange>
         </Wave>
      </Parameter>
      <Extension><HelioViewerID>1</HelioViewerID></Extension>
   </NumericalData>
</Spase>