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  <NumericalData>
    <ResourceID>spase://NASA/NumericalData/STEREO-B/SECCHI/HI/L2_RAL</ResourceID>
    <NamingAuthority>NASA</NamingAuthority>
    <ResourceType>NumericalData</ResourceType>
    <ResourceHeader>
      <ResourceName>STEREO-B SECCHI HI Level 2 produced by UK Solar System Data Centre</ResourceName>
      <ReleaseDate>2025-12-04T13:31:40Z</ReleaseDate>
      <RevisionHistory>
        <RevisionEvent>
          <ReleaseDate>2020-07-07T21:15:23Z</ReleaseDate>
          <Note>Only known prior ReleaseDate of the metadata</Note>
        </RevisionEvent>
        <RevisionEvent>
          <ReleaseDate>2025-08-05T13:12:32Z</ReleaseDate>
          <Note>Added ObservedRegion(s). ZCB</Note>
        </RevisionEvent>
        <RevisionEvent>
          <ReleaseDate>2025-12-04T13:31:40Z</ReleaseDate>
          <Note>Added MetadataRightsList and RightsList(s). Added ResourceType and NamingAuthority. Updated to 2.7.1. ZCB</Note>
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      <Description>
STEREO-B SECCHI HI Level 2 FITS files produced by the UK Solar System Data Centre, calibrated and background subtracted.  Images stored in FITS files with filenames such as "20140101_180501_24h1A_br11.fts". The meaning of the different parts of this filename is as follows:

* 20140101 is the observation date, 2014-01-01;
* 180501 is the observation time, 18:05:01 UT;
* 2 represents Level-2;
* 4 is a code for the data units, where 4=Dn/Sec/Pixel, b=Mean Solar Brightness (MSB), and t=S10. MSB \&amp; S10 have the diffuse source correction applied;
* h1 or h2 for HI-1 or HI-2;
* A or B for STEREO-A or STEREO-B;
* br for Buffinton/RAL background subtracted--a full running window where the F-corona is computed as the mean of the lowest quartile of pixels;
* 11 is the length of the running window in days, usually either 01 or 11 for HI-1, and 03 or 11 for HI-2.
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      <Contact>
        <PersonID>spase://SMWG/Person/William.T.Thompson</PersonID>
        <Role>GeneralContact</Role>
      </Contact>
      <InformationURL>
        <Name>UKSSDC - STEREO HI data processing documentation</Name>
        <URL>https://www.ukssdc.ac.uk/solar/stereo/documentation/HI_processing_L2_data.html</URL>
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      <PriorID>spase://VSPO/NumericalData/STEREO-B/SECCHI/HI/L2_RAL</PriorID>
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      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
      <AccessURL>
        <Name>UKSSDC - STEREO Archive data access</Name>
        <URL>https://www.ukssdc.ac.uk/solar/stereo/data.html</URL>
      </AccessURL>
      <Format>Text</Format>
    </AccessInformation>
    <AccessInformation>
      <RepositoryID>spase://SMWG/Repository/NASA/GSFC/STEREO_SC</RepositoryID>
      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
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          <RightsName>Creative Commons Zero v1.0 Universal</RightsName>
          <Note>CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products</Note>
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      <AccessURL>
        <Name>STEREO Science Center</Name>
        <URL>https://stereo-ssc.nascom.nasa.gov/data/ins_data/secchi_hi/</URL>
      </AccessURL>
      <Format>Text</Format>
    </AccessInformation>
    <InstrumentID>spase://SMWG/Instrument/STEREO-B/SECCHI</InstrumentID>
    <MeasurementType>ImageIntensity</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2006-10-01T00:00:00Z</StartDate>
        <RelativeStopDate>-P15D</RelativeStopDate>
      </TimeSpan>
    </TemporalDescription>
    <ObservedRegion>Heliosphere.Inner</ObservedRegion>
    <ObservedRegion>Heliosphere.Remote1AU</ObservedRegion>
    <ObservedRegion>Sun.Corona</ObservedRegion>
  </NumericalData>
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