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    <ResourceID>spase://NASA/NumericalData/SDO/HMI/Vector_Magnetic_Field/PT720S</ResourceID>
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    <ResourceHeader>
      <ResourceName>SDO/HMI Vector Magnetic Field</ResourceName>
      <DOI>https://doi.org/10.48322/qa09-xp16</DOI>
      <ReleaseDate>2026-07-21T12:07:12Z</ReleaseDate>
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      <Description>The vector magnetic field is derived from full-disk filtergrams collected in a 135-second sequence. (90 seconds after 13 April 2016). The observations are obtained in polarized light at several wavelengths across a spectral line. The filtergrams are calibrated and registered to account for solar rotation before being combined to provide Stokes polarization parameters. The parameters are used to determine the magnetic and other plasma parameters using VFISV, a Milne-Eddington inversion code. The final step is to disambiguate the data, that is to infer the azimuthal direction of the transverse field.</Description>
      <PublicationInfo>
        <Authors>The HMI Consortium: Stanford University (USA); NASA Goddard Space Flight Center (USA); Lockheed Martin Solar and Astrophysics Laboratory (USA); National Center for Atmospheric Research (USA)</Authors>
        <PublicationDate>2011-01-21T00:00:00Z</PublicationDate>
        <PublishedBy>Stanford University</PublishedBy>
      </PublicationInfo>
      <Contact>
        <PersonID>spase://SMWG/Person/Philip.H.Scherrer</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <Contact>
        <PersonID>spase://SMWG/Person/Rick.Bogart</PersonID>
        <Role>GeneralContact</Role>
      </Contact>
      <InformationURL>
        <Name>The HMI website at Stanford</Name>
        <URL>http://hmi.stanford.edu/</URL>
      </InformationURL>
      <InformationURL>
        <Name>The SDO/HMI Instrument paper</Name>
        <URL>https://doi.org/10.1007/s11207-011-9834-2</URL>
      </InformationURL>
      <InformationURL>
        <Name>HelioData</Name>
        <URL>https://helio.data.nasa.gov/dataset/SDO_HMI_Vector_Magnetic_Field_PT720S</URL>
        <Description>The HelioData dataset page provides an overview of the dataset with access links, associated variables, and more.</Description>
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    <AccessInformation>
      <RepositoryID>spase://SMWG/Repository/Stanford/HMI-AIA.JSOC</RepositoryID>
      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
      <AccessURL>
        <Name>JSOC Data Center</Name>
        <URL>http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s[2020-01-01T00:00:00/60m]</URL>
        <Style>Search</Style>
        <Description>Change the date and the time to find the HMI data.</Description>
      </AccessURL>
      <AccessURL>
        <Name>SDO/HMI Data Search via Virtual Solar Observatory</Name>
        <URL>https://sdac.virtualsolar.org/cgi/search?time=1&amp;instrument=HMI&amp;spectrum=1&amp;version=current&amp;build=1</URL>
        <Description>VSO path to JSOC-resident SDO HMI data files</Description>
      </AccessURL>
      <Format>FITS</Format>
    </AccessInformation>
    <InstrumentID>spase://SMWG/Instrument/SDO/HMI</InstrumentID>
    <MeasurementType>Magnetogram</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2010-05-01T00:00:00Z</StartDate>
        <RelativeStopDate>-P3D</RelativeStopDate>
      </TimeSpan>
      <Cadence>PT720S</Cadence>
    </TemporalDescription>
    <ObservedRegion>Sun</ObservedRegion>
    <ObservedRegion>Sun.Photosphere</ObservedRegion>
    <Parameter>
      <Name>FITS Data Array</Name>
      <Description>Vector magnetic field strength</Description>
      <Cadence>PT720S</Cadence>
      <Units>gauss</Units>
      <Field>
        <Qualifier>Vector</Qualifier>
        <FieldQuantity>Magnetic</FieldQuantity>
      </Field>
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        <CoordinateSystem>
          <CoordinateRepresentation>Cartesian</CoordinateRepresentation>
          <CoordinateSystemName>HPC</CoordinateSystemName>
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        <Description>Array size: 4096x4096
Pixel Resolution: 0.504 arcsec</Description>
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