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      <ResourceID>spase://IUGONET/DisplayData/ISEE/IPS/synoptic_map</ResourceID>
      <ResourceHeader>
         <ResourceName>Annual solar wind speed maps</ResourceName>
         <ReleaseDate>2011-04-01T00:00:00</ReleaseDate>
         <ExpirationDate>2199-12-31T00:00:00</ExpirationDate>
         <Description>Annual synoptic source surface maps in the Carrington Rotation Number versus Heliographic Latitude. The source surface was assumed to be at 2.5 solar radii. The IPS-CAT method was applied to derive these maps.</Description>
         <Acknowledgement>References: Kojima, M., M. Tokumaru, H. Watanabe, A. Yokobe, K. Asai, B.V. Jackson, and P.L. Hick, &quot;Heliospheric tomography using interplanetary scintillation observations, II. Latitude and heliocentric distance dependence of solar wind structure at 0.1-1 AU&quot;, Journal of Geophysical Research, Vol.103, pp1981-1989, 1998. Kojima, M., M. Tokumaru, K. Fujiki, K. Hayashi, and B. V. Jackson, &quot;IPS tomographic observations of 3D solar wind structure&quot;, Astronomical and Astrophysical Transactions, Vol. 26, No. 6, 467-476, 2007.</Acknowledgement>
         <Contact>
            <PersonID>spase://IUGONET/Person/Munetoshi.Tokumaru</PersonID>
            <Role>PrincipalInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://IUGONET/Person/Tomoaki.Hori</PersonID>
            <Role>MetadataContact</Role>
         </Contact>
         <Contact>
            <PersonID>spase://IUGONET/Person/ISEE.Metadata.Management.Group</PersonID>
            <Role>MetadataContact</Role>
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      <AccessInformation>
         <RepositoryID>spase://IUGONET/Repository/ISEE/IPS_data_site</RepositoryID>
         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <URL>http://stesun5.stelab.nagoya-u.ac.jp/ips_data.html</URL>
         </AccessURL>
         <Format>GIF</Format>
         <Acknowledgement>References: Kojima, M., M. Tokumaru, H. Watanabe, A. Yokobe, K. Asai, B.V. Jackson, and P.L. Hick, &quot;Heliospheric tomography using interplanetary scintillation observations, II. Latitude and heliocentric distance dependence of solar wind structure at 0.1-1 AU&quot;, Journal of Geophysical Research, Vol.103, pp1981-1989, 1998. Kojima, M., M. Tokumaru, K. Fujiki, K. Hayashi, and B. V. Jackson, &quot;IPS tomographic observations of 3D solar wind structure&quot;, Astronomical and Astrophysical Transactions, Vol. 26, No. 6, 467-476, 2007.</Acknowledgement>
      </AccessInformation>
      <ProcessingLevel>Calibrated</ProcessingLevel>
      <InstrumentID>spase://IUGONET/Instrument/ISEE/IPS/Fuji/uhf_radio_telescope</InstrumentID>
      <InstrumentID>spase://IUGONET/Instrument/ISEE/IPS/Kiso/uhf_radio_telescope</InstrumentID>
      <InstrumentID>spase://IUGONET/Instrument/ISEE/IPS/Sugadaira/uhf_radio_telescope</InstrumentID>
      <InstrumentID>spase://IUGONET/Instrument/ISEE/IPS/Toyokawa/uhf_radio_telescope</InstrumentID>
      <MeasurementType>Irradiance</MeasurementType>
      <TemporalDescription>
         <TimeSpan>
            <StartDate>1985-01-01T00:00:00</StartDate>
            <RelativeStopDate>-P1Y</RelativeStopDate>
         </TimeSpan>
         <Cadence>P1Y</Cadence>
      </TemporalDescription>
      <ObservedRegion>Heliosphere.Inner</ObservedRegion>
      <SpatialCoverage>
         <CoordinateSystem>
            <CoordinateRepresentation>Spherical</CoordinateRepresentation>
            <CoordinateSystemName>GEO</CoordinateSystemName>
         </CoordinateSystem>
         <NorthernmostLatitude>90.0</NorthernmostLatitude>
         <SouthernmostLatitude>-90.0</SouthernmostLatitude>
         <EasternmostLongitude>360.</EasternmostLongitude>
         <WesternmostLongitude>0.</WesternmostLongitude>
      </SpatialCoverage>
      <Keyword>EARTH SCIENCE Sun-earth Interactions Solar Velocity Fields</Keyword>
      <Parameter>
         <Name>Solar wind velocity map</Name>
         <Description>Solar wind velocity distribution on the plane of heliographic latitude v.s. Carrington rotation number remotely measured by Interplanetary Scintillation method</Description>
         <Particle>
            <ParticleType>Ion</ParticleType>
            <ParticleQuantity>Velocity</ParticleQuantity>
         </Particle>
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