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NumericalOutput/CDPP-AMDA/TAO/Cassini/tao-cass-sw.xml 5.81 KB
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<?xml version="1.0" encoding="UTF-8"?>
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<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://amda.irap.omp.eu/public/schemas/spase-sim-1_0_0.xsd">
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   <Version>2.2.6</Version>
   <NumericalOutput>
      <ResourceID>spase://CNES/NumericalOutput/CDPP-AMDA/TAO/Juno/tao-cass-sw</ResourceID>
      <ResourceHeader>
         <ResourceName>SW / Input OMNI</ResourceName>
         <AlternateName>Tao SW Cassini / Input OMNI : Cruise Phase</AlternateName>
         <ReleaseDate>2017-02-27T16:52:03Z</ReleaseDate>
         <Description>OMNI solar wind 1-hour data is used as model input. Calculation : IRAP.</Description>
         <Acknowledgement>TBD</Acknowledgement>
         <Contact>
            <PersonID>spase://CNES/Person/Chihiro.Tao</PersonID>
            <Role>PrincipalInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
            <Role>TechnicalContact</Role>
         </Contact>
         <InformationURL>
            <Name>Model Description</Name>
            <URL>http://www.astro.phys.s.chiba-u.ac.jp/netlab/astro/index2-e.html</URL>
            <Description/>
         </InformationURL>
         <InformationURL>
            <Name>Model Article</Name>
            <URL>http://onlinelibrary.wiley.com/doi/10.1029/2004JA010959/abstract</URL>
          </InformationURL>  
      </ResourceHeader>
      <AccessInformation>
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         <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
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         <Availability>Online</Availability>
         <AccessRights>Open</AccessRights>
         <AccessURL>
            <Name>AMDA at CDPP</Name>
            <URL>http://amda.cdpp.eu</URL>
         </AccessURL>
         <Format>Text.ASCII</Format>
         <Acknowledgement> AMDA is a science analysis system provided by the Centre de Donnees de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Universite Paul Sabatier, Toulouse</Acknowledgement>
      </AccessInformation>
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      <SimulationRunID>spase://CNES/SimulationRun/CDPP-AMDA/TAO/Cassini</SimulationRunID>
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      <MeasurementType>ThermalPlasma</MeasurementType>
      <TemporalDescription>
         <TimeSpan>
            <StartDate>2012-01-01T00:00:00Z</StartDate>
            <StopDate>2016-11-02T22:00:00Z</StopDate>
         </TimeSpan>
         <Cadence>PT1H</Cadence>
      </TemporalDescription>
      <SimulatedRegion>Cassini</SimulatedRegion>
      <Caveats>Note an important parameter - angle Cassini-Sun-Earth - which could be considered as quality flag.</Caveats>
      <InputResourceID>spase://CDPP/NumericalData/AMDA/OMNI/omni-hour-all</InputResourceID>
      <Parameter>
         <Name>density</Name>
         <ParameterKey>cass_sw_n</ParameterKey>
         <Description>Solar Wind Proton Number Density, scalar</Description>
         <Units>cm^-3</Units>
         <FillValue>NaN</FillValue>
         <Particle>
            <ParticleType>Proton</ParticleType>
            <ParticleQuantity>NumberDensity</ParticleQuantity>
         </Particle>
      </Parameter>
      <Parameter>
         <Name>velocity</Name>
         <ParameterKey>cass_sw_v</ParameterKey>
         <Description>Solar Wind Bulk Speed</Description>
         <Units>km/s</Units>
         <Structure>
            <Size>3</Size>
            <Element>
               <Name>V r</Name>
               <Qualifier>Component.I</Qualifier>
               <Index>1</Index>
               <ParameterKey>cass_sw_v(0)</ParameterKey>
               <ValidMin/>
               <ValidMax/>
               <FillValue/>
            </Element>
            <Element>
               <Name>V t</Name>
               <Qualifier>Component.J</Qualifier>
               <Index>2</Index>
               <ParameterKey>cass_sw_v(1)</ParameterKey>
               <ValidMin/>
               <ValidMax/>
               <FillValue/>
            </Element>
         </Structure>
         <FillValue>NaN</FillValue>
         <Particle>
            <ParticleType>Proton</ParticleType>
            <ParticleQuantity>Velocity</ParticleQuantity>
         </Particle>
      </Parameter>
      <Parameter>
         <Name>temperature</Name>
         <ParameterKey>cass_sw_t</ParameterKey>
         <Description/>
         <Units>eV</Units>
         <FillValue>NaN</FillValue>
         <Particle>
            <ParticleType>Proton</ParticleType>
            <ParticleQuantity>Temperature</ParticleQuantity>
         </Particle>
      </Parameter>
      <Parameter>
         <Name>dynamic pressure</Name>
         <ParameterKey>cass_sw_pdyn</ParameterKey>
         <Description/>
         <Units>nPa</Units>
         <FillValue>NaN</FillValue>
         <Particle>
            <ParticleType>Proton</ParticleType>
            <ParticleQuantity>Pressure</ParticleQuantity>
         </Particle>
      </Parameter>
      <Parameter>
         <Name>b tangential</Name>
         <ParameterKey>cass_sw_b</ParameterKey>
         <Description/>
         <Units>nT</Units>          
         <FillValue>NaN</FillValue>
         <Field>
            <FieldQuantity>Magnetic</FieldQuantity>
         </Field>
      </Parameter>
      <Parameter>
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         <Name>b radial</Name>
         <ParameterKey>cass_sw_bx</ParameterKey>
         <Description>br along parker spiral computed with tao model outputs</Description>
         <Units>nT</Units>          
         <FillValue>NaN</FillValue>
         <Field>
            <FieldQuantity>Magnetic</FieldQuantity>
         </Field>
      </Parameter>
      <Parameter>
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         <Name>angle Cassini-Sun-Earth</Name>
         <ParameterKey>cass_sw_da</ParameterKey>
         <Description/>
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	 <Units>deg</Units>
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         <FillValue>NaN</FillValue>
         <Support>
            <SupportQuantity>Positional</SupportQuantity>
         </Support>
      </Parameter>
   </NumericalOutput>
</Spase>