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NumericalData/CDPP-AMDA/Rosetta/IES/ros-elc-azimuth.xml 4.8 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-2_3_1.xsd">
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   <Version>2.3.1</Version>
   <NumericalData>
      <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Rosetta/IES/ros-elc-azimuth</ResourceID>
      <ResourceHeader>
         <ResourceName>azimuthal spectra : eflux</ResourceName>
         <AlternateName>electron azimuthal spectra : dE fluxes</AlternateName>
         <ReleaseDate>2017-03-17T23:15:10Z</ReleaseDate>
         <Description>Electron azimuthal (16 anodes) spectra : differential energy fluxes summed over energies and elevations.
            * Azimuth  180.0-202.5 - Anode #0 
            * Azimuth  202.5-225.0 - Anode #1 
            * Azimuth  225.0-247.5 - Anode #2
            * Azimuth  247.5-270.0 - Anode #3
            * Azimuth  270.0-292.5 - Anode #4
            * Azimuth  292.5-315.0 - Anode #5
            * Azimuth  315.0-337.5 - Anode #6
            * Azimuth  337.5-360.0 - Anode #7
            * Azimuth  00.0 - 22.5 - Anode #8
            * Azimuth  22.5 - 45.0 - Anode #9
            * Azimuth  45.0 - 67.5 - Anode #10
            * Azimuth  67.5 - 90.0 - Anode #11
            * Azimuth  90.0 -112.5 - Anode #12
            * Azimuth  112.5-135.0 - Anode #13
            * Azimuth  135.0-157.5 - Anode #14
            * Azimuth  157.5-180.0 - Anode #15
         </Description>
         <Acknowledgement>Principal Investigator : James L. Burch, SwRI</Acknowledgement>
         <Contact>
            <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
            <Role>PrincipalInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://CNES/Person/Ray.Goldstein</PersonID>
            <Role>CoInvestigator</Role>
         </Contact>
         <Contact>
            <PersonID>spase://CNES/Person/Brad.Trantham</PersonID>
            <Role>DataProducer</Role>
         </Contact>
         <InformationURL>
            <Name/>
            <URL/>
            <Description/>
         </InformationURL>
         <Association>
                <AssociationID>ros-elc-all</AssociationID>
                <AssociationType>PartOf</AssociationType>
                <Note>electrons</Note>
            </Association>
      </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>NetCDF</Format>
         <Acknowledgement/>
      </AccessInformation>
      <ProviderName>SwRI</ProviderName>
      <ProviderResourceName>V02</ProviderResourceName>
      <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
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      <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Rosetta/IES</InstrumentID>
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      <MeasurementType>ThermalPlasma</MeasurementType>
      <TemporalDescription>
         <TimeSpan>
            <StartDate>2010-11-29T23:18:19Z</StartDate>
            <StopDate>2016-09-30T23:58:44Z</StopDate>
         </TimeSpan>
         <Cadence>PT128S</Cadence>
      </TemporalDescription>
      <ObservedRegion>Comet</ObservedRegion>
      <Caveats>Sometimes anode data are combined on board in certain operating modes because of telemetry
limitations. In those cases each of the anodes is given identical values (sum/number of anodes).
Occasionally the electron data exhibit a signal at narrow energy ranges between 200-2000 eV, appearing
as short dashes in spectrograms, as a result of interference from a neighboring instrument (ICA).  
Anode 11 became noisy shortly after launch and since 16 September 2007 data from that anode have not
been downloaded. In those operating modes for which data from 2 or more anodes are combined will
result in the absence of data from one or more anodes adjacent to number 11.
It was discovered after launch, apparently as a result of a light leak, that when the sun is incident between
elevation steps 6 and 7 a high count rate may be seen in anodes 8 - 10.
</Caveats>
      <Parameter>
         <Name>e- flux</Name>
         <ParameterKey>ros_elc_az_flux</ParameterKey>
         <Description/>
         <Ucd/>
         <Units>eV/(m**2*s*sr*eV)</Units>
         <UnitsConversion/>
         <RenderingHints>
            <DisplayType>Spectrogram</DisplayType>
         </RenderingHints>                  
         <Structure>
            <Size>16</Size>
         </Structure>        
         <FillValue>-1</FillValue>
         <Particle>
            <ParticleType>Electron</ParticleType>
            <ParticleQuantity>EnergyFlux</ParticleQuantity>
         </Particle>
      </Parameter>
  </NumericalData>
</Spase>