ros-ion-az.xml
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<?xml version="1.0" encoding="UTF-8"?>
<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">
<Version>2.3.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Rosetta/IES/ros-ion-az</ResourceID>
<ResourceHeader>
<ResourceName>azimuthal spectra : countrate</ResourceName>
<AlternateName>ion azimuthal spectra : countrate</AlternateName>
<ReleaseDate>2017-03-17T23:15:14Z</ReleaseDate>
<Description>Ion azimuthal (16 anodes) spectra : Counts summed over energies and elevations.
* Azimuth 45 - 90 - Anode #0
* Azimuth 00 - 45 - Anode #1
* Azimuth 315-360 - Anode #2
* Azimuth 310-315 - Anode #3
* Azimuth 305-310 - Anode #4
* Azimuth 300-305 - Anode #5
* Azimuth 295-300 - Anode #6
* Azimuth 290-295 - Anode #7
* Azimuth 285-290 - Anode #8
* Azimuth 280-285 - Anode #9
* Azimuth 275-280 - Anode #10
* Azimuth 270-275 - Anode #11
* Azimuth 225-270 - Anode #12
* Azimuth 180-225 - Anode #13
* Azimuth 135-180 - Anode #14
* Azimuth 90-135 - 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-ion-all</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>ions</Note>
</Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
<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 / ImperialCollege</ProviderName>
<ProviderProcessingLevel>Uncalibrated</ProviderProcessingLevel>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Rosetta/IES</InstrumentID>
<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).
Anodes 13 and 14 are often noisy so caution is recommended when using data from them.
The so-called "fine anodes" (3 - 11) are sometimes combined on board in certain operating modes
because of telemetry limitations. In those cases each of these 9 anodes are given identical values (the
sum/9).
The data from individual fine anodes, when provided, suffer from crosstalk between these anodes and
thus may not be reliable.
It was discovered after launch, apparently as a result of a light leak, that when the sun is incident between
anodes 2 and 3, a high count rate is seen in anode 12. It is also seen in anode 13 when counts in 12 and 13
are combined.</Caveats>
<Parameter>
<Name>ion countrate</Name>
<ParameterKey>ros_ion_az</ParameterKey>
<Description/>
<Ucd/>
<Units>s**-1</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<FillValue>-1</FillValue>
<Particle>
<ParticleType>Ion</ParticleType>
<ParticleQuantity>CountRate</ParticleQuantity>
</Particle>
</Parameter>
</NumericalData>
</Spase>