<?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://cdpp.irap.omp.eu/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd"> <Version>2.2.6</Version> <NumericalData> <ResourceID>spase://CDPP/NumericalData/AMDA/Rosetta/IES/ros-ion-az</ResourceID> <ResourceHeader> <ResourceName>ion azimuthal spectra</ResourceName> <ReleaseDate>2017-03-12T10:48:29Z</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 I * 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://CDPP/Person/James.L.Burch</PersonID> <Role>PrincipalInvestigator</Role> </Contact> <Contact> <PersonID>spase://CDPP/Person/Ray.Goldstein</PersonID> <Role>CoInvestigator</Role> </Contact> <Contact> <PersonID>spase://CDPP/Person/Brad.Trantham</PersonID> <Role>DataProducer</Role> </Contact> <InformationURL> <Name/> <URL/> <Description/> </InformationURL> </ResourceHeader> <AccessInformation> <RepositoryID>spase://SMWG/Repository/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://CDPP/Instrument/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>counts</Name> <ParameterKey>ros_ion_az</ParameterKey> <Description/> <Ucd/> <Units>counts</Units> <UnitsConversion/> <RenderingHints> <DisplayType>Spectrogram</DisplayType> </RenderingHints> <Structure> <Size>16</Size> </Structure> <FillValue>-1</FillValue> <Particle> <ParticleType>Ion</ParticleType> <ParticleQuantity>Counts</ParticleQuantity> </Particle> </Parameter> </NumericalData> </Spase>