mess-eps-spec.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/MESSENGER/EPS/mess-eps-spec</ResourceID>
<ResourceHeader>
<ResourceName>pitch-angle distribution</ResourceName>
<ReleaseDate>2016-04-11T19:14:50Z</ReleaseDate>
<Description>The particle measurements are averaged in 120-second bins.
Pitch angle bins are 11.25 degrees wide, and run from 0 to 180 degrees.
Please note that the D03 detector on EPS has a very high background and is
not useable for any science data product.</Description>
<Contact>
<PersonID>spase://CNES/Person/George.Ho</PersonID>
<Role>DataProducer</Role>
</Contact>
<InformationURL>
<Name>Data product PDS description</Name>
<URL>https://pds-ppi.igpp.ucla.edu/data/MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/DOCUMENT/DDR_SIS/EPPS_DDR_SIS.HTM</URL>
</InformationURL>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://CDPP/Repository/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
<Format>NetCDF</Format>
</AccessInformation>
<ProviderName>PDS</ProviderName>
<ProviderResourceName>MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM</ProviderResourceName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/MESSENGER/EPS</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2008-08-20T16:03:35Z</StartDate>
<StopDate>2015-04-30T15:08:18Z</StopDate>
</TimeSpan>
<Cadence>PT120S</Cadence>
</TemporalDescription>
<ObservedRegion>Mercury</ObservedRegion>
<Caveats>EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel.
The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV).
Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons.
Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products.
</Caveats>
<Parameter>
<Name>countrate</Name>
<ParameterKey>mes_eps_pad</ParameterKey>
<Description></Description>
<Ucd/>
<Units>cnts/s</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
</NumericalData>
</Spase>