so-het-sun.1.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://www.spase-group.org/data/schema/spase-2_3_0.xsd">
<Version>2.3.0</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.1</ResourceID>
<ResourceHeader>
<ResourceName>anti-sunward flow</ResourceName>
<AlternateName>Electron HighEnergy ( 38-96 MeV ) / He3 / He4 From Sun Direction ( mean Parker spiral )</AlternateName>
<ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
<Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates.
HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
state detectors and a BGO crystal to provide identification of particle species from the relative energy
deposited in the different detectors. Thus, HET measures count rates for different ion species, as
well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
Anti-Sun, North and South)
Parameter ID uses Detector looking directon.
</Description>
<Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
<Contact>
<PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
<Name>SolO Archive Support Data</Name>
<URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
<Description></Description>
</InformationURL>
<Association>
<AssociationID>solo-epd-het.1</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>L2 : e- 38-96 MeV / he3 / he4 flux</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>Text</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>
<ProviderName>http://soar.esac.esa.int/soar</ProviderName>
<ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
<ProviderAcknowlegment></ProviderAcknowlegment>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2018-09-02T00:00:12Z</StartDate>
<StopDate>2025-08-12T23:59:55Z</StopDate>
</TimeSpan>
<CadenceMin>PT5S</CadenceMin>
<CadenceMax>PT30S</CadenceMax>
</TemporalDescription>
<ObservedRegion>Heliosphere.Inner</ObservedRegion>
<ObservedRegion>Sun.Corona</ObservedRegion>
<Parameter>
<Name>e- HE flux: anti-sunward</Name>
<ParameterKey>solo_het_sun_eheflux</ParameterKey>
<Description>Electron flux in 38 - 96 MeV energy range</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
</Parameter>
<Parameter>
<Name>e- HE flux unc: anti-sunward</Name>
<ParameterKey>solo_het_sun_eheunc</ParameterKey>
<Description>Uncertainty in electron flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
</Parameter>
<Parameter>
<Name>he3 flux: anti-sunward</Name>
<ParameterKey>solo_het_sun_he3flux</ParameterKey>
<Description>He3 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>9</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he3 flux unc: anti-sunward</Name>
<ParameterKey>solo_het_sun_he3unc</ParameterKey>
<Description>Uncertainty in He3 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>9</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he4 flux: anti-sunward</Name>
<ParameterKey>solo_het_sun_he4flux</ParameterKey>
<Description>He4 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>15</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he4 flux unc: anti-sunward</Name>
<ParameterKey>solo_het_sun_he4unc</ParameterKey>
<Description>Uncertainty in He4 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>15</Size>
</Structure>
</Parameter>
<Parameter>
<Name>quality flag: anti-sunward</Name>
<ParameterKey>solo_het_sun_1_qf</ParameterKey>
<Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
<Ucd/>
<Units/>
<UnitsConversion/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
</Parameter>
</NumericalData>
</Spase>