so-step-rates.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-2.4.1.xsd">
<Version>2.4.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rates</ResourceID>
<ResourceHeader>
<ResourceName>flux</ResourceName>
<AlternateName>Flux averaged over sectors</AlternateName>
<ReleaseDate>2022-01-17T05:52:44Z</ReleaseDate>
<Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates.
STEP is designed to measure electrons and ions in the suprathermal energy range (280 keV). To
allow for the separation of electrons and ions, STEP has 2 different channels, each equipped with its
own solid state detectors for detecting particles:
* Magnet channel. Uses a permanent magnet to deflect electrons, measuring only ions (mostly protons).
* Integral channel. Measures all incoming particles.
The electron flux is recovered by subtracting the magnet channel measurements from the integral
channel ones. Each channel is divided in 15 sectors, disposed in 3 rows of 5 pixels, providing
directional information of the incoming particles within the field of view. An additional pixel, not directly
exposed to the incoming flux, measures the cosmic ray background.</Description>
<Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
<Contact>
<PersonID>spase://CNES/Person/CDPP-AMDA/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>
</InformationURL>
<Association>
<AssociationID>solo-epd-step</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>L2 : rates</Note>
</Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>CDPP/AMDA HAPI Server</Name>
<URL>http://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<Description>Web Service to this product using the HAPI interface.</Description>
</AccessURL>
<Format>CSV</Format>
<Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>CDPP/AMDA Web application</Name>
<URL>http://amda.cdpp.eu</URL>
<Description>Access to Data via CDPP/AMDA Web application.</Description>
</AccessURL>
<Format>CSV</Format>
<Format>VOTable</Format>
<Format>CDF</Format>
<Format>PNG</Format>
<Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<ProviderName>http://soar.esac.esa.int/soar</ProviderName>
<ProviderResourceName>EPD-STEP-RATES</ProviderResourceName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2020-04-30T00:00:11Z</StartDate>
<StopDate>2021-10-22T11:48:29Z</StopDate>
</TimeSpan>
<CadenceMin>PT10S</CadenceMin>
<CadenceMax>PT60S</CadenceMax>
</TemporalDescription>
<ObservedRegion>Heliosphere.Inner</ObservedRegion>
<ObservedRegion>Sun.Corona</ObservedRegion>
<Parameter>
<Name>ion flux</Name>
<ParameterKey>solo_step_mflux</ParameterKey>
<Description>Magnet channel. Uses a permanet magnet to deflect electrons. Measuring only ions (mostly protons)</Description>
<Units>1/(s cm^2 sr MeV)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>ion flux unc</Name>
<ParameterKey>solo_step_munc</ParameterKey>
<Description>Uncertainty in sector averaged magnet channel flux</Description>
<Units>1/(s cm^2 sr MeV)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>ion cntrate</Name>
<ParameterKey>solo_step_mrate</ParameterKey>
<Description>Sector averaged magnet channel count rate</Description>
<Units>cnts/s</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>CountRate</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>el flux</Name>
<ParameterKey>solo_step_eflux</ParameterKey>
<Description>The electron flux is recovered by subtracting the magnet channel measurements from the integral channel ones</Description>
<Units>1/(s cm^2 sr MeV)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>total flux</Name>
<ParameterKey>solo_step_iflux</ParameterKey>
<Description>Integral channel. Measures all incoming particles</Description>
<Units>1/(s cm^2 sr MeV)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>total flux unc</Name>
<ParameterKey>solo_step_iunc</ParameterKey>
<Description>Uncertainty in sector averaged integral channel flux</Description>
<Units>1/(s cm^2 sr MeV)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>total cntrate</Name>
<ParameterKey>solo_step_irate</ParameterKey>
<Description>Sector averaged integral channel count rate</Description>
<Units>cnts/s</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>48</Size>
</Structure>
<Particle>
<ParticleQuantity>CountRate</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>quality flag</Name>
<ParameterKey>solo_step_qf</ParameterKey>
<Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Support>
<SupportQuantity>DataQuality</SupportQuantity>
</Support>
</Parameter>
</NumericalData>
</Spase>