solo-sisa-slow.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/solo-sisa-slow</ResourceID>
<ResourceHeader>
<ResourceName>slow mode</ResourceName>
<AlternateName>SIS-A ion anti-sunward flux </AlternateName>
<ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
<Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, Rates.
SIS relies in the time-of-flight technique for identifying ions, providing particle counts for several ion
species in the energy range between 14 keV/n and 20 MeV/n. It consists of 2 telescopes: SIS-A
looking in the sunward direction, along the mean Parker spiral and SIS-B looking anti-sunward. The
main scientific measurements that SIS provides are:
* Particle rates. Count rates of 12 ion species (H, He3, He4, C, N, O, Ne, Mg, Si, S, Ca and Fe) in 21 energy channels.
* Helium histogram. Helium events is collected in a mass histogram for better separation of He3 and He4 intensities.
* PHA data with information about individual events.
</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-sisa</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>L2 : sis-a ; anti-sunward flow</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-SIS</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2018-09-02T00:00:12Z</StartDate>
<StopDate>2025-08-12T23:59:55Z</StopDate>
</TimeSpan>
<Cadence>PT30M</Cadence>
</TemporalDescription>
<ObservedRegion>Heliosphere.Inner</ObservedRegion>
<ObservedRegion>Sun.Corona</ObservedRegion>
<Parameter>
<Name>h flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_hflux</ParameterKey>
<Description>Hydrogen flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>11</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he3 flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_he3flux</ParameterKey>
<Description>Helium-3 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>12</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he4 flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_he4flux</ParameterKey>
<Description>Heliun-4 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>13</Size>
</Structure>
</Parameter>
<Parameter>
<Name>c flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_cflux</ParameterKey>
<Description>Carbon flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
<Parameter>
<Name>n flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_nflux</ParameterKey>
<Description>Nitrogen flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
<Parameter>
<Name>o flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_oflux</ParameterKey>
<Description>Oxygen flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
<Parameter>
<Name>ne flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_neflux</ParameterKey>
<Description>Neon flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
<Parameter>
<Name>mg flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_mgflux</ParameterKey>
<Description>Magnesium flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
<Parameter>
<Name>si flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_siflux</ParameterKey>
<Description>Silicium flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>17</Size>
</Structure>
</Parameter>
<Parameter>
<Name>s flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_sflux</ParameterKey>
<Description>Sulfur flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>17</Size>
</Structure>
</Parameter>
<Parameter>
<Name>ca flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_caflux</ParameterKey>
<Description>Calcium flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
</Parameter>
<Parameter>
<Name>fe flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_feflux</ParameterKey>
<Description>Ferrum flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV/n)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>15</Size>
</Structure>
</Parameter>
<Parameter>
<Name>quality flag: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_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>