diff --git a/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.3.xml b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.3.xml new file mode 100644 index 0000000..27a2989 --- /dev/null +++ b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.3.xml @@ -0,0 +1,106 @@ +<?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-anti.3</ResourceID> + <ResourceHeader> + <ResourceName>sunward flow</ResourceName> + <AlternateName>Fe Flux From Antisun 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.3</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>L2 : fe 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>PT5M</CadenceMin> + <CadenceMax>PT10M</CadenceMax> + </TemporalDescription> + <ObservedRegion>Heliosphere.Inner</ObservedRegion> + <ObservedRegion>Sun.Corona</ObservedRegion> + <Parameter> + <Name>fe flux: sunward</Name> + <ParameterKey>solo_het_asun_feflux</ParameterKey> + <Description>Ferrum 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 unc: sunward</Name> + <ParameterKey>solo_het_asun_feunc</ParameterKey> + <Description>Ferrum flux uncertainty</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>quality flag: sunward</Name> + <ParameterKey>solo_het_asun_3_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> diff --git a/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-north.3.xml b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-north.3.xml new file mode 100644 index 0000000..f1661c4 --- /dev/null +++ b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-north.3.xml @@ -0,0 +1,106 @@ +<?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-north.3</ResourceID> + <ResourceHeader> + <ResourceName>southward flow</ResourceName> + <AlternateName>Fe Flux From North Hemisphere Direction</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.3</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>L2 : fe 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>PT5M</CadenceMin> + <CadenceMax>PT10M</CadenceMax> + </TemporalDescription> + <ObservedRegion>Heliosphere.Inner</ObservedRegion> + <ObservedRegion>Sun.Corona</ObservedRegion> + <Parameter> + <Name>fe flux: southward</Name> + <ParameterKey>solo_het_north_feflux</ParameterKey> + <Description>Ferrum 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 unc: southward</Name> + <ParameterKey>solo_het_north_feunc</ParameterKey> + <Description>Ferrum flux uncertainty</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>quality flag: southward</Name> + <ParameterKey>solo_het_north_3_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> diff --git a/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.3.xml b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.3.xml new file mode 100644 index 0000000..8721989 --- /dev/null +++ b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.3.xml @@ -0,0 +1,106 @@ +<?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-south.3</ResourceID> + <ResourceHeader> + <ResourceName>northward flow</ResourceName> + <AlternateName>Fe Flux From South Hemisphere Direction</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.3</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>L2 : fe 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>PT5M</CadenceMin> + <CadenceMax>PT10M</CadenceMax> + </TemporalDescription> + <ObservedRegion>Heliosphere.Inner</ObservedRegion> + <ObservedRegion>Sun.Corona</ObservedRegion> + <Parameter> + <Name>fe flux: northward</Name> + <ParameterKey>solo_het_south_feflux</ParameterKey> + <Description>Ferrum 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 unc: northward</Name> + <ParameterKey>solo_het_south_feunc</ParameterKey> + <Description>Ferrum flux uncertainty</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>quality flag: northward</Name> + <ParameterKey>solo_het_south_3_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> diff --git a/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.3.xml b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.3.xml new file mode 100644 index 0000000..3347945 --- /dev/null +++ b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.3.xml @@ -0,0 +1,106 @@ +<?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.3</ResourceID> + <ResourceHeader> + <ResourceName>anti-sunward flow</ResourceName> + <AlternateName>Fe 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.3</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>L2 : fe 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>PT5M</CadenceMin> + <CadenceMax>PT10M</CadenceMax> + </TemporalDescription> + <ObservedRegion>Heliosphere.Inner</ObservedRegion> + <ObservedRegion>Sun.Corona</ObservedRegion> + <Parameter> + <Name>fe flux: anti-sunward</Name> + <ParameterKey>solo_het_sun_feflux</ParameterKey> + <Description>Ferrum 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 unc: anti-sunward</Name> + <ParameterKey>solo_het_sun_feunc</ParameterKey> + <Description>Ferrum flux uncertainty</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>quality flag: anti-sunward</Name> + <ParameterKey>solo_het_sun_3_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> diff --git a/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-total.3.xml b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-total.3.xml new file mode 100644 index 0000000..a71d54e --- /dev/null +++ b/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-total.3.xml @@ -0,0 +1,83 @@ +<?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-total.3</ResourceID> + <ResourceHeader> + <ResourceName>total flux</ResourceName> + <AlternateName>Fe Total Flux</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) + </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.3</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>L2 : fe flux</Note> + </Association> + <PriorID>so-het-sun.3</PriorID> + <PriorID>so-het-anti.3</PriorID> + <PriorID>so-het-north.3</PriorID> + <PriorID>so-het-south.3</PriorID> + </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>PT5M</CadenceMin> + <CadenceMax>PT10M</CadenceMax> + </TemporalDescription> + <ObservedRegion>Heliosphere.Inner</ObservedRegion> + <ObservedRegion>Sun.Corona</ObservedRegion> + <Parameter> + <Name>fe flux: total</Name> + <ParameterKey>solo_het_tot_feflux</ParameterKey> + <Description>Ferrum flux</Description> + <Ucd/> + <Units>1/(s cm^2 sr MeV/n)</Units> + <UnitsConversion/> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <Structure> + <Size>16</Size> + </Structure> + </Parameter> +</NumericalData> +</Spase> -- libgit2 0.21.2