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SolO EPD STEP
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| 1 | +<?xml version="1.0" encoding="UTF-8"?> | ||
| 2 | +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd"> | ||
| 3 | + <Version>2.3.1</Version> | ||
| 4 | + <Instrument> | ||
| 5 | + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</ResourceID> | ||
| 6 | + <ResourceHeader> | ||
| 7 | + <ResourceName>EPD/STEP</ResourceName> | ||
| 8 | + <AlternateName>Energetic Particle Detector / SupraThermal Electrons and Protons</AlternateName> | ||
| 9 | + <ReleaseDate>2018-10-27T18:45:12Z</ReleaseDate> | ||
| 10 | + <Description>The Energetic Particle Detector (EPD) is an instrument suite comprising different sensors that have been designed | ||
| 11 | + to measure the spectra, composition, time variations, and directional distributions ofenergetic particles. | ||
| 12 | + These measurements will be performed over a partly overlapping energy range encompassing a few keV to | ||
| 13 | + 450 MeV/n, with sufficient time, energy, angular, and mass resolution to achieve the mission science goals. | ||
| 14 | + The EPD consists of the following units : | ||
| 15 | + * SupraThermal Electrons and Protons (STEP). | ||
| 16 | + | ||
| 17 | + Designed to measure protons and electrons | ||
| 18 | + at supra-thermal energies (between 2 and 80 keV). It employs two co-aligned sensor heads with a parallel field of view. | ||
| 19 | + One of the sensor heads contains a permanent magnet that deflects electrons out of the nominal field of view, this is referred | ||
| 20 | + to as magnet channel and measures all types of particles except electrons. | ||
| 21 | + The other head measures every particle in the energy range including electrons and is called integral channel. | ||
| 22 | + Each head contains a solid state detector divided in several pixels to achieve angular resolution. For each channel there are | ||
| 23 | + 15 pixels distributed in 3 rows and 5 columns, plus a separate pixel for measuring background. | ||
| 24 | + </Description> | ||
| 25 | + <Acknowledgement></Acknowledgement> | ||
| 26 | + <Contact> | ||
| 27 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | ||
| 28 | + <Role>PrincipalInvestigator</Role> | ||
| 29 | + </Contact> | ||
| 30 | + <InformationURL> | ||
| 31 | + <Name>Instrument Description</Name> | ||
| 32 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data?preview=/60885589/60886052/SO-EPD-PO-TN-0038_iss1_rev1_DPDD.pdf</URL> | ||
| 33 | + </InformationURL> | ||
| 34 | + </ResourceHeader> | ||
| 35 | + <InstrumentType>SolidStateDetector</InstrumentType> | ||
| 36 | + <InvestigationName>EPD</InvestigationName> | ||
| 37 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/SolO</ObservatoryID> | ||
| 38 | + </Instrument> | ||
| 39 | +</Spase> |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rates.xml
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| 1 | +<?xml version="1.0" encoding="UTF-8"?> | ||
| 2 | +<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"> | ||
| 3 | + <Version>2.3.0</Version> | ||
| 4 | + <NumericalData> | ||
| 5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rates</ResourceID> | ||
| 6 | + <ResourceHeader> | ||
| 7 | + <ResourceName>flux</ResourceName> | ||
| 8 | + <AlternateName>Flux averaged over sectors</AlternateName> | ||
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | ||
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates. | ||
| 11 | + | ||
| 12 | + STEP is designed to measure electrons and ions in the suprathermal energy range (280 keV). To | ||
| 13 | + allow for the separation of electrons and ions, STEP has 2 different channels, each equipped with its | ||
| 14 | + own solid state detectors for detecting particles: | ||
| 15 | + * Magnet channel. Uses a permanent magnet to deflect electrons, measuring only ions (mostly protons). | ||
| 16 | + * Integral channel. Measures all incoming particles. | ||
| 17 | + | ||
| 18 | + The electron flux is recovered by subtracting the magnet channel measurements from the integral | ||
| 19 | + channel ones. Each channel is divided in 15 sectors, disposed in 3 rows of 5 pixels, providing | ||
| 20 | + directional information of the incoming particles within the field of view. An additional pixel, not directly | ||
| 21 | + exposed to the incoming flux, measures the cosmic ray background.</Description> | ||
| 22 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | ||
| 23 | + <Contact> | ||
| 24 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | ||
| 25 | + <Role>PrincipalInvestigator</Role> | ||
| 26 | + </Contact> | ||
| 27 | + <InformationURL> | ||
| 28 | + <Name>SolO Archive Support Data</Name> | ||
| 29 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | ||
| 30 | + <Description></Description> | ||
| 31 | + </InformationURL> | ||
| 32 | + <Association> | ||
| 33 | + <AssociationID>solo-epd-step</AssociationID> | ||
| 34 | + <AssociationType>PartOf</AssociationType> | ||
| 35 | + <Note>L2 : rates</Note> | ||
| 36 | + </Association> | ||
| 37 | + </ResourceHeader> | ||
| 38 | + <AccessInformation> | ||
| 39 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | ||
| 40 | + <Availability>Online</Availability> | ||
| 41 | + <AccessRights>Open</AccessRights> | ||
| 42 | + <AccessURL> | ||
| 43 | + <Name>AMDA at CDPP</Name> | ||
| 44 | + <URL>http://amda.cdpp.eu</URL> | ||
| 45 | + </AccessURL> | ||
| 46 | + <Format>Text</Format> | ||
| 47 | + <Acknowledgement> | ||
| 48 | + AMDA is a science analysis system provided by the Centre de Donnees de la | ||
| 49 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | ||
| 50 | + Universite Paul Sabatier, Toulouse | ||
| 51 | + </Acknowledgement> | ||
| 52 | + </AccessInformation> | ||
| 53 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | ||
| 54 | + <ProviderResourceName>EPD-STEP-RATES</ProviderResourceName> | ||
| 55 | + <ProviderAcknowlegment></ProviderAcknowlegment> | ||
| 56 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</InstrumentID> | ||
| 57 | + <MeasurementType>EnergeticParticles</MeasurementType> | ||
| 58 | + <TemporalDescription> | ||
| 59 | + <TimeSpan> | ||
| 60 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | ||
| 61 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | ||
| 62 | + </TimeSpan> | ||
| 63 | + <CadenceMin>PT10S</CadenceMin> | ||
| 64 | + <CadenceMax>PT60S</CadenceMax> | ||
| 65 | + </TemporalDescription> | ||
| 66 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | ||
| 67 | + <ObservedRegion>Sun.Corona</ObservedRegion> | ||
| 68 | + <Parameter> | ||
| 69 | + <Name>ion flux</Name> | ||
| 70 | + <ParameterKey>solo_step_mflux</ParameterKey> | ||
| 71 | + <Description>Magnet channel. Uses a permanet magnet to deflect electrons. Measuring only ions (mostly protons)</Description> | ||
| 72 | + <Ucd/> | ||
| 73 | + <Units>1/(s cm^2 sr MeV)</Units> | ||
| 74 | + <UnitsConversion/> | ||
| 75 | + <RenderingHints> | ||
| 76 | + <DisplayType>Spectrogram</DisplayType> | ||
| 77 | + </RenderingHints> | ||
| 78 | + <Structure> | ||
| 79 | + <Size>48</Size> | ||
| 80 | + </Structure> | ||
| 81 | + </Parameter> | ||
| 82 | + <Parameter> | ||
| 83 | + <Name>ion flux unc</Name> | ||
| 84 | + <ParameterKey>solo_step_munc</ParameterKey> | ||
| 85 | + <Description>Uncertainty in sector averaged magnet channel flux</Description> | ||
| 86 | + <Ucd/> | ||
| 87 | + <Units>1/(s cm^2 sr MeV)</Units> | ||
| 88 | + <UnitsConversion/> | ||
| 89 | + <RenderingHints> | ||
| 90 | + <DisplayType>Spectrogram</DisplayType> | ||
| 91 | + </RenderingHints> | ||
| 92 | + <Structure> | ||
| 93 | + <Size>48</Size> | ||
| 94 | + </Structure> | ||
| 95 | + </Parameter> | ||
| 96 | + <Parameter> | ||
| 97 | + <Name>ion cntrate</Name> | ||
| 98 | + <ParameterKey>solo_step_mrate</ParameterKey> | ||
| 99 | + <Description>Sector averaged magnet channel count rate</Description> | ||
| 100 | + <Ucd/> | ||
| 101 | + <Units>cnts/s</Units> | ||
| 102 | + <UnitsConversion/> | ||
| 103 | + <RenderingHints> | ||
| 104 | + <DisplayType>Spectrogram</DisplayType> | ||
| 105 | + </RenderingHints> | ||
| 106 | + <Structure> | ||
| 107 | + <Size>48</Size> | ||
| 108 | + </Structure> | ||
| 109 | + </Parameter> | ||
| 110 | + <Parameter> | ||
| 111 | + <Name>el flux</Name> | ||
| 112 | + <ParameterKey>solo_step_eflux</ParameterKey> | ||
| 113 | + <Description>The electron flux is recovered by subtracting the magnet channel measurements from the integral channel ones</Description> | ||
| 114 | + <Ucd/> | ||
| 115 | + <Units>1/(s cm^2 sr MeV)</Units> | ||
| 116 | + <UnitsConversion/> | ||
| 117 | + <RenderingHints> | ||
| 118 | + <DisplayType>Spectrogram</DisplayType> | ||
| 119 | + </RenderingHints> | ||
| 120 | + <Structure> | ||
| 121 | + <Size>48</Size> | ||
| 122 | + </Structure> | ||
| 123 | + </Parameter> | ||
| 124 | + <Parameter> | ||
| 125 | + <Name>total flux</Name> | ||
| 126 | + <ParameterKey>solo_step_iflux</ParameterKey> | ||
| 127 | + <Description>Integral channel. Measures all incoming particles</Description> | ||
| 128 | + <Ucd/> | ||
| 129 | + <Units>1/(s cm^2 sr MeV)</Units> | ||
| 130 | + <UnitsConversion/> | ||
| 131 | + <RenderingHints> | ||
| 132 | + <DisplayType>Spectrogram</DisplayType> | ||
| 133 | + </RenderingHints> | ||
| 134 | + <Structure> | ||
| 135 | + <Size>48</Size> | ||
| 136 | + </Structure> | ||
| 137 | + </Parameter> | ||
| 138 | + <Parameter> | ||
| 139 | + <Name>total flux unc</Name> | ||
| 140 | + <ParameterKey>solo_step_iunc</ParameterKey> | ||
| 141 | + <Description>Uncertainty in sector averaged integral channel flux</Description> | ||
| 142 | + <Ucd/> | ||
| 143 | + <Units>1/(s cm^2 sr MeV)</Units> | ||
| 144 | + <UnitsConversion/> | ||
| 145 | + <RenderingHints> | ||
| 146 | + <DisplayType>Spectrogram</DisplayType> | ||
| 147 | + </RenderingHints> | ||
| 148 | + <Structure> | ||
| 149 | + <Size>48</Size> | ||
| 150 | + </Structure> | ||
| 151 | + </Parameter> | ||
| 152 | + <Parameter> | ||
| 153 | + <Name>total cntrate</Name> | ||
| 154 | + <ParameterKey>solo_step_irate</ParameterKey> | ||
| 155 | + <Description>Sector averaged integral channel count rate</Description> | ||
| 156 | + <Ucd/> | ||
| 157 | + <Units>cnts/s</Units> | ||
| 158 | + <UnitsConversion/> | ||
| 159 | + <RenderingHints> | ||
| 160 | + <DisplayType>Spectrogram</DisplayType> | ||
| 161 | + </RenderingHints> | ||
| 162 | + <Structure> | ||
| 163 | + <Size>48</Size> | ||
| 164 | + </Structure> | ||
| 165 | + </Parameter> | ||
| 166 | + <Parameter> | ||
| 167 | + <Name>quality flag</Name> | ||
| 168 | + <ParameterKey>solo_step_qf</ParameterKey> | ||
| 169 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | ||
| 170 | + <Ucd/> | ||
| 171 | + <Units/> | ||
| 172 | + <UnitsConversion/> | ||
| 173 | + <RenderingHints> | ||
| 174 | + <DisplayType>TimeSeries</DisplayType> | ||
| 175 | + </RenderingHints> | ||
| 176 | + </Parameter> | ||
| 177 | +</NumericalData> | ||
| 178 | +</Spase> |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rtn.xml
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| @@ -0,0 +1,89 @@ | @@ -0,0 +1,89 @@ | ||
| 1 | +<?xml version="1.0" encoding="UTF-8"?> | ||
| 2 | +<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"> | ||
| 3 | + <Version>2.3.0</Version> | ||
| 4 | + <NumericalData> | ||
| 5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rtn</ResourceID> | ||
| 6 | + <ResourceHeader> | ||
| 7 | + <ResourceName>flux direction RTN</ResourceName> | ||
| 8 | + <AlternateName></AlternateName> | ||
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | ||
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates.</Description> | ||
| 11 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | ||
| 12 | + <Contact> | ||
| 13 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | ||
| 14 | + <Role>PrincipalInvestigator</Role> | ||
| 15 | + </Contact> | ||
| 16 | + <InformationURL> | ||
| 17 | + <Name>SolO Archive Support Data</Name> | ||
| 18 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | ||
| 19 | + <Description></Description> | ||
| 20 | + </InformationURL> | ||
| 21 | + <Association> | ||
| 22 | + <AssociationID>solo-epd-step</AssociationID> | ||
| 23 | + <AssociationType>PartOf</AssociationType> | ||
| 24 | + <Note>L2 : rates</Note> | ||
| 25 | + </Association> | ||
| 26 | + </ResourceHeader> | ||
| 27 | + <AccessInformation> | ||
| 28 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | ||
| 29 | + <Availability>Online</Availability> | ||
| 30 | + <AccessRights>Open</AccessRights> | ||
| 31 | + <AccessURL> | ||
| 32 | + <Name>AMDA at CDPP</Name> | ||
| 33 | + <URL>http://amda.cdpp.eu</URL> | ||
| 34 | + </AccessURL> | ||
| 35 | + <Format>Text</Format> | ||
| 36 | + <Acknowledgement> | ||
| 37 | + AMDA is a science analysis system provided by the Centre de Donnees de la | ||
| 38 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | ||
| 39 | + Universite Paul Sabatier, Toulouse | ||
| 40 | + </Acknowledgement> | ||
| 41 | + </AccessInformation> | ||
| 42 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | ||
| 43 | + <ProviderResourceName>EPD-STEP-RATES</ProviderResourceName> | ||
| 44 | + <ProviderAcknowlegment></ProviderAcknowlegment> | ||
| 45 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</InstrumentID> | ||
| 46 | + <MeasurementType>EnergeticParticles</MeasurementType> | ||
| 47 | + <TemporalDescription> | ||
| 48 | + <TimeSpan> | ||
| 49 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | ||
| 50 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | ||
| 51 | + </TimeSpan> | ||
| 52 | + <Cadence>PT60S</Cadence> | ||
| 53 | + </TemporalDescription> | ||
| 54 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | ||
| 55 | + <ObservedRegion>Sun.Corona</ObservedRegion> | ||
| 56 | + <Parameter> | ||
| 57 | + <Name>flux direction</Name> | ||
| 58 | + <ParameterKey>solo_step_dir_rtn</ParameterKey> | ||
| 59 | + <Description>Particle flow direction (unit vector) in RTN coordinates</Description> | ||
| 60 | + <Ucd/> | ||
| 61 | + <Units/> | ||
| 62 | + <UnitsConversion/> | ||
| 63 | + <RenderingHints> | ||
| 64 | + <DisplayType>TimeSeries</DisplayType> | ||
| 65 | + </RenderingHints> | ||
| 66 | + <Structure> | ||
| 67 | + <Size>3</Size> | ||
| 68 | + <Element> | ||
| 69 | + <Name>r</Name> | ||
| 70 | + <Qualifier>Component.I</Qualifier> | ||
| 71 | + <Index>1</Index> | ||
| 72 | + <ParameterKey>solo_step_dir_rtn(0)</ParameterKey> | ||
| 73 | + </Element> | ||
| 74 | + <Element> | ||
| 75 | + <Name>t</Name> | ||
| 76 | + <Qualifier>Component.J</Qualifier> | ||
| 77 | + <Index>2</Index> | ||
| 78 | + <ParameterKey>solo_step_dir_rtn(1)</ParameterKey> | ||
| 79 | + </Element> | ||
| 80 | + <Element> | ||
| 81 | + <Name>n</Name> | ||
| 82 | + <Qualifier>Component.K</Qualifier> | ||
| 83 | + <Index>3</Index> | ||
| 84 | + <ParameterKey>solo_step_dir_rtn(2)</ParameterKey> | ||
| 85 | + </Element> | ||
| 86 | + </Structure> | ||
| 87 | + </Parameter> | ||
| 88 | +</NumericalData> | ||
| 89 | +</Spase> |