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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-EPT</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>EPD/EPT</ResourceName> | |
| 8 | + <AlternateName>Energetic Particle Detector / Electron Proton Telescope</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 | + * Electron Proton Telescope (EPT). | |
| 16 | + | |
| 17 | + EPT measures electrons and ions (mostly protons) in the | |
| 18 | + lower energy part of the energetic particle spectrum (25 - 500 keV for electrons and from 25 keV to few MeV for ions). | |
| 19 | + It relies on the magnet/foil technique adapted from STEREO/SEPT to separate electrons and ions. | |
| 20 | + EPT consists of 2 double-ended telescopes providing 4 fields of view. Each telescope end has 2 channels, | |
| 21 | + one of them is equipped with a set of magnets deflecting electrons and measures only ions, | |
| 22 | + the other channel contains a foil that stops ions with energies below 400 keV while leaving the electron | |
| 23 | + spectrum unchanged in the measured range.</Description> | |
| 24 | + <Acknowledgement></Acknowledgement> | |
| 25 | + <Contact> | |
| 26 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 27 | + <Role>PrincipalInvestigator</Role> | |
| 28 | + </Contact> | |
| 29 | + <InformationURL> | |
| 30 | + <Name>Instrument Description</Name> | |
| 31 | + <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> | |
| 32 | + </InformationURL> | |
| 33 | + </ResourceHeader> | |
| 34 | + <InstrumentType>SolidStateDetector</InstrumentType> | |
| 35 | + <InvestigationName>EPD</InvestigationName> | |
| 36 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/SolO</ObservatoryID> | |
| 37 | + </Instrument> | |
| 38 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-anti.xml
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| ... | ... | @@ -0,0 +1,168 @@ |
| 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-ept-anti</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>sunward flow</ResourceName> | |
| 8 | + <AlternateName>Ion Flux From AntiSun Direction</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 23 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 24 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 25 | + </Description> | |
| 26 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 27 | + <Contact> | |
| 28 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 29 | + <Role>PrincipalInvestigator</Role> | |
| 30 | + </Contact> | |
| 31 | + <InformationURL> | |
| 32 | + <Name>SolO Archive Support Data</Name> | |
| 33 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 34 | + <Description></Description> | |
| 35 | + </InformationURL> | |
| 36 | + <Association> | |
| 37 | + <AssociationID>solo-epd-eptsun</AssociationID> | |
| 38 | + <AssociationType>PartOf</AssociationType> | |
| 39 | + <Note>L2 : ion flux</Note> | |
| 40 | + </Association> | |
| 41 | + </ResourceHeader> | |
| 42 | + <AccessInformation> | |
| 43 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 44 | + <Availability>Online</Availability> | |
| 45 | + <AccessRights>Open</AccessRights> | |
| 46 | + <AccessURL> | |
| 47 | + <Name>AMDA at CDPP</Name> | |
| 48 | + <URL>http://amda.cdpp.eu</URL> | |
| 49 | + </AccessURL> | |
| 50 | + <Format>Text</Format> | |
| 51 | + <Acknowledgement> | |
| 52 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 53 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 54 | + Universite Paul Sabatier, Toulouse | |
| 55 | + </Acknowledgement> | |
| 56 | + </AccessInformation> | |
| 57 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 58 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 59 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 60 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 61 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 62 | + <TemporalDescription> | |
| 63 | + <TimeSpan> | |
| 64 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 65 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 66 | + </TimeSpan> | |
| 67 | + <CadenceMin>PT5S</CadenceMin> | |
| 68 | + <CadenceMax>PT30S</CadenceMax> | |
| 69 | + </TemporalDescription> | |
| 70 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 71 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 72 | + <Parameter> | |
| 73 | + <Name>ion flux : sunward</Name> | |
| 74 | + <ParameterKey>solo_ept_asun_iflux</ParameterKey> | |
| 75 | + <Description>Particle flux in magnet channel</Description> | |
| 76 | + <Ucd/> | |
| 77 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 78 | + <UnitsConversion/> | |
| 79 | + <RenderingHints> | |
| 80 | + <DisplayType>Spectrogram</DisplayType> | |
| 81 | + </RenderingHints> | |
| 82 | + <Structure> | |
| 83 | + <Size>64</Size> | |
| 84 | + </Structure> | |
| 85 | + </Parameter> | |
| 86 | + <Parameter> | |
| 87 | + <Name>ion flux unc: sunward</Name> | |
| 88 | + <ParameterKey>solo_ept_asun_iunc</ParameterKey> | |
| 89 | + <Description>Uncertainty in ion flux</Description> | |
| 90 | + <Ucd/> | |
| 91 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 92 | + <UnitsConversion/> | |
| 93 | + <RenderingHints> | |
| 94 | + <DisplayType>Spectrogram</DisplayType> | |
| 95 | + </RenderingHints> | |
| 96 | + <Structure> | |
| 97 | + <Size>64</Size> | |
| 98 | + </Structure> | |
| 99 | + </Parameter> | |
| 100 | + <Parameter> | |
| 101 | + <Name>ion cntrate: sunward</Name> | |
| 102 | + <ParameterKey>solo_ept_asun_irate</ParameterKey> | |
| 103 | + <Description>Particle count rate in magnet channel</Description> | |
| 104 | + <Ucd/> | |
| 105 | + <Units>cnts/s</Units> | |
| 106 | + <UnitsConversion/> | |
| 107 | + <RenderingHints> | |
| 108 | + <DisplayType>Spectrogram</DisplayType> | |
| 109 | + </RenderingHints> | |
| 110 | + <Structure> | |
| 111 | + <Size>64</Size> | |
| 112 | + </Structure> | |
| 113 | + </Parameter> | |
| 114 | + <Parameter> | |
| 115 | + <Name>alpha flux: sunward</Name> | |
| 116 | + <ParameterKey>solo_ept_asun_aflux</ParameterKey> | |
| 117 | + <Description>High energy particle flux in magnet channel</Description> | |
| 118 | + <Ucd/> | |
| 119 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 120 | + <UnitsConversion/> | |
| 121 | + <RenderingHints> | |
| 122 | + <DisplayType>Spectrogram</DisplayType> | |
| 123 | + </RenderingHints> | |
| 124 | + <Structure> | |
| 125 | + <Size>8</Size> | |
| 126 | + </Structure> | |
| 127 | + </Parameter> | |
| 128 | + <Parameter> | |
| 129 | + <Name>alpha flux unc: sunward</Name> | |
| 130 | + <ParameterKey>solo_ept_asun_aunc</ParameterKey> | |
| 131 | + <Description>Uncertainty in alpha flux</Description> | |
| 132 | + <Ucd/> | |
| 133 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 134 | + <UnitsConversion/> | |
| 135 | + <RenderingHints> | |
| 136 | + <DisplayType>Spectrogram</DisplayType> | |
| 137 | + </RenderingHints> | |
| 138 | + <Structure> | |
| 139 | + <Size>8</Size> | |
| 140 | + </Structure> | |
| 141 | + </Parameter> | |
| 142 | + <Parameter> | |
| 143 | + <Name>alpha cntrate: sunward</Name> | |
| 144 | + <ParameterKey>solo_ept_asun_arate</ParameterKey> | |
| 145 | + <Description>High energy particle count rate in magnet channel</Description> | |
| 146 | + <Ucd/> | |
| 147 | + <Units>cnts/s</Units> | |
| 148 | + <UnitsConversion/> | |
| 149 | + <RenderingHints> | |
| 150 | + <DisplayType>Spectrogram</DisplayType> | |
| 151 | + </RenderingHints> | |
| 152 | + <Structure> | |
| 153 | + <Size>8</Size> | |
| 154 | + </Structure> | |
| 155 | + </Parameter> | |
| 156 | + <Parameter> | |
| 157 | + <Name>quality flag: sunward</Name> | |
| 158 | + <ParameterKey>solo_ept_asun_qf</ParameterKey> | |
| 159 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
| 160 | + <Ucd/> | |
| 161 | + <Units/> | |
| 162 | + <UnitsConversion/> | |
| 163 | + <RenderingHints> | |
| 164 | + <DisplayType>TimeSeries</DisplayType> | |
| 165 | + </RenderingHints> | |
| 166 | + </Parameter> | |
| 167 | +</NumericalData> | |
| 168 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.anti.xml
0 → 100644
| ... | ... | @@ -0,0 +1,117 @@ |
| 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-ept-e.anti</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>sunward flow</ResourceName> | |
| 8 | + <AlternateName>Electron Flux From AntiSun Direction</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 23 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 24 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 25 | + </Description> | |
| 26 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 27 | + <Contact> | |
| 28 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 29 | + <Role>PrincipalInvestigator</Role> | |
| 30 | + </Contact> | |
| 31 | + <InformationURL> | |
| 32 | + <Name>SolO Archive Support Data</Name> | |
| 33 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 34 | + <Description></Description> | |
| 35 | + </InformationURL> | |
| 36 | + <Association> | |
| 37 | + <AssociationID>solo-epd-eptel</AssociationID> | |
| 38 | + <AssociationType>PartOf</AssociationType> | |
| 39 | + <Note>L2 : electron flux</Note> | |
| 40 | + </Association> | |
| 41 | + </ResourceHeader> | |
| 42 | + <AccessInformation> | |
| 43 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 44 | + <Availability>Online</Availability> | |
| 45 | + <AccessRights>Open</AccessRights> | |
| 46 | + <AccessURL> | |
| 47 | + <Name>AMDA at CDPP</Name> | |
| 48 | + <URL>http://amda.cdpp.eu</URL> | |
| 49 | + </AccessURL> | |
| 50 | + <Format>Text</Format> | |
| 51 | + <Acknowledgement> | |
| 52 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 53 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 54 | + Universite Paul Sabatier, Toulouse | |
| 55 | + </Acknowledgement> | |
| 56 | + </AccessInformation> | |
| 57 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 58 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 59 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 60 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 61 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 62 | + <TemporalDescription> | |
| 63 | + <TimeSpan> | |
| 64 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 65 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 66 | + </TimeSpan> | |
| 67 | + <CadenceMin>PT60S</CadenceMin> | |
| 68 | + <CadenceMax>PT300S</CadenceMax> | |
| 69 | + </TemporalDescription> | |
| 70 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 71 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 72 | + <Caveats>Ions with energies around 500 keV can penetrate the foil and give a signal in the electron | |
| 73 | + channel. In the presence of high ion flux, there could be a considerable contamination from ions in this product.</Caveats> | |
| 74 | + <Parameter> | |
| 75 | + <Name>el flux: sunward</Name> | |
| 76 | + <ParameterKey>solo_ept_anti_eflux</ParameterKey> | |
| 77 | + <Description>Particle flux in foil channel</Description> | |
| 78 | + <Ucd/> | |
| 79 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 80 | + <UnitsConversion/> | |
| 81 | + <RenderingHints> | |
| 82 | + <DisplayType>Spectrogram</DisplayType> | |
| 83 | + </RenderingHints> | |
| 84 | + <Structure> | |
| 85 | + <Size>34</Size> | |
| 86 | + </Structure> | |
| 87 | + </Parameter> | |
| 88 | + <Parameter> | |
| 89 | + <Name>el flux unc: sunward</Name> | |
| 90 | + <ParameterKey>solo_ept_anti_eunc</ParameterKey> | |
| 91 | + <Description>Uncertainty in electron flux</Description> | |
| 92 | + <Ucd/> | |
| 93 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 94 | + <UnitsConversion/> | |
| 95 | + <RenderingHints> | |
| 96 | + <DisplayType>Spectrogram</DisplayType> | |
| 97 | + </RenderingHints> | |
| 98 | + <Structure> | |
| 99 | + <Size>34</Size> | |
| 100 | + </Structure> | |
| 101 | + </Parameter> | |
| 102 | + <Parameter> | |
| 103 | + <Name>el cntrate: sunward</Name> | |
| 104 | + <ParameterKey>solo_ept_anti_erate</ParameterKey> | |
| 105 | + <Description>Particle count rate in foil channel</Description> | |
| 106 | + <Ucd/> | |
| 107 | + <Units>cnts/s</Units> | |
| 108 | + <UnitsConversion/> | |
| 109 | + <RenderingHints> | |
| 110 | + <DisplayType>Spectrogram</DisplayType> | |
| 111 | + </RenderingHints> | |
| 112 | + <Structure> | |
| 113 | + <Size>34</Size> | |
| 114 | + </Structure> | |
| 115 | + </Parameter> | |
| 116 | +</NumericalData> | |
| 117 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.north.xml
0 → 100644
| ... | ... | @@ -0,0 +1,117 @@ |
| 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-ept-e.north</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>southward flow</ResourceName> | |
| 8 | + <AlternateName>Electron Flux From North Ecliptic Hemisphere Direction</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 23 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 24 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 25 | + </Description> | |
| 26 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 27 | + <Contact> | |
| 28 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 29 | + <Role>PrincipalInvestigator</Role> | |
| 30 | + </Contact> | |
| 31 | + <InformationURL> | |
| 32 | + <Name>SolO Archive Support Data</Name> | |
| 33 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 34 | + <Description></Description> | |
| 35 | + </InformationURL> | |
| 36 | + <Association> | |
| 37 | + <AssociationID>solo-epd-eptel</AssociationID> | |
| 38 | + <AssociationType>PartOf</AssociationType> | |
| 39 | + <Note>L2 : electron flux</Note> | |
| 40 | + </Association> | |
| 41 | + </ResourceHeader> | |
| 42 | + <AccessInformation> | |
| 43 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 44 | + <Availability>Online</Availability> | |
| 45 | + <AccessRights>Open</AccessRights> | |
| 46 | + <AccessURL> | |
| 47 | + <Name>AMDA at CDPP</Name> | |
| 48 | + <URL>http://amda.cdpp.eu</URL> | |
| 49 | + </AccessURL> | |
| 50 | + <Format>Text</Format> | |
| 51 | + <Acknowledgement> | |
| 52 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 53 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 54 | + Universite Paul Sabatier, Toulouse | |
| 55 | + </Acknowledgement> | |
| 56 | + </AccessInformation> | |
| 57 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 58 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 59 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 60 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 61 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 62 | + <TemporalDescription> | |
| 63 | + <TimeSpan> | |
| 64 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 65 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 66 | + </TimeSpan> | |
| 67 | + <CadenceMin>PT60S</CadenceMin> | |
| 68 | + <CadenceMax>PT300S</CadenceMax> | |
| 69 | + </TemporalDescription> | |
| 70 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 71 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 72 | + <Caveats>Ions with energies around 500 keV can penetrate the foil and give a signal in the electron | |
| 73 | + channel. In the presence of high ion flux, there could be a considerable contamination from ions in this product.</Caveats> | |
| 74 | + <Parameter> | |
| 75 | + <Name>el flux: southward</Name> | |
| 76 | + <ParameterKey>solo_ept_north_eflux</ParameterKey> | |
| 77 | + <Description>Particle flux in foil channel</Description> | |
| 78 | + <Ucd/> | |
| 79 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 80 | + <UnitsConversion/> | |
| 81 | + <RenderingHints> | |
| 82 | + <DisplayType>Spectrogram</DisplayType> | |
| 83 | + </RenderingHints> | |
| 84 | + <Structure> | |
| 85 | + <Size>34</Size> | |
| 86 | + </Structure> | |
| 87 | + </Parameter> | |
| 88 | + <Parameter> | |
| 89 | + <Name>el flux unc: southward</Name> | |
| 90 | + <ParameterKey>solo_ept_north_eunc</ParameterKey> | |
| 91 | + <Description>Uncertainty in electron flux</Description> | |
| 92 | + <Ucd/> | |
| 93 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 94 | + <UnitsConversion/> | |
| 95 | + <RenderingHints> | |
| 96 | + <DisplayType>Spectrogram</DisplayType> | |
| 97 | + </RenderingHints> | |
| 98 | + <Structure> | |
| 99 | + <Size>34</Size> | |
| 100 | + </Structure> | |
| 101 | + </Parameter> | |
| 102 | + <Parameter> | |
| 103 | + <Name>el cntrate: southward</Name> | |
| 104 | + <ParameterKey>solo_ept_north_erate</ParameterKey> | |
| 105 | + <Description>Particle count rate in foil channel</Description> | |
| 106 | + <Ucd/> | |
| 107 | + <Units>cnts/s</Units> | |
| 108 | + <UnitsConversion/> | |
| 109 | + <RenderingHints> | |
| 110 | + <DisplayType>Spectrogram</DisplayType> | |
| 111 | + </RenderingHints> | |
| 112 | + <Structure> | |
| 113 | + <Size>34</Size> | |
| 114 | + </Structure> | |
| 115 | + </Parameter> | |
| 116 | +</NumericalData> | |
| 117 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.south.xml
0 → 100644
| ... | ... | @@ -0,0 +1,117 @@ |
| 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-ept-e.south</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>northward flow</ResourceName> | |
| 8 | + <AlternateName>Electron Flux From South Ecliptic Hemisphere Direction</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 23 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 24 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 25 | + </Description> | |
| 26 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 27 | + <Contact> | |
| 28 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 29 | + <Role>PrincipalInvestigator</Role> | |
| 30 | + </Contact> | |
| 31 | + <InformationURL> | |
| 32 | + <Name>SolO Archive Support Data</Name> | |
| 33 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 34 | + <Description></Description> | |
| 35 | + </InformationURL> | |
| 36 | + <Association> | |
| 37 | + <AssociationID>solo-epd-eptel</AssociationID> | |
| 38 | + <AssociationType>PartOf</AssociationType> | |
| 39 | + <Note>L2 : electron flux</Note> | |
| 40 | + </Association> | |
| 41 | + </ResourceHeader> | |
| 42 | + <AccessInformation> | |
| 43 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 44 | + <Availability>Online</Availability> | |
| 45 | + <AccessRights>Open</AccessRights> | |
| 46 | + <AccessURL> | |
| 47 | + <Name>AMDA at CDPP</Name> | |
| 48 | + <URL>http://amda.cdpp.eu</URL> | |
| 49 | + </AccessURL> | |
| 50 | + <Format>Text</Format> | |
| 51 | + <Acknowledgement> | |
| 52 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 53 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 54 | + Universite Paul Sabatier, Toulouse | |
| 55 | + </Acknowledgement> | |
| 56 | + </AccessInformation> | |
| 57 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 58 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 59 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 60 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 61 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 62 | + <TemporalDescription> | |
| 63 | + <TimeSpan> | |
| 64 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 65 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 66 | + </TimeSpan> | |
| 67 | + <CadenceMin>PT60S</CadenceMin> | |
| 68 | + <CadenceMax>PT300S</CadenceMax> | |
| 69 | + </TemporalDescription> | |
| 70 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 71 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 72 | + <Caveats>Ions with energies around 500 keV can penetrate the foil and give a signal in the electron | |
| 73 | + channel. In the presence of high ion flux, there could be a considerable contamination from ions in this product.</Caveats> | |
| 74 | + <Parameter> | |
| 75 | + <Name>el flux: nortward</Name> | |
| 76 | + <ParameterKey>solo_ept_south_eflux</ParameterKey> | |
| 77 | + <Description>Particle flux in foil channel</Description> | |
| 78 | + <Ucd/> | |
| 79 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 80 | + <UnitsConversion/> | |
| 81 | + <RenderingHints> | |
| 82 | + <DisplayType>Spectrogram</DisplayType> | |
| 83 | + </RenderingHints> | |
| 84 | + <Structure> | |
| 85 | + <Size>34</Size> | |
| 86 | + </Structure> | |
| 87 | + </Parameter> | |
| 88 | + <Parameter> | |
| 89 | + <Name>el flux unc: northward</Name> | |
| 90 | + <ParameterKey>solo_ept_south_eunc</ParameterKey> | |
| 91 | + <Description>Uncertainty in electron flux</Description> | |
| 92 | + <Ucd/> | |
| 93 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 94 | + <UnitsConversion/> | |
| 95 | + <RenderingHints> | |
| 96 | + <DisplayType>Spectrogram</DisplayType> | |
| 97 | + </RenderingHints> | |
| 98 | + <Structure> | |
| 99 | + <Size>34</Size> | |
| 100 | + </Structure> | |
| 101 | + </Parameter> | |
| 102 | + <Parameter> | |
| 103 | + <Name>el cntrate: northward</Name> | |
| 104 | + <ParameterKey>solo_ept_south_erate</ParameterKey> | |
| 105 | + <Description>Particle count rate in foil channel</Description> | |
| 106 | + <Ucd/> | |
| 107 | + <Units>cnts/s</Units> | |
| 108 | + <UnitsConversion/> | |
| 109 | + <RenderingHints> | |
| 110 | + <DisplayType>Spectrogram</DisplayType> | |
| 111 | + </RenderingHints> | |
| 112 | + <Structure> | |
| 113 | + <Size>34</Size> | |
| 114 | + </Structure> | |
| 115 | + </Parameter> | |
| 116 | +</NumericalData> | |
| 117 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun.xml
0 → 100644
| ... | ... | @@ -0,0 +1,117 @@ |
| 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-ept-e.sun</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>anti-sunward flow</ResourceName> | |
| 8 | + <AlternateName>Ion Flux From Sun Direction ( mean Parker spiral )</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 23 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 24 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 25 | + </Description> | |
| 26 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 27 | + <Contact> | |
| 28 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 29 | + <Role>PrincipalInvestigator</Role> | |
| 30 | + </Contact> | |
| 31 | + <InformationURL> | |
| 32 | + <Name>SolO Archive Support Data</Name> | |
| 33 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 34 | + <Description></Description> | |
| 35 | + </InformationURL> | |
| 36 | + <Association> | |
| 37 | + <AssociationID>solo-epd-eptel</AssociationID> | |
| 38 | + <AssociationType>PartOf</AssociationType> | |
| 39 | + <Note>L2 : electron flux</Note> | |
| 40 | + </Association> | |
| 41 | + </ResourceHeader> | |
| 42 | + <AccessInformation> | |
| 43 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 44 | + <Availability>Online</Availability> | |
| 45 | + <AccessRights>Open</AccessRights> | |
| 46 | + <AccessURL> | |
| 47 | + <Name>AMDA at CDPP</Name> | |
| 48 | + <URL>http://amda.cdpp.eu</URL> | |
| 49 | + </AccessURL> | |
| 50 | + <Format>Text</Format> | |
| 51 | + <Acknowledgement> | |
| 52 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 53 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 54 | + Universite Paul Sabatier, Toulouse | |
| 55 | + </Acknowledgement> | |
| 56 | + </AccessInformation> | |
| 57 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 58 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 59 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 60 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 61 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 62 | + <TemporalDescription> | |
| 63 | + <TimeSpan> | |
| 64 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 65 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 66 | + </TimeSpan> | |
| 67 | + <MinCadence>PT60S</MinCadence> | |
| 68 | + <MaxCadence>PT300S</MaxCadence> | |
| 69 | + </TemporalDescription> | |
| 70 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 71 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 72 | + <Caveats>Ions with energies around 500 keV can penetrate the foil and give a signal in the electron | |
| 73 | + channel. In the presence of high ion flux, there could be a considerable contamination from ions in this product.</Caveats> | |
| 74 | + <Parameter> | |
| 75 | + <Name>el flux: anti-sunward</Name> | |
| 76 | + <ParameterKey>solo_ept_sun_eflux</ParameterKey> | |
| 77 | + <Description>Particle flux in foil channel</Description> | |
| 78 | + <Ucd/> | |
| 79 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 80 | + <UnitsConversion/> | |
| 81 | + <RenderingHints> | |
| 82 | + <DisplayType>Spectrogram</DisplayType> | |
| 83 | + </RenderingHints> | |
| 84 | + <Structure> | |
| 85 | + <Size>34</Size> | |
| 86 | + </Structure> | |
| 87 | + </Parameter> | |
| 88 | + <Parameter> | |
| 89 | + <Name>el flux unc: anti-sunward</Name> | |
| 90 | + <ParameterKey>solo_ept_sun_eunc</ParameterKey> | |
| 91 | + <Description>Uncertainty in electron flux</Description> | |
| 92 | + <Ucd/> | |
| 93 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 94 | + <UnitsConversion/> | |
| 95 | + <RenderingHints> | |
| 96 | + <DisplayType>Spectrogram</DisplayType> | |
| 97 | + </RenderingHints> | |
| 98 | + <Structure> | |
| 99 | + <Size>34</Size> | |
| 100 | + </Structure> | |
| 101 | + </Parameter> | |
| 102 | + <Parameter> | |
| 103 | + <Name>el cntrate: anti-sunward</Name> | |
| 104 | + <ParameterKey>solo_ept_sun_erate</ParameterKey> | |
| 105 | + <Description>Particle count rate in foil channel</Description> | |
| 106 | + <Ucd/> | |
| 107 | + <Units>cnts/s</Units> | |
| 108 | + <UnitsConversion/> | |
| 109 | + <RenderingHints> | |
| 110 | + <DisplayType>Spectrogram</DisplayType> | |
| 111 | + </RenderingHints> | |
| 112 | + <Structure> | |
| 113 | + <Size>34</Size> | |
| 114 | + </Structure> | |
| 115 | + </Parameter> | |
| 116 | +</NumericalData> | |
| 117 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.total.xml
0 → 100644
| ... | ... | @@ -0,0 +1,91 @@ |
| 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-ept-e.total</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>total flux</ResourceName> | |
| 8 | + <AlternateName>Total Electron Flux</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 21 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 22 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 23 | + </Description> | |
| 24 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 25 | + <Contact> | |
| 26 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 27 | + <Role>PrincipalInvestigator</Role> | |
| 28 | + </Contact> | |
| 29 | + <InformationURL> | |
| 30 | + <Name>SolO Archive Support Data</Name> | |
| 31 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 32 | + <Description></Description> | |
| 33 | + </InformationURL> | |
| 34 | + <Association> | |
| 35 | + <AssociationID>solo-epd-eptel</AssociationID> | |
| 36 | + <AssociationType>PartOf</AssociationType> | |
| 37 | + <Note>L2 : electron flux</Note> | |
| 38 | + </Association> | |
| 39 | + <PriorID>so-ept-e.sun</PriorID> | |
| 40 | + <PriorID>so-ept-e.anti</PriorID> | |
| 41 | + <PriorID>so-ept-e.north</PriorID> | |
| 42 | + <PriorID>so-ept-e.south</PriorID> | |
| 43 | + </ResourceHeader> | |
| 44 | + <AccessInformation> | |
| 45 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 46 | + <Availability>Online</Availability> | |
| 47 | + <AccessRights>Open</AccessRights> | |
| 48 | + <AccessURL> | |
| 49 | + <Name>AMDA at CDPP</Name> | |
| 50 | + <URL>http://amda.cdpp.eu</URL> | |
| 51 | + </AccessURL> | |
| 52 | + <Format>Text</Format> | |
| 53 | + <Acknowledgement> | |
| 54 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 55 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 56 | + Universite Paul Sabatier, Toulouse | |
| 57 | + </Acknowledgement> | |
| 58 | + </AccessInformation> | |
| 59 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 60 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 61 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 62 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 63 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 64 | + <TemporalDescription> | |
| 65 | + <TimeSpan> | |
| 66 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 67 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 68 | + </TimeSpan> | |
| 69 | + <CadenceMin>PT60S</CadenceMin> | |
| 70 | + <CadenceMax>PT300S</CadenceMax> | |
| 71 | + </TemporalDescription> | |
| 72 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 73 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 74 | + <Caveats>Ions with energies around 500 keV can penetrate the foil and give a signal in the electron | |
| 75 | + channel. In the presence of high ion flux, there could be a considerable contamination from ions in this product.</Caveats> | |
| 76 | + <Parameter> | |
| 77 | + <Name>el flux: total</Name> | |
| 78 | + <ParameterKey>solo_ept_tot_eflux</ParameterKey> | |
| 79 | + <Description>Particle flux in foil channel</Description> | |
| 80 | + <Ucd/> | |
| 81 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 82 | + <UnitsConversion/> | |
| 83 | + <RenderingHints> | |
| 84 | + <DisplayType>Spectrogram</DisplayType> | |
| 85 | + </RenderingHints> | |
| 86 | + <Structure> | |
| 87 | + <Size>34</Size> | |
| 88 | + </Structure> | |
| 89 | + </Parameter> | |
| 90 | +</NumericalData> | |
| 91 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-north.xml
0 → 100644
| ... | ... | @@ -0,0 +1,168 @@ |
| 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-ept-north</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>southward flow</ResourceName> | |
| 8 | + <AlternateName>Ion Flux From North Ecliptic Hemispere Direction</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 23 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 24 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 25 | + </Description> | |
| 26 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 27 | + <Contact> | |
| 28 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 29 | + <Role>PrincipalInvestigator</Role> | |
| 30 | + </Contact> | |
| 31 | + <InformationURL> | |
| 32 | + <Name>SolO Archive Support Data</Name> | |
| 33 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 34 | + <Description></Description> | |
| 35 | + </InformationURL> | |
| 36 | + <Association> | |
| 37 | + <AssociationID>solo-epd-eptsun</AssociationID> | |
| 38 | + <AssociationType>PartOf</AssociationType> | |
| 39 | + <Note>L2 : ion flux</Note> | |
| 40 | + </Association> | |
| 41 | + </ResourceHeader> | |
| 42 | + <AccessInformation> | |
| 43 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 44 | + <Availability>Online</Availability> | |
| 45 | + <AccessRights>Open</AccessRights> | |
| 46 | + <AccessURL> | |
| 47 | + <Name>AMDA at CDPP</Name> | |
| 48 | + <URL>http://amda.cdpp.eu</URL> | |
| 49 | + </AccessURL> | |
| 50 | + <Format>Text</Format> | |
| 51 | + <Acknowledgement> | |
| 52 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 53 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 54 | + Universite Paul Sabatier, Toulouse | |
| 55 | + </Acknowledgement> | |
| 56 | + </AccessInformation> | |
| 57 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 58 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 59 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 60 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 61 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 62 | + <TemporalDescription> | |
| 63 | + <TimeSpan> | |
| 64 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 65 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 66 | + </TimeSpan> | |
| 67 | + <CadenceMin>PT5S</CadenceMin> | |
| 68 | + <CadenceMax>PT30S</CadenceMax> | |
| 69 | + </TemporalDescription> | |
| 70 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 71 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 72 | + <Parameter> | |
| 73 | + <Name>ion flux: southward</Name> | |
| 74 | + <ParameterKey>solo_ept_north_iflux</ParameterKey> | |
| 75 | + <Description>Particle flux in magnet channel</Description> | |
| 76 | + <Ucd/> | |
| 77 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 78 | + <UnitsConversion/> | |
| 79 | + <RenderingHints> | |
| 80 | + <DisplayType>Spectrogram</DisplayType> | |
| 81 | + </RenderingHints> | |
| 82 | + <Structure> | |
| 83 | + <Size>64</Size> | |
| 84 | + </Structure> | |
| 85 | + </Parameter> | |
| 86 | + <Parameter> | |
| 87 | + <Name>ion flux unc: southward</Name> | |
| 88 | + <ParameterKey>solo_ept_north_iunc</ParameterKey> | |
| 89 | + <Description>Uncertainty in ion flux</Description> | |
| 90 | + <Ucd/> | |
| 91 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 92 | + <UnitsConversion/> | |
| 93 | + <RenderingHints> | |
| 94 | + <DisplayType>Spectrogram</DisplayType> | |
| 95 | + </RenderingHints> | |
| 96 | + <Structure> | |
| 97 | + <Size>64</Size> | |
| 98 | + </Structure> | |
| 99 | + </Parameter> | |
| 100 | + <Parameter> | |
| 101 | + <Name>ion cntrate: southward</Name> | |
| 102 | + <ParameterKey>solo_ept_north_irate</ParameterKey> | |
| 103 | + <Description>Particle count rate in magnet channel</Description> | |
| 104 | + <Ucd/> | |
| 105 | + <Units>cnts/s</Units> | |
| 106 | + <UnitsConversion/> | |
| 107 | + <RenderingHints> | |
| 108 | + <DisplayType>Spectrogram</DisplayType> | |
| 109 | + </RenderingHints> | |
| 110 | + <Structure> | |
| 111 | + <Size>64</Size> | |
| 112 | + </Structure> | |
| 113 | + </Parameter> | |
| 114 | + <Parameter> | |
| 115 | + <Name>alpha flux: southward</Name> | |
| 116 | + <ParameterKey>solo_ept_north_aflux</ParameterKey> | |
| 117 | + <Description>High energy particle flux in magnet channel</Description> | |
| 118 | + <Ucd/> | |
| 119 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 120 | + <UnitsConversion/> | |
| 121 | + <RenderingHints> | |
| 122 | + <DisplayType>Spectrogram</DisplayType> | |
| 123 | + </RenderingHints> | |
| 124 | + <Structure> | |
| 125 | + <Size>8</Size> | |
| 126 | + </Structure> | |
| 127 | + </Parameter> | |
| 128 | + <Parameter> | |
| 129 | + <Name>alpha flux unc: southward</Name> | |
| 130 | + <ParameterKey>solo_ept_north_aunc</ParameterKey> | |
| 131 | + <Description>Uncertainty in alpha flux</Description> | |
| 132 | + <Ucd/> | |
| 133 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 134 | + <UnitsConversion/> | |
| 135 | + <RenderingHints> | |
| 136 | + <DisplayType>Spectrogram</DisplayType> | |
| 137 | + </RenderingHints> | |
| 138 | + <Structure> | |
| 139 | + <Size>8</Size> | |
| 140 | + </Structure> | |
| 141 | + </Parameter> | |
| 142 | + <Parameter> | |
| 143 | + <Name>alpha cntrate: southward</Name> | |
| 144 | + <ParameterKey>solo_ept_north_arate</ParameterKey> | |
| 145 | + <Description>High energy particle count rate in magnet channel</Description> | |
| 146 | + <Ucd/> | |
| 147 | + <Units>cnts/s</Units> | |
| 148 | + <UnitsConversion/> | |
| 149 | + <RenderingHints> | |
| 150 | + <DisplayType>Spectrogram</DisplayType> | |
| 151 | + </RenderingHints> | |
| 152 | + <Structure> | |
| 153 | + <Size>8</Size> | |
| 154 | + </Structure> | |
| 155 | + </Parameter> | |
| 156 | + <Parameter> | |
| 157 | + <Name>quality flag: southward</Name> | |
| 158 | + <ParameterKey>solo_ept_north_qf</ParameterKey> | |
| 159 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
| 160 | + <Ucd/> | |
| 161 | + <Units/> | |
| 162 | + <UnitsConversion/> | |
| 163 | + <RenderingHints> | |
| 164 | + <DisplayType>TimeSeries</DisplayType> | |
| 165 | + </RenderingHints> | |
| 166 | + </Parameter> | |
| 167 | +</NumericalData> | |
| 168 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-south.xml
0 → 100644
| ... | ... | @@ -0,0 +1,169 @@ |
| 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-ept-south</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>northward flow</ResourceName> | |
| 8 | + <AlternateName>Ion Flux From South Ecliptic Hemispere Direction</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID uses Detector looking directon. | |
| 21 | + | |
| 22 | + | |
| 23 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 24 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 25 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 26 | + </Description> | |
| 27 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 28 | + <Contact> | |
| 29 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 30 | + <Role>PrincipalInvestigator</Role> | |
| 31 | + </Contact> | |
| 32 | + <InformationURL> | |
| 33 | + <Name>SolO Archive Support Data</Name> | |
| 34 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 35 | + <Description></Description> | |
| 36 | + </InformationURL> | |
| 37 | + <Association> | |
| 38 | + <AssociationID>solo-epd-eptsun</AssociationID> | |
| 39 | + <AssociationType>PartOf</AssociationType> | |
| 40 | + <Note>L2 : ion flux</Note> | |
| 41 | + </Association> | |
| 42 | + </ResourceHeader> | |
| 43 | + <AccessInformation> | |
| 44 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 45 | + <Availability>Online</Availability> | |
| 46 | + <AccessRights>Open</AccessRights> | |
| 47 | + <AccessURL> | |
| 48 | + <Name>AMDA at CDPP</Name> | |
| 49 | + <URL>http://amda.cdpp.eu</URL> | |
| 50 | + </AccessURL> | |
| 51 | + <Format>Text</Format> | |
| 52 | + <Acknowledgement> | |
| 53 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 54 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 55 | + Universite Paul Sabatier, Toulouse | |
| 56 | + </Acknowledgement> | |
| 57 | + </AccessInformation> | |
| 58 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 59 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 60 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 61 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 62 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 63 | + <TemporalDescription> | |
| 64 | + <TimeSpan> | |
| 65 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 66 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 67 | + </TimeSpan> | |
| 68 | + <CadenceMin>PT5S</CadenceMin> | |
| 69 | + <CadenceMax>PT30S</CadenceMax> | |
| 70 | + </TemporalDescription> | |
| 71 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 72 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 73 | + <Parameter> | |
| 74 | + <Name>ion flux: northward</Name> | |
| 75 | + <ParameterKey>solo_ept_south_iflux</ParameterKey> | |
| 76 | + <Description>Particle flux in magnet channel</Description> | |
| 77 | + <Ucd/> | |
| 78 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 79 | + <UnitsConversion/> | |
| 80 | + <RenderingHints> | |
| 81 | + <DisplayType>Spectrogram</DisplayType> | |
| 82 | + </RenderingHints> | |
| 83 | + <Structure> | |
| 84 | + <Size>64</Size> | |
| 85 | + </Structure> | |
| 86 | + </Parameter> | |
| 87 | + <Parameter> | |
| 88 | + <Name>ion flux unc: northward</Name> | |
| 89 | + <ParameterKey>solo_ept_south_iunc</ParameterKey> | |
| 90 | + <Description>Uncertainty in ion flux</Description> | |
| 91 | + <Ucd/> | |
| 92 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 93 | + <UnitsConversion/> | |
| 94 | + <RenderingHints> | |
| 95 | + <DisplayType>Spectrogram</DisplayType> | |
| 96 | + </RenderingHints> | |
| 97 | + <Structure> | |
| 98 | + <Size>64</Size> | |
| 99 | + </Structure> | |
| 100 | + </Parameter> | |
| 101 | + <Parameter> | |
| 102 | + <Name>ion cntrate: northward</Name> | |
| 103 | + <ParameterKey>solo_ept_south_irate</ParameterKey> | |
| 104 | + <Description>Particle count rate in magnet channel</Description> | |
| 105 | + <Ucd/> | |
| 106 | + <Units>cnts/s</Units> | |
| 107 | + <UnitsConversion/> | |
| 108 | + <RenderingHints> | |
| 109 | + <DisplayType>Spectrogram</DisplayType> | |
| 110 | + </RenderingHints> | |
| 111 | + <Structure> | |
| 112 | + <Size>64</Size> | |
| 113 | + </Structure> | |
| 114 | + </Parameter> | |
| 115 | + <Parameter> | |
| 116 | + <Name>alpha flux: northward</Name> | |
| 117 | + <ParameterKey>solo_ept_south_aflux</ParameterKey> | |
| 118 | + <Description>High energy particle flux in magnet channel</Description> | |
| 119 | + <Ucd/> | |
| 120 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 121 | + <UnitsConversion/> | |
| 122 | + <RenderingHints> | |
| 123 | + <DisplayType>Spectrogram</DisplayType> | |
| 124 | + </RenderingHints> | |
| 125 | + <Structure> | |
| 126 | + <Size>8</Size> | |
| 127 | + </Structure> | |
| 128 | + </Parameter> | |
| 129 | + <Parameter> | |
| 130 | + <Name>alpha flux unc: northward</Name> | |
| 131 | + <ParameterKey>solo_ept_south_aunc</ParameterKey> | |
| 132 | + <Description>Uncertainty in alpha flux</Description> | |
| 133 | + <Ucd/> | |
| 134 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 135 | + <UnitsConversion/> | |
| 136 | + <RenderingHints> | |
| 137 | + <DisplayType>Spectrogram</DisplayType> | |
| 138 | + </RenderingHints> | |
| 139 | + <Structure> | |
| 140 | + <Size>8</Size> | |
| 141 | + </Structure> | |
| 142 | + </Parameter> | |
| 143 | + <Parameter> | |
| 144 | + <Name>alpha cntrate: northward</Name> | |
| 145 | + <ParameterKey>solo_ept_south_arate</ParameterKey> | |
| 146 | + <Description>High energy particle count rate in magnet channel</Description> | |
| 147 | + <Ucd/> | |
| 148 | + <Units>cnts/s</Units> | |
| 149 | + <UnitsConversion/> | |
| 150 | + <RenderingHints> | |
| 151 | + <DisplayType>Spectrogram</DisplayType> | |
| 152 | + </RenderingHints> | |
| 153 | + <Structure> | |
| 154 | + <Size>8</Size> | |
| 155 | + </Structure> | |
| 156 | + </Parameter> | |
| 157 | + <Parameter> | |
| 158 | + <Name>quality flag: northward</Name> | |
| 159 | + <ParameterKey>solo_ept_south_qf</ParameterKey> | |
| 160 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
| 161 | + <Ucd/> | |
| 162 | + <Units/> | |
| 163 | + <UnitsConversion/> | |
| 164 | + <RenderingHints> | |
| 165 | + <DisplayType>TimeSeries</DisplayType> | |
| 166 | + </RenderingHints> | |
| 167 | + </Parameter> | |
| 168 | +</NumericalData> | |
| 169 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-sun.xml
0 → 100644
| ... | ... | @@ -0,0 +1,169 @@ |
| 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-ept-sun</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>anti-sunward flow</ResourceName> | |
| 8 | + <AlternateName>Ion Flux From Sun Direction ( mean Parker spiral )</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. | |
| 11 | + | |
| 12 | + EPT measures electrons and ions in the lower part of the energetic particle spectrum. It | |
| 13 | +effectuates measurements in 4 different fields of view : | |
| 14 | + | |
| 15 | +* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | +* Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | +* Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | +* Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | +Parameter ID suffix is Detector looking directon. | |
| 21 | + . | |
| 22 | + | |
| 23 | +Additionally, EPT has 2 channels that separate electrons and ions: | |
| 24 | +* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 25 | +* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. | |
| 26 | + </Description> | |
| 27 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 28 | + <Contact> | |
| 29 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 30 | + <Role>PrincipalInvestigator</Role> | |
| 31 | + </Contact> | |
| 32 | + <InformationURL> | |
| 33 | + <Name>SolO Archive Support Data</Name> | |
| 34 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 35 | + <Description></Description> | |
| 36 | + </InformationURL> | |
| 37 | + <Association> | |
| 38 | + <AssociationID>solo-epd-eptsun</AssociationID> | |
| 39 | + <AssociationType>PartOf</AssociationType> | |
| 40 | + <Note>L2 : ion flux</Note> | |
| 41 | + </Association> | |
| 42 | + </ResourceHeader> | |
| 43 | + <AccessInformation> | |
| 44 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 45 | + <Availability>Online</Availability> | |
| 46 | + <AccessRights>Open</AccessRights> | |
| 47 | + <AccessURL> | |
| 48 | + <Name>AMDA at CDPP</Name> | |
| 49 | + <URL>http://amda.cdpp.eu</URL> | |
| 50 | + </AccessURL> | |
| 51 | + <Format>Text</Format> | |
| 52 | + <Acknowledgement> | |
| 53 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 54 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 55 | + Universite Paul Sabatier, Toulouse | |
| 56 | + </Acknowledgement> | |
| 57 | + </AccessInformation> | |
| 58 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 59 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 60 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 61 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 62 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 63 | + <TemporalDescription> | |
| 64 | + <TimeSpan> | |
| 65 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 66 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 67 | + </TimeSpan> | |
| 68 | + <CadenceMin>PT5S</CadenceMin> | |
| 69 | + <CadenceMax>PT30S</CadenceMax> | |
| 70 | + </TemporalDescription> | |
| 71 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 72 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 73 | + <Parameter> | |
| 74 | + <Name>ion flux: anti-sunward</Name> | |
| 75 | + <ParameterKey>solo_ept_sun_iflux</ParameterKey> | |
| 76 | + <Description>Particle flux in magnet channel</Description> | |
| 77 | + <Ucd/> | |
| 78 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 79 | + <UnitsConversion/> | |
| 80 | + <RenderingHints> | |
| 81 | + <DisplayType>Spectrogram</DisplayType> | |
| 82 | + </RenderingHints> | |
| 83 | + <Structure> | |
| 84 | + <Size>64</Size> | |
| 85 | + </Structure> | |
| 86 | + </Parameter> | |
| 87 | + <Parameter> | |
| 88 | + <Name>ion flux unc: anti-sunward</Name> | |
| 89 | + <ParameterKey>solo_ept_sun_iunc</ParameterKey> | |
| 90 | + <Description>Uncertainty in ion flux</Description> | |
| 91 | + <Ucd/> | |
| 92 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 93 | + <UnitsConversion/> | |
| 94 | + <RenderingHints> | |
| 95 | + <DisplayType>Spectrogram</DisplayType> | |
| 96 | + </RenderingHints> | |
| 97 | + <Structure> | |
| 98 | + <Size>64</Size> | |
| 99 | + </Structure> | |
| 100 | + </Parameter> | |
| 101 | + <Parameter> | |
| 102 | + <Name>ion cntrate: anti-sunward</Name> | |
| 103 | + <ParameterKey>solo_ept_sun_irate</ParameterKey> | |
| 104 | + <Description>Particle count rate in magnet channel</Description> | |
| 105 | + <Ucd/> | |
| 106 | + <Units>cnts/s</Units> | |
| 107 | + <UnitsConversion/> | |
| 108 | + <RenderingHints> | |
| 109 | + <DisplayType>Spectrogram</DisplayType> | |
| 110 | + </RenderingHints> | |
| 111 | + <Structure> | |
| 112 | + <Size>64</Size> | |
| 113 | + </Structure> | |
| 114 | + </Parameter> | |
| 115 | + <Parameter> | |
| 116 | + <Name>alpha flux: anti-sunward</Name> | |
| 117 | + <ParameterKey>solo_ept_sun_aflux</ParameterKey> | |
| 118 | + <Description>High energy particle flux in magnet channel</Description> | |
| 119 | + <Ucd/> | |
| 120 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 121 | + <UnitsConversion/> | |
| 122 | + <RenderingHints> | |
| 123 | + <DisplayType>Spectrogram</DisplayType> | |
| 124 | + </RenderingHints> | |
| 125 | + <Structure> | |
| 126 | + <Size>8</Size> | |
| 127 | + </Structure> | |
| 128 | + </Parameter> | |
| 129 | + <Parameter> | |
| 130 | + <Name>alpha flux unc: anti-sunward</Name> | |
| 131 | + <ParameterKey>solo_ept_sun_aunc</ParameterKey> | |
| 132 | + <Description>Uncertainty in alpha flux</Description> | |
| 133 | + <Ucd/> | |
| 134 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 135 | + <UnitsConversion/> | |
| 136 | + <RenderingHints> | |
| 137 | + <DisplayType>Spectrogram</DisplayType> | |
| 138 | + </RenderingHints> | |
| 139 | + <Structure> | |
| 140 | + <Size>8</Size> | |
| 141 | + </Structure> | |
| 142 | + </Parameter> | |
| 143 | + <Parameter> | |
| 144 | + <Name>alpha cntrate: anti-sunward</Name> | |
| 145 | + <ParameterKey>solo_ept_sun_arate</ParameterKey> | |
| 146 | + <Description>High energy particle count rate in magnet channel</Description> | |
| 147 | + <Ucd/> | |
| 148 | + <Units>cnts/s</Units> | |
| 149 | + <UnitsConversion/> | |
| 150 | + <RenderingHints> | |
| 151 | + <DisplayType>Spectrogram</DisplayType> | |
| 152 | + </RenderingHints> | |
| 153 | + <Structure> | |
| 154 | + <Size>8</Size> | |
| 155 | + </Structure> | |
| 156 | + </Parameter> | |
| 157 | + <Parameter> | |
| 158 | + <Name>quality flag: anti-sunward</Name> | |
| 159 | + <ParameterKey>solo_ept_sun_qf</ParameterKey> | |
| 160 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
| 161 | + <Ucd/> | |
| 162 | + <Units/> | |
| 163 | + <UnitsConversion/> | |
| 164 | + <RenderingHints> | |
| 165 | + <DisplayType>TimeSeries</DisplayType> | |
| 166 | + </RenderingHints> | |
| 167 | + </Parameter> | |
| 168 | +</NumericalData> | |
| 169 | +</Spase> | |
| ... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-total.xml
0 → 100644
| ... | ... | @@ -0,0 +1,102 @@ |
| 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-ept-total</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>total flux</ResourceName> | |
| 8 | + <AlternateName>Total Ion Flux</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and | |
| 11 | + Proton Telescope, Rates. EPT measures electrons and ions in the lower part of the | |
| 12 | + energetic particle spectrum. It effectuates measurements in 4 different fields of | |
| 13 | + view : | |
| 14 | + | |
| 15 | + * Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. | |
| 16 | + * Sunward Flow. Detector looks opposite to the Sun direction. | |
| 17 | + * Northward Flow. Detector looks towards the south ecliptic hemisphere. | |
| 18 | + * Southward Flow. Detector looks towards the north ecliptic hemisphere. | |
| 19 | + | |
| 20 | + Additionally,EPT has 2 channels that separate electrons and ions: | |
| 21 | + * Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. | |
| 22 | + * Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements.</Description> | |
| 23 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
| 24 | + <Contact> | |
| 25 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
| 26 | + <Role>PrincipalInvestigator</Role> | |
| 27 | + </Contact> | |
| 28 | + <InformationURL> | |
| 29 | + <Name>SolO Archive Support Data</Name> | |
| 30 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
| 31 | + <Description/> | |
| 32 | + </InformationURL> | |
| 33 | + <Association> | |
| 34 | + <AssociationID>solo-epd-eptsun</AssociationID> | |
| 35 | + <AssociationType>PartOf</AssociationType> | |
| 36 | + <Note>L2 : ion flux</Note> | |
| 37 | + </Association> | |
| 38 | + <PriorID>so-ept-sun</PriorID> | |
| 39 | + <PriorID>so-ept-anti</PriorID> | |
| 40 | + <PriorID>so-ept-north</PriorID> | |
| 41 | + <PriorID>so-ept-south</PriorID> | |
| 42 | + </ResourceHeader> | |
| 43 | + <AccessInformation> | |
| 44 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 45 | + <Availability>Online</Availability> | |
| 46 | + <AccessRights>Open</AccessRights> | |
| 47 | + <AccessURL> | |
| 48 | + <Name>AMDA at CDPP</Name> | |
| 49 | + <URL>http://amda.cdpp.eu</URL> | |
| 50 | + </AccessURL> | |
| 51 | + <Format>Text</Format> | |
| 52 | + <Acknowledgement> | |
| 53 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 54 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 55 | + Universite Paul Sabatier, Toulouse | |
| 56 | + </Acknowledgement> | |
| 57 | + </AccessInformation> | |
| 58 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
| 59 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
| 60 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
| 61 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</InstrumentID> | |
| 62 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
| 63 | + <TemporalDescription> | |
| 64 | + <TimeSpan> | |
| 65 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 66 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 67 | + </TimeSpan> | |
| 68 | + <CadenceMin>PT5S</CadenceMin> | |
| 69 | + <CadenceMax>PT30S</CadenceMax> | |
| 70 | + </TemporalDescription> | |
| 71 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 72 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 73 | + <Parameter> | |
| 74 | + <Name>ion flux : total</Name> | |
| 75 | + <ParameterKey>solo_ept_tot_iflux</ParameterKey> | |
| 76 | + <Description>Particle flux in magnet channel</Description> | |
| 77 | + <Ucd/> | |
| 78 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 79 | + <UnitsConversion/> | |
| 80 | + <RenderingHints> | |
| 81 | + <DisplayType>Spectrogram</DisplayType> | |
| 82 | + </RenderingHints> | |
| 83 | + <Structure> | |
| 84 | + <Size>64</Size> | |
| 85 | + </Structure> | |
| 86 | + </Parameter> | |
| 87 | + <Parameter> | |
| 88 | + <Name>alpha flux: total</Name> | |
| 89 | + <ParameterKey>solo_ept_tot_aflux</ParameterKey> | |
| 90 | + <Description>High energy particle flux in magnet channel</Description> | |
| 91 | + <Ucd/> | |
| 92 | + <Units>1/(s cm^2 sr MeV)</Units> | |
| 93 | + <UnitsConversion/> | |
| 94 | + <RenderingHints> | |
| 95 | + <DisplayType>Spectrogram</DisplayType> | |
| 96 | + </RenderingHints> | |
| 97 | + <Structure> | |
| 98 | + <Size>8</Size> | |
| 99 | + </Structure> | |
| 100 | + </Parameter> | |
| 101 | +</NumericalData> | |
| 102 | +</Spase> | |
| ... | ... |