CDPP / CNES

Commit 693caf071b7d7b96a4cfc501f7af04f058da0270

Authored by Elena.Budnik
1 parent e538d737
Exists in master and in 11 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

SolO EPD HET 1 part

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Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET.xml 0 → 100644
  Diff comments   View file @693caf0
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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-HET</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>EPD/HET</ResourceName>
  8 + <AlternateName>Energetic Particle Detector / High Energy 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 + * High Energy Telescope (HET).
  16 +
  17 + HET measures electrons, protons and heavy ions and covers
  18 + the upper energy end of the EPD range. There two HET units, each consisting of a double-sided telescope and an
  19 + electronics box which is shared with EPT. Consequently it provides measurements in 4 distinct fields
  20 + of view (the same as EPT). Each telescope contains 2 solid state detectors (A and B) for each direction and a shared BGO
  21 + scintillator (C). Measuring the characteristics of the energy deposition in the different detectors, HET is able to
  22 + identify particle species in a wide energy range.</Description>
  23 + <Acknowledgement></Acknowledgement>
  24 + <Contact>
  25 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  26 + <Role>PrincipalInvestigator</Role>
  27 + </Contact>
  28 + <InformationURL>
  29 + <Name>Instrument Description</Name>
  30 + <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>
  31 + </InformationURL>
  32 + </ResourceHeader>
  33 + <InstrumentType>SolidStateDetector</InstrumentType>
  34 + <InvestigationName>EPD</InvestigationName>
  35 + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/SolO</ObservatoryID>
  36 + </Instrument>
  37 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-sun.xml
  Diff comments   View file @693caf0
... ... @@ -17,8 +17,7 @@ effectuates measurements in 4 different fields of view :
17 17 * Northward Flow. Detector looks towards the south ecliptic hemisphere.
18 18 * Southward Flow. Detector looks towards the north ecliptic hemisphere.
19 19  
20   -Parameter ID suffix is Detector looking directon.
21   - .
  20 +Parameter ID uses Detector looking directon.
22 21  
23 22 Additionally, EPT has 2 channels that separate electrons and ions:
24 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.
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.xml 0 → 100644
  Diff comments   View file @693caf0
... ... @@ -0,0 +1,121 @@
  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-het-anti</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>sunward flow</ResourceName>
  8 + <AlternateName>Hydrogen Flux From AntiSun Direction ( mean Parker spiral )</AlternateName>
  9 + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
  10 + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates.
  11 +
  12 +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
  13 +state detectors and a BGO crystal to provide identification of particle species from the relative energy
  14 +deposited in the different detectors. Thus, HET measures count rates for different ion species, as
  15 +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
  16 +Anti-Sun, North and South)
  17 +
  18 +Parameter ID uses Detector looking directon.
  19 +
  20 + </Description>
  21 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  22 + <Contact>
  23 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  24 + <Role>PrincipalInvestigator</Role>
  25 + </Contact>
  26 + <InformationURL>
  27 + <Name>SolO Archive Support Data</Name>
  28 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  29 + <Description></Description>
  30 + </InformationURL>
  31 + <Association>
  32 + <AssociationID>solo-epd-het</AssociationID>
  33 + <AssociationType>PartOf</AssociationType>
  34 + <Note>L2 : h flux</Note>
  35 + </Association>
  36 + </ResourceHeader>
  37 + <AccessInformation>
  38 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  39 + <Availability>Online</Availability>
  40 + <AccessRights>Open</AccessRights>
  41 + <AccessURL>
  42 + <Name>AMDA at CDPP</Name>
  43 + <URL>http://amda.cdpp.eu</URL>
  44 + </AccessURL>
  45 + <Format>Text</Format>
  46 + <Acknowledgement>
  47 + AMDA is a science analysis system provided by the Centre de Donnees de la
  48 + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
  49 + Universite Paul Sabatier, Toulouse
  50 + </Acknowledgement>
  51 + </AccessInformation>
  52 + <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
  53 + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
  54 + <ProviderAcknowlegment></ProviderAcknowlegment>
  55 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
  56 + <MeasurementType>EnergeticParticles</MeasurementType>
  57 + <TemporalDescription>
  58 + <TimeSpan>
  59 + <StartDate>2018-09-02T00:00:12Z</StartDate>
  60 + <StopDate>2025-08-12T23:59:55Z</StopDate>
  61 + </TimeSpan>
  62 + <CadenceMin>PT5S</CadenceMin>
  63 + <CadenceMax>PT30S</CadenceMax>
  64 + </TemporalDescription>
  65 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  66 + <ObservedRegion>Sun.Corona</ObservedRegion>
  67 + <Parameter>
  68 + <Name>h flux: sunward</Name>
  69 + <ParameterKey>solo_het_asun_hflux</ParameterKey>
  70 + <Description>Hydrogen flux</Description>
  71 + <Ucd/>
  72 + <Units>1/(s cm^2 sr MeV)</Units>
  73 + <UnitsConversion/>
  74 + <RenderingHints>
  75 + <DisplayType>Spectrogram</DisplayType>
  76 + </RenderingHints>
  77 + <Structure>
  78 + <Size>36</Size>
  79 + </Structure>
  80 + </Parameter>
  81 + <Parameter>
  82 + <Name>h flux unc: sunward</Name>
  83 + <ParameterKey>solo_het_asun_hunc</ParameterKey>
  84 + <Description>Uncertainty in Hydrogen flux</Description>
  85 + <Ucd/>
  86 + <Units>1/(s cm^2 sr MeV)</Units>
  87 + <UnitsConversion/>
  88 + <RenderingHints>
  89 + <DisplayType>Spectrogram</DisplayType>
  90 + </RenderingHints>
  91 + <Structure>
  92 + <Size>36</Size>
  93 + </Structure>
  94 + </Parameter>
  95 + <Parameter>
  96 + <Name>h cntrate: sunward</Name>
  97 + <ParameterKey>solo_het_asun_hrate</ParameterKey>
  98 + <Description>Hydrogen count rate</Description>
  99 + <Ucd/>
  100 + <Units>cnts/s</Units>
  101 + <UnitsConversion/>
  102 + <RenderingHints>
  103 + <DisplayType>Spectrogram</DisplayType>
  104 + </RenderingHints>
  105 + <Structure>
  106 + <Size>36</Size>
  107 + </Structure>
  108 + </Parameter>
  109 + <Parameter>
  110 + <Name>quality flag: sunward</Name>
  111 + <ParameterKey>solo_het_asun_qf</ParameterKey>
  112 + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
  113 + <Ucd/>
  114 + <Units/>
  115 + <UnitsConversion/>
  116 + <RenderingHints>
  117 + <DisplayType>TimeSeries</DisplayType>
  118 + </RenderingHints>
  119 + </Parameter>
  120 +</NumericalData>
  121 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-north.xml 0 → 100644
  Diff comments   View file @693caf0
... ... @@ -0,0 +1,120 @@
  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-het-north</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>southward flow</ResourceName>
  8 + <AlternateName>Hydrogen Flux From North Hemisphere Direction</AlternateName>
  9 + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
  10 + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates.
  11 +
  12 +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
  13 +state detectors and a BGO crystal to provide identification of particle species from the relative energy
  14 +deposited in the different detectors. Thus, HET measures count rates for different ion species, as
  15 +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
  16 +Anti-Sun, North and South)Parameter ID uses Detector looking directon.
  17 +
  18 +Parameter ID uses Detector looking directon.
  19 + </Description>
  20 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  21 + <Contact>
  22 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  23 + <Role>PrincipalInvestigator</Role>
  24 + </Contact>
  25 + <InformationURL>
  26 + <Name>SolO Archive Support Data</Name>
  27 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  28 + <Description></Description>
  29 + </InformationURL>
  30 + <Association>
  31 + <AssociationID>solo-epd-het</AssociationID>
  32 + <AssociationType>PartOf</AssociationType>
  33 + <Note>L2 : h flux</Note>
  34 + </Association>
  35 + </ResourceHeader>
  36 + <AccessInformation>
  37 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  38 + <Availability>Online</Availability>
  39 + <AccessRights>Open</AccessRights>
  40 + <AccessURL>
  41 + <Name>AMDA at CDPP</Name>
  42 + <URL>http://amda.cdpp.eu</URL>
  43 + </AccessURL>
  44 + <Format>Text</Format>
  45 + <Acknowledgement>
  46 + AMDA is a science analysis system provided by the Centre de Donnees de la
  47 + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
  48 + Universite Paul Sabatier, Toulouse
  49 + </Acknowledgement>
  50 + </AccessInformation>
  51 + <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
  52 + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
  53 + <ProviderAcknowlegment></ProviderAcknowlegment>
  54 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
  55 + <MeasurementType>EnergeticParticles</MeasurementType>
  56 + <TemporalDescription>
  57 + <TimeSpan>
  58 + <StartDate>2018-09-02T00:00:12Z</StartDate>
  59 + <StopDate>2025-08-12T23:59:55Z</StopDate>
  60 + </TimeSpan>
  61 + <CadenceMin>PT5S</CadenceMin>
  62 + <CadenceMax>PT30S</CadenceMax>
  63 + </TemporalDescription>
  64 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  65 + <ObservedRegion>Sun.Corona</ObservedRegion>
  66 + <Parameter>
  67 + <Name>h flux: southward</Name>
  68 + <ParameterKey>solo_het_north_hflux</ParameterKey>
  69 + <Description>Hydrogen flux</Description>
  70 + <Ucd/>
  71 + <Units>1/(s cm^2 sr MeV)</Units>
  72 + <UnitsConversion/>
  73 + <RenderingHints>
  74 + <DisplayType>Spectrogram</DisplayType>
  75 + </RenderingHints>
  76 + <Structure>
  77 + <Size>36</Size>
  78 + </Structure>
  79 + </Parameter>
  80 + <Parameter>
  81 + <Name>h flux unc: southward</Name>
  82 + <ParameterKey>solo_het_north_hunc</ParameterKey>
  83 + <Description>Uncertainty in Hydrogen flux</Description>
  84 + <Ucd/>
  85 + <Units>1/(s cm^2 sr MeV)</Units>
  86 + <UnitsConversion/>
  87 + <RenderingHints>
  88 + <DisplayType>Spectrogram</DisplayType>
  89 + </RenderingHints>
  90 + <Structure>
  91 + <Size>36</Size>
  92 + </Structure>
  93 + </Parameter>
  94 + <Parameter>
  95 + <Name>h cntrate: southward</Name>
  96 + <ParameterKey>solo_het_north_hrate</ParameterKey>
  97 + <Description>Hydrogen count rate</Description>
  98 + <Ucd/>
  99 + <Units>cnts/s</Units>
  100 + <UnitsConversion/>
  101 + <RenderingHints>
  102 + <DisplayType>Spectrogram</DisplayType>
  103 + </RenderingHints>
  104 + <Structure>
  105 + <Size>36</Size>
  106 + </Structure>
  107 + </Parameter>
  108 + <Parameter>
  109 + <Name>quality flag: southward</Name>
  110 + <ParameterKey>solo_het_north_qf</ParameterKey>
  111 + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
  112 + <Ucd/>
  113 + <Units/>
  114 + <UnitsConversion/>
  115 + <RenderingHints>
  116 + <DisplayType>TimeSeries</DisplayType>
  117 + </RenderingHints>
  118 + </Parameter>
  119 +</NumericalData>
  120 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.xml 0 → 100644
  Diff comments   View file @693caf0
... ... @@ -0,0 +1,120 @@
  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-het-south</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>northward flow</ResourceName>
  8 + <AlternateName>Hydrogen Flux From South Hemisphere Direction</AlternateName>
  9 + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
  10 + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates.
  11 +
  12 +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
  13 +state detectors and a BGO crystal to provide identification of particle species from the relative energy
  14 +deposited in the different detectors. Thus, HET measures count rates for different ion species, as
  15 +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
  16 +Anti-Sun, North and South)
  17 +
  18 +Parameter ID suffix is Detector looking directon.
  19 + </Description>
  20 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  21 + <Contact>
  22 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  23 + <Role>PrincipalInvestigator</Role>
  24 + </Contact>
  25 + <InformationURL>
  26 + <Name>SolO Archive Support Data</Name>
  27 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  28 + <Description></Description>
  29 + </InformationURL>
  30 + <Association>
  31 + <AssociationID>solo-epd-het</AssociationID>
  32 + <AssociationType>PartOf</AssociationType>
  33 + <Note>L2 : h flux</Note>
  34 + </Association>
  35 + </ResourceHeader>
  36 + <AccessInformation>
  37 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  38 + <Availability>Online</Availability>
  39 + <AccessRights>Open</AccessRights>
  40 + <AccessURL>
  41 + <Name>AMDA at CDPP</Name>
  42 + <URL>http://amda.cdpp.eu</URL>
  43 + </AccessURL>
  44 + <Format>Text</Format>
  45 + <Acknowledgement>
  46 + AMDA is a science analysis system provided by the Centre de Donnees de la
  47 + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
  48 + Universite Paul Sabatier, Toulouse
  49 + </Acknowledgement>
  50 + </AccessInformation>
  51 + <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
  52 + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
  53 + <ProviderAcknowlegment></ProviderAcknowlegment>
  54 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
  55 + <MeasurementType>EnergeticParticles</MeasurementType>
  56 + <TemporalDescription>
  57 + <TimeSpan>
  58 + <StartDate>2018-09-02T00:00:12Z</StartDate>
  59 + <StopDate>2025-08-12T23:59:55Z</StopDate>
  60 + </TimeSpan>
  61 + <CadenceMin>PT5S</CadenceMin>
  62 + <CadenceMax>PT30S</CadenceMax>
  63 + </TemporalDescription>
  64 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  65 + <ObservedRegion>Sun.Corona</ObservedRegion>
  66 + <Parameter>
  67 + <Name>h flux: northward</Name>
  68 + <ParameterKey>solo_het_south_hflux</ParameterKey>
  69 + <Description>Hydrogen flux</Description>
  70 + <Ucd/>
  71 + <Units>1/(s cm^2 sr MeV)</Units>
  72 + <UnitsConversion/>
  73 + <RenderingHints>
  74 + <DisplayType>Spectrogram</DisplayType>
  75 + </RenderingHints>
  76 + <Structure>
  77 + <Size>36</Size>
  78 + </Structure>
  79 + </Parameter>
  80 + <Parameter>
  81 + <Name>h flux unc: northward</Name>
  82 + <ParameterKey>solo_het_south_hunc</ParameterKey>
  83 + <Description>Uncertainty in Hydrogen flux</Description>
  84 + <Ucd/>
  85 + <Units>1/(s cm^2 sr MeV)</Units>
  86 + <UnitsConversion/>
  87 + <RenderingHints>
  88 + <DisplayType>Spectrogram</DisplayType>
  89 + </RenderingHints>
  90 + <Structure>
  91 + <Size>36</Size>
  92 + </Structure>
  93 + </Parameter>
  94 + <Parameter>
  95 + <Name>h cntrate: northward</Name>
  96 + <ParameterKey>solo_het_south_hrate</ParameterKey>
  97 + <Description>Hydrogen count rate</Description>
  98 + <Ucd/>
  99 + <Units>cnts/s</Units>
  100 + <UnitsConversion/>
  101 + <RenderingHints>
  102 + <DisplayType>Spectrogram</DisplayType>
  103 + </RenderingHints>
  104 + <Structure>
  105 + <Size>36</Size>
  106 + </Structure>
  107 + </Parameter>
  108 + <Parameter>
  109 + <Name>quality flag: northward</Name>
  110 + <ParameterKey>solo_het_south_qf</ParameterKey>
  111 + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
  112 + <Ucd/>
  113 + <Units/>
  114 + <UnitsConversion/>
  115 + <RenderingHints>
  116 + <DisplayType>TimeSeries</DisplayType>
  117 + </RenderingHints>
  118 + </Parameter>
  119 +</NumericalData>
  120 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.xml 0 → 100644
  Diff comments   View file @693caf0
... ... @@ -0,0 +1,120 @@
  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-het-sun</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>anti-sunward flow</ResourceName>
  8 + <AlternateName>Hydrogen 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, High Energy Telescope, Rates.
  11 +
  12 +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
  13 +state detectors and a BGO crystal to provide identification of particle species from the relative energy
  14 +deposited in the different detectors. Thus, HET measures count rates for different ion species, as
  15 +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
  16 +Anti-Sun, North and South)
  17 +
  18 +Parameter ID uses Detector looking directon.
  19 + </Description>
  20 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  21 + <Contact>
  22 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  23 + <Role>PrincipalInvestigator</Role>
  24 + </Contact>
  25 + <InformationURL>
  26 + <Name>SolO Archive Support Data</Name>
  27 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  28 + <Description></Description>
  29 + </InformationURL>
  30 + <Association>
  31 + <AssociationID>solo-epd-het</AssociationID>
  32 + <AssociationType>PartOf</AssociationType>
  33 + <Note>L2 : h flux</Note>
  34 + </Association>
  35 + </ResourceHeader>
  36 + <AccessInformation>
  37 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  38 + <Availability>Online</Availability>
  39 + <AccessRights>Open</AccessRights>
  40 + <AccessURL>
  41 + <Name>AMDA at CDPP</Name>
  42 + <URL>http://amda.cdpp.eu</URL>
  43 + </AccessURL>
  44 + <Format>Text</Format>
  45 + <Acknowledgement>
  46 + AMDA is a science analysis system provided by the Centre de Donnees de la
  47 + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
  48 + Universite Paul Sabatier, Toulouse
  49 + </Acknowledgement>
  50 + </AccessInformation>
  51 + <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
  52 + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
  53 + <ProviderAcknowlegment></ProviderAcknowlegment>
  54 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
  55 + <MeasurementType>EnergeticParticles</MeasurementType>
  56 + <TemporalDescription>
  57 + <TimeSpan>
  58 + <StartDate>2018-09-02T00:00:12Z</StartDate>
  59 + <StopDate>2025-08-12T23:59:55Z</StopDate>
  60 + </TimeSpan>
  61 + <CadenceMin>PT5S</CadenceMin>
  62 + <CadenceMax>PT30S</CadenceMax>
  63 + </TemporalDescription>
  64 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  65 + <ObservedRegion>Sun.Corona</ObservedRegion>
  66 + <Parameter>
  67 + <Name>h flux: anti-sunward</Name>
  68 + <ParameterKey>solo_het_sun_hflux</ParameterKey>
  69 + <Description>Hydrogen flux</Description>
  70 + <Ucd/>
  71 + <Units>1/(s cm^2 sr MeV)</Units>
  72 + <UnitsConversion/>
  73 + <RenderingHints>
  74 + <DisplayType>Spectrogram</DisplayType>
  75 + </RenderingHints>
  76 + <Structure>
  77 + <Size>36</Size>
  78 + </Structure>
  79 + </Parameter>
  80 + <Parameter>
  81 + <Name>h flux unc: anti-sunward</Name>
  82 + <ParameterKey>solo_het_sun_hunc</ParameterKey>
  83 + <Description>Uncertainty in Hydrogen flux</Description>
  84 + <Ucd/>
  85 + <Units>1/(s cm^2 sr MeV)</Units>
  86 + <UnitsConversion/>
  87 + <RenderingHints>
  88 + <DisplayType>Spectrogram</DisplayType>
  89 + </RenderingHints>
  90 + <Structure>
  91 + <Size>36</Size>
  92 + </Structure>
  93 + </Parameter>
  94 + <Parameter>
  95 + <Name>h cntrate: anti-sunward</Name>
  96 + <ParameterKey>solo_het_sun_hrate</ParameterKey>
  97 + <Description>Hydrogen count rate</Description>
  98 + <Ucd/>
  99 + <Units>cnts/s</Units>
  100 + <UnitsConversion/>
  101 + <RenderingHints>
  102 + <DisplayType>Spectrogram</DisplayType>
  103 + </RenderingHints>
  104 + <Structure>
  105 + <Size>36</Size>
  106 + </Structure>
  107 + </Parameter>
  108 + <Parameter>
  109 + <Name>quality flag: anti-sunward</Name>
  110 + <ParameterKey>solo_het_sun_qf</ParameterKey>
  111 + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
  112 + <Ucd/>
  113 + <Units/>
  114 + <UnitsConversion/>
  115 + <RenderingHints>
  116 + <DisplayType>TimeSeries</DisplayType>
  117 + </RenderingHints>
  118 + </Parameter>
  119 +</NumericalData>
  120 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-total.xml 0 → 100644
  Diff comments   View file @693caf0
... ... @@ -0,0 +1,83 @@
  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-het-total</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>total flux</ResourceName>
  8 + <AlternateName>Total Hydrogen Flux</AlternateName>
  9 + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
  10 + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates.
  11 +
  12 +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
  13 +state detectors and a BGO crystal to provide identification of particle species from the relative energy
  14 +deposited in the different detectors. Thus, HET measures count rates for different ion species, as
  15 +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
  16 +Anti-Sun, North and South)
  17 + </Description>
  18 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  19 + <Contact>
  20 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  21 + <Role>PrincipalInvestigator</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <Name>SolO Archive Support Data</Name>
  25 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  26 + <Description></Description>
  27 + </InformationURL>
  28 + <Association>
  29 + <AssociationID>solo-epd-het</AssociationID>
  30 + <AssociationType>PartOf</AssociationType>
  31 + <Note>L2 : h flux</Note>
  32 + </Association>
  33 + <PriorID>so-het-sun</PriorID>
  34 + <PriorID>so-het-anti</PriorID>
  35 + <PriorID>so-het-north</PriorID>
  36 + <PriorID>so-het-south</PriorID>
  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-EPT-SUN-RATES</ProviderResourceName>
  55 + <ProviderAcknowlegment></ProviderAcknowlegment>
  56 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</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>PT5S</CadenceMin>
  64 + <CadenceMax>PT30S</CadenceMax>
  65 + </TemporalDescription>
  66 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  67 + <ObservedRegion>Sun.Corona</ObservedRegion>
  68 + <Parameter>
  69 + <Name>h flux: total</Name>
  70 + <ParameterKey>solo_het_total_hflux</ParameterKey>
  71 + <Description>Hydrogen flux</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>36</Size>
  80 + </Structure>
  81 + </Parameter>
  82 +</NumericalData>
  83 +</Spase>
... ...