Commit 6b75e44b46a71eeb644c53fdcf72402ab02cf0d4

Authored by Elena.Budnik
1 parent 8ffcba07

SolO EPD STEP

Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP.xml 0 → 100644
... ... @@ -0,0 +1,39 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>EPD/STEP</ResourceName>
  8 + <AlternateName>Energetic Particle Detector / SupraThermal Electrons and Protons</AlternateName>
  9 + <ReleaseDate>2018-10-27T18:45:12Z</ReleaseDate>
  10 + <Description>The Energetic Particle Detector (EPD) is an instrument suite comprising different sensors that have been designed
  11 + to measure the spectra, composition, time variations, and directional distributions ofenergetic particles.
  12 + These measurements will be performed over a partly overlapping energy range encompassing a few keV to
  13 + 450 MeV/n, with sufficient time, energy, angular, and mass resolution to achieve the mission science goals.
  14 + The EPD consists of the following units :
  15 + * SupraThermal Electrons and Protons (STEP).
  16 +
  17 + Designed to measure protons and electrons
  18 + at supra-thermal energies (between 2 and 80 keV). It employs two co-aligned sensor heads with a parallel field of view.
  19 + One of the sensor heads contains a permanent magnet that deflects electrons out of the nominal field of view, this is referred
  20 + to as magnet channel and measures all types of particles except electrons.
  21 + The other head measures every particle in the energy range including electrons and is called integral channel.
  22 + Each head contains a solid state detector divided in several pixels to achieve angular resolution. For each channel there are
  23 + 15 pixels distributed in 3 rows and 5 columns, plus a separate pixel for measuring background.
  24 + </Description>
  25 + <Acknowledgement></Acknowledgement>
  26 + <Contact>
  27 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  28 + <Role>PrincipalInvestigator</Role>
  29 + </Contact>
  30 + <InformationURL>
  31 + <Name>Instrument Description</Name>
  32 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data?preview=/60885589/60886052/SO-EPD-PO-TN-0038_iss1_rev1_DPDD.pdf</URL>
  33 + </InformationURL>
  34 + </ResourceHeader>
  35 + <InstrumentType>SolidStateDetector</InstrumentType>
  36 + <InvestigationName>EPD</InvestigationName>
  37 + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/SolO</ObservatoryID>
  38 + </Instrument>
  39 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rates.xml 0 → 100644
... ... @@ -0,0 +1,178 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_3_0.xsd">
  3 + <Version>2.3.0</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rates</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>flux</ResourceName>
  8 + <AlternateName>Flux averaged over sectors</AlternateName>
  9 + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
  10 + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates.
  11 +
  12 + STEP is designed to measure electrons and ions in the suprathermal energy range (280 keV). To
  13 + allow for the separation of electrons and ions, STEP has 2 different channels, each equipped with its
  14 + own solid state detectors for detecting particles:
  15 + * Magnet channel. Uses a permanent magnet to deflect electrons, measuring only ions (mostly protons).
  16 + * Integral channel. Measures all incoming particles.
  17 +
  18 + The electron flux is recovered by subtracting the magnet channel measurements from the integral
  19 + channel ones. Each channel is divided in 15 sectors, disposed in 3 rows of 5 pixels, providing
  20 + directional information of the incoming particles within the field of view. An additional pixel, not directly
  21 + exposed to the incoming flux, measures the cosmic ray background.</Description>
  22 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  23 + <Contact>
  24 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  25 + <Role>PrincipalInvestigator</Role>
  26 + </Contact>
  27 + <InformationURL>
  28 + <Name>SolO Archive Support Data</Name>
  29 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  30 + <Description></Description>
  31 + </InformationURL>
  32 + <Association>
  33 + <AssociationID>solo-epd-step</AssociationID>
  34 + <AssociationType>PartOf</AssociationType>
  35 + <Note>L2 : rates</Note>
  36 + </Association>
  37 + </ResourceHeader>
  38 + <AccessInformation>
  39 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  40 + <Availability>Online</Availability>
  41 + <AccessRights>Open</AccessRights>
  42 + <AccessURL>
  43 + <Name>AMDA at CDPP</Name>
  44 + <URL>http://amda.cdpp.eu</URL>
  45 + </AccessURL>
  46 + <Format>Text</Format>
  47 + <Acknowledgement>
  48 + AMDA is a science analysis system provided by the Centre de Donnees de la
  49 + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
  50 + Universite Paul Sabatier, Toulouse
  51 + </Acknowledgement>
  52 + </AccessInformation>
  53 + <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
  54 + <ProviderResourceName>EPD-STEP-RATES</ProviderResourceName>
  55 + <ProviderAcknowlegment></ProviderAcknowlegment>
  56 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</InstrumentID>
  57 + <MeasurementType>EnergeticParticles</MeasurementType>
  58 + <TemporalDescription>
  59 + <TimeSpan>
  60 + <StartDate>2018-09-02T00:00:12Z</StartDate>
  61 + <StopDate>2025-08-12T23:59:55Z</StopDate>
  62 + </TimeSpan>
  63 + <CadenceMin>PT10S</CadenceMin>
  64 + <CadenceMax>PT60S</CadenceMax>
  65 + </TemporalDescription>
  66 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  67 + <ObservedRegion>Sun.Corona</ObservedRegion>
  68 + <Parameter>
  69 + <Name>ion flux</Name>
  70 + <ParameterKey>solo_step_mflux</ParameterKey>
  71 + <Description>Magnet channel. Uses a permanet magnet to deflect electrons. Measuring only ions (mostly protons)</Description>
  72 + <Ucd/>
  73 + <Units>1/(s cm^2 sr MeV)</Units>
  74 + <UnitsConversion/>
  75 + <RenderingHints>
  76 + <DisplayType>Spectrogram</DisplayType>
  77 + </RenderingHints>
  78 + <Structure>
  79 + <Size>48</Size>
  80 + </Structure>
  81 + </Parameter>
  82 + <Parameter>
  83 + <Name>ion flux unc</Name>
  84 + <ParameterKey>solo_step_munc</ParameterKey>
  85 + <Description>Uncertainty in sector averaged magnet channel flux</Description>
  86 + <Ucd/>
  87 + <Units>1/(s cm^2 sr MeV)</Units>
  88 + <UnitsConversion/>
  89 + <RenderingHints>
  90 + <DisplayType>Spectrogram</DisplayType>
  91 + </RenderingHints>
  92 + <Structure>
  93 + <Size>48</Size>
  94 + </Structure>
  95 + </Parameter>
  96 + <Parameter>
  97 + <Name>ion cntrate</Name>
  98 + <ParameterKey>solo_step_mrate</ParameterKey>
  99 + <Description>Sector averaged magnet channel count rate</Description>
  100 + <Ucd/>
  101 + <Units>cnts/s</Units>
  102 + <UnitsConversion/>
  103 + <RenderingHints>
  104 + <DisplayType>Spectrogram</DisplayType>
  105 + </RenderingHints>
  106 + <Structure>
  107 + <Size>48</Size>
  108 + </Structure>
  109 + </Parameter>
  110 + <Parameter>
  111 + <Name>el flux</Name>
  112 + <ParameterKey>solo_step_eflux</ParameterKey>
  113 + <Description>The electron flux is recovered by subtracting the magnet channel measurements from the integral channel ones</Description>
  114 + <Ucd/>
  115 + <Units>1/(s cm^2 sr MeV)</Units>
  116 + <UnitsConversion/>
  117 + <RenderingHints>
  118 + <DisplayType>Spectrogram</DisplayType>
  119 + </RenderingHints>
  120 + <Structure>
  121 + <Size>48</Size>
  122 + </Structure>
  123 + </Parameter>
  124 + <Parameter>
  125 + <Name>total flux</Name>
  126 + <ParameterKey>solo_step_iflux</ParameterKey>
  127 + <Description>Integral channel. Measures all incoming particles</Description>
  128 + <Ucd/>
  129 + <Units>1/(s cm^2 sr MeV)</Units>
  130 + <UnitsConversion/>
  131 + <RenderingHints>
  132 + <DisplayType>Spectrogram</DisplayType>
  133 + </RenderingHints>
  134 + <Structure>
  135 + <Size>48</Size>
  136 + </Structure>
  137 + </Parameter>
  138 + <Parameter>
  139 + <Name>total flux unc</Name>
  140 + <ParameterKey>solo_step_iunc</ParameterKey>
  141 + <Description>Uncertainty in sector averaged integral channel flux</Description>
  142 + <Ucd/>
  143 + <Units>1/(s cm^2 sr MeV)</Units>
  144 + <UnitsConversion/>
  145 + <RenderingHints>
  146 + <DisplayType>Spectrogram</DisplayType>
  147 + </RenderingHints>
  148 + <Structure>
  149 + <Size>48</Size>
  150 + </Structure>
  151 + </Parameter>
  152 + <Parameter>
  153 + <Name>total cntrate</Name>
  154 + <ParameterKey>solo_step_irate</ParameterKey>
  155 + <Description>Sector averaged integral channel count rate</Description>
  156 + <Ucd/>
  157 + <Units>cnts/s</Units>
  158 + <UnitsConversion/>
  159 + <RenderingHints>
  160 + <DisplayType>Spectrogram</DisplayType>
  161 + </RenderingHints>
  162 + <Structure>
  163 + <Size>48</Size>
  164 + </Structure>
  165 + </Parameter>
  166 + <Parameter>
  167 + <Name>quality flag</Name>
  168 + <ParameterKey>solo_step_qf</ParameterKey>
  169 + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
  170 + <Ucd/>
  171 + <Units/>
  172 + <UnitsConversion/>
  173 + <RenderingHints>
  174 + <DisplayType>TimeSeries</DisplayType>
  175 + </RenderingHints>
  176 + </Parameter>
  177 +</NumericalData>
  178 +</Spase>
... ...
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rtn.xml 0 → 100644
... ... @@ -0,0 +1,89 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_3_0.xsd">
  3 + <Version>2.3.0</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rtn</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>flux direction RTN</ResourceName>
  8 + <AlternateName></AlternateName>
  9 + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
  10 + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates.</Description>
  11 + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
  12 + <Contact>
  13 + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
  14 + <Role>PrincipalInvestigator</Role>
  15 + </Contact>
  16 + <InformationURL>
  17 + <Name>SolO Archive Support Data</Name>
  18 + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
  19 + <Description></Description>
  20 + </InformationURL>
  21 + <Association>
  22 + <AssociationID>solo-epd-step</AssociationID>
  23 + <AssociationType>PartOf</AssociationType>
  24 + <Note>L2 : rates</Note>
  25 + </Association>
  26 + </ResourceHeader>
  27 + <AccessInformation>
  28 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  29 + <Availability>Online</Availability>
  30 + <AccessRights>Open</AccessRights>
  31 + <AccessURL>
  32 + <Name>AMDA at CDPP</Name>
  33 + <URL>http://amda.cdpp.eu</URL>
  34 + </AccessURL>
  35 + <Format>Text</Format>
  36 + <Acknowledgement>
  37 + AMDA is a science analysis system provided by the Centre de Donnees de la
  38 + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
  39 + Universite Paul Sabatier, Toulouse
  40 + </Acknowledgement>
  41 + </AccessInformation>
  42 + <ProviderName>http://soar.esac.esa.int/soar</ProviderName>
  43 + <ProviderResourceName>EPD-STEP-RATES</ProviderResourceName>
  44 + <ProviderAcknowlegment></ProviderAcknowlegment>
  45 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP</InstrumentID>
  46 + <MeasurementType>EnergeticParticles</MeasurementType>
  47 + <TemporalDescription>
  48 + <TimeSpan>
  49 + <StartDate>2018-09-02T00:00:12Z</StartDate>
  50 + <StopDate>2025-08-12T23:59:55Z</StopDate>
  51 + </TimeSpan>
  52 + <Cadence>PT60S</Cadence>
  53 + </TemporalDescription>
  54 + <ObservedRegion>Heliosphere.Inner</ObservedRegion>
  55 + <ObservedRegion>Sun.Corona</ObservedRegion>
  56 + <Parameter>
  57 + <Name>flux direction</Name>
  58 + <ParameterKey>solo_step_dir_rtn</ParameterKey>
  59 + <Description>Particle flow direction (unit vector) in RTN coordinates</Description>
  60 + <Ucd/>
  61 + <Units/>
  62 + <UnitsConversion/>
  63 + <RenderingHints>
  64 + <DisplayType>TimeSeries</DisplayType>
  65 + </RenderingHints>
  66 + <Structure>
  67 + <Size>3</Size>
  68 + <Element>
  69 + <Name>r</Name>
  70 + <Qualifier>Component.I</Qualifier>
  71 + <Index>1</Index>
  72 + <ParameterKey>solo_step_dir_rtn(0)</ParameterKey>
  73 + </Element>
  74 + <Element>
  75 + <Name>t</Name>
  76 + <Qualifier>Component.J</Qualifier>
  77 + <Index>2</Index>
  78 + <ParameterKey>solo_step_dir_rtn(1)</ParameterKey>
  79 + </Element>
  80 + <Element>
  81 + <Name>n</Name>
  82 + <Qualifier>Component.K</Qualifier>
  83 + <Index>3</Index>
  84 + <ParameterKey>solo_step_dir_rtn(2)</ParameterKey>
  85 + </Element>
  86 + </Structure>
  87 + </Parameter>
  88 +</NumericalData>
  89 +</Spase>
... ...