Commit afd3415f8283cf9a060bec33a550f6466b922876

Authored by Benjamin Renard
1 parent 76d0caca

Merge SOHO/ERNE & SOHO/EPHIN from amdadev

Instrument/CDPP-AMDA/SOHO/COSTEP.xml 0 → 100644
... ... @@ -0,0 +1,25 @@
  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://www.spase-group.org/data/schema/spase-2_0_0.xsd">
  3 + <Version>2.0.0</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/SOHO/COSTEP</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>COSTEP</ResourceName>
  8 + <AlternateName>Comprehensive Suprathermal and Energetic Particle Instrument (COSTEP)</AlternateName>
  9 + <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
  10 + <Description>The COSTEP (COmprehensive SupraThermal and Energetic Particle) instrument with sensors LION and EPHIN is a subset of the CEPAC experiment measuring the solar particle emission over a wide range of species (electrons through iron) and energies (40 KeV/particle to 500 MeV/nucleon). LION (Low-energy Ion and electron instrument) has two sensor heads, each containing a double telescope and measuring spectra of ions and electrons in the range 40 KeV to 5 MeV for protons, 1.5--6 MeV/nucleon for Helium nuclei, and 40--300 KeV for electrons. The LION detector system consists of three ion implanted silicon detectors. One sensor head employs a broom magnet to sweep electrons of energies &lt;300 KeV away from the detectors. The total field of view is 60 x 40 degrees. A total of 32 energy channels are accumulated with 15 s resolution. From these it is possible to derive good spectra during large solar events with about one minute resolution. The EPHIN sensor is a multi-element array of solid state detectors with anticoincidence to measure energy spectra of electrons in the range 150 KeV to &gt;5MeV and hydrogen and helium isotopes in the range 4 MeV/nucleon to &gt;53 MeV/nucleon with a maximum geometric factor of 5.1 cm**3 sr (self-adapting to particle fluxes). The field of view is a cone of 90 degrees full angle. The separation of particle species is provided by a set of five thresholds in the first detector. A small sample of particles is analyzed in pulse height. Four 128-bin histograms containing coarse spectral information are generated on-board separately for four detector ranges and transmitted each minute together with rates and pulse height words. The COSTEP data will be routinely searched for irregular 3He contributions in the EPHIN pulse height words, especially during special campaigns or if other information is available predicting higher contributions. If 3He is observed, the correlation with electron observations of various energies will be investigated to compare acceleration, release, and travel times as well as spectral features. This information is from the paper ``COSTEP - Comprehensive Suprathermal and Energetic Particle Analyser for SOHO - Scientific Goals and Data Description,'' by H. Kunow et al. (Proceedings of the First SOHO Workshop, ESA SP-348, pp. 43-46, November 1992).</Description>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Horst.W.Kunow</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 +</Contact>
  15 + <InformationURL>
  16 + <Name>NSSDC's Master Catalog</Name>
  17 + <URL>https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1995-065A&amp;ex=8</URL>
  18 + <Description>Information about the Comprehensive Suprathermal and Energetic Particle Instrument (COSTEP) experiment on the SOHO mission.</Description>
  19 +</InformationURL>
  20 +</ResourceHeader>
  21 + <InstrumentType>EnergeticParticleInstrument</InstrumentType>
  22 + <InvestigationName>Comprehensive Suprathermal and Energetic Particle Instrument (COSTEP) on SOHO</InvestigationName>
  23 + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/SOHO</ObservatoryID>
  24 +</Instrument>
  25 +</Spase>
... ...
Instrument/CDPP-AMDA/SOHO/ERNE.xml 0 → 100644
... ... @@ -0,0 +1,27 @@
  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://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/SOHO/ERNE</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>ERNE</ResourceName>
  8 + <AlternateName>Energetic and Relativistic Nuclei and Electrons</AlternateName>
  9 + <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
  10 + <Description>The Energetic and Relativistic Nuclei and Electrons (ERNE) experiment will investigate the solar atmosphere by detecting particles produced in various kinds of energy release processes. Measurements will cover the particle flux at quiet times, solar particle events, flux enhancement due to particle acceleration by interplanetary shocks, and solar modulation of galactic cosmic rays. The instrument will measure the energy spectra of elements in the range Z = 1--30, and will also measure the abundance ratios of isotopes as well as the anisotropy of the particle flux. Isotopic resolution varies with particle type and energy; for carbon in the 20--140 MeV/nucleon range the resolution is 0.25 amu. The instrument uses two separate particle telescopes, LED and HED, where a particle penetrates through active layers and the energy deposited in each layer is measured. By comparing to a theoretical energy loss, the particle type and energy can be determined. The LED (Low Energy Detector) consists of an outer circular solid state detector, covered by a thin (1 mg/cm**2) kapton foil, an inner detector, and an anticoincidence detector. The HED (High Energy Detector) uses silicon detectors and scintillation detectors read by photo diodes. The outer two detectors are mutually orthogonal, single-sided strip detectors each, thus forming a pair of two-dimensional position-sensitive detectors. Following these are additional silicon detectors and CsI(Tl) and BGO scintillators. The LED has a field of view (FOV) of 64 degrees and identifies isotopes from H to Ne. Its energy range is 1.4--12 MeV/nucleon for protons and helium, 2.1--46 MeV/nucleon for other nuclei. HED has a 120 degree FOV and its energy range is 12--110 MeV/nucleon for protons and helium, 25--540 MeV/nucleon for other nuclei, and 5--60 MeV for electrons. This information is from the paper ``Energetic Particle Analyser ERNE,'' by J. Torsti et al. (Proceedings of the First SOHO Workshop, ESA SP-348, p. 47-50, November 1992).
  11 +</Description>
  12 + <Contact>
  13 + <PersonID>spase://SMWG/Person/Jarmo.Torsti</PersonID>
  14 + <Role>PrincipalInvestigator</Role>
  15 + </Contact>
  16 + <InformationURL>
  17 + <Name>NSSDC's Master Catalog</Name>
  18 + <URL>https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1995-065A&amp;ex=9</URL>
  19 + <Description>Information about the Energetic and Relativistic Nuclei and Electrons (ERNE) experiment on the SOHO mission.
  20 +</Description>
  21 + </InformationURL>
  22 + </ResourceHeader>
  23 + <InstrumentType>EnergeticParticleInstrument</InstrumentType>
  24 + <InvestigationName>Energetic and Relativistic Nuclei and Electrons (ERNE) on SOHO</InvestigationName>
  25 + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/SOHO</ObservatoryID>
  26 + </Instrument>
  27 +</Spase>
... ...
NumericalData/CDPP-AMDA/SOHO/COSTEP/soho-ephin-10min.xml 0 → 100644
... ... @@ -0,0 +1,109 @@
  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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/SOHO/COSTEP/soho-ephin-10min</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>10 min</ResourceName>
  8 + <ReleaseDate>2022-01-17T00:00:00Z</ReleaseDate>
  9 + <Description>10 minutes Level3 intensity data of protons at four energies between 4.3 and 53 Mev,
  10 +and of alpha particles at four energies between 4.3 and 53 MeV/n.</Description>
  11 + <Contact>
  12 + <PersonID>spase://CNES/Person/Patrick.Kuhl</PersonID>
  13 + <Role>DataProducer</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/Bernd.Heber</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <InformationURL>
  20 + <Name>SOHO/EPHIN Level3 data product</Name>
  21 + <URL>http://ulysses.physik.uni-kiel.de/costep/level3/l3i/</URL>
  22 + </InformationURL>
  23 + <Association>
  24 + <AssociationID>soho-costep-ephin</AssociationID>
  25 + <AssociationType>PartOf</AssociationType>
  26 + <Note>EPHIN</Note>
  27 + </Association>
  28 + </ResourceHeader>
  29 + <AccessInformation>
  30 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  31 + <Availability>Online</Availability>
  32 + <AccessRights>Open</AccessRights>
  33 + <AccessURL>
  34 + <URL>http://amda.cdpp.eu</URL>
  35 + </AccessURL>
  36 + <Format>NetCDF</Format>
  37 + </AccessInformation>
  38 + <ProcessingLevel>ValueAdded</ProcessingLevel>
  39 + <ProviderName>http://ulysses.physik.uni-kiel.de/costep/level3/l3i/</ProviderName>
  40 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/SOHO/COSTEP</InstrumentID>
  41 + <MeasurementType>EnergeticParticles</MeasurementType>
  42 + <Parameter>
  43 + <Name>proton flux</Name>
  44 + <ParameterKey>soho_ephin_10minp</ParameterKey>
  45 + <Units>1/(cm**2 s sr MeV)</Units>
  46 + <Structure>
  47 + <Size>4</Size>
  48 + <Element>
  49 + <Name>4.3 - 7.8 MeV</Name>
  50 + <Index>1</Index>
  51 + <ParameterKey>soho_ephin_10minp(0)</ParameterKey>
  52 + </Element>
  53 + <Element>
  54 + <Name>7.8 - 25 MeV</Name>
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  56 + <ParameterKey>soho_ephin_10minp(1)</ParameterKey>
  57 + </Element>
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  59 + <Name>25 - 40.9 MeV</Name>
  60 + <Index>3</Index>
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  62 + </Element>
  63 + <Element>
  64 + <Name>40.9 - 53 MeV</Name>
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  66 + <ParameterKey>soho_ephin_10minp(3)</ParameterKey>
  67 + </Element>
  68 + </Structure>
  69 + <FillValue>-1</FillValue>
  70 + <Particle>
  71 + <ParticleType>Proton</ParticleType>
  72 + <ParticleQuantity>NumberFlux</ParticleQuantity>
  73 + </Particle>
  74 + </Parameter>
  75 + <Parameter>
  76 + <Name>He flux</Name>
  77 + <ParameterKey>soho_ephin_10minhe</ParameterKey>
  78 + <Units>1/(cm**2 s sr MeV/n)</Units>
  79 + <Structure>
  80 + <Size>4</Size>
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  96 + <Element>
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  99 + <ParameterKey>soho_ephin_10minhe(3)</ParameterKey>
  100 + </Element>
  101 + </Structure>
  102 + <FillValue>-1</FillValue>
  103 + <Particle>
  104 + <ParticleType>AlphaParticle</ParticleType>
  105 + <ParticleQuantity>NumberFlux</ParticleQuantity>
  106 + </Particle>
  107 + </Parameter>
  108 + </NumericalData>
  109 +</Spase>
... ...
NumericalData/CDPP-AMDA/SOHO/COSTEP/soho-ephin-1min.xml 0 → 100644
... ... @@ -0,0 +1,109 @@
  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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/SOHO/COSTEP/soho-ephin-1min</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>1 min</ResourceName>
  8 + <ReleaseDate>2022-01-17T00:00:00Z</ReleaseDate>
  9 + <Description>1 minute Level3 intensity data of protons at four energies between 4.3 and 53 Mev,
  10 +and of alpha particles at four energies between 4.3 and 53 MeV/n.</Description>
  11 + <Contact>
  12 + <PersonID>spase://CNES/Person/Patrick.Kuhl</PersonID>
  13 + <Role>DataProducer</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/Bernd.Heber</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <InformationURL>
  20 + <Name>SOHO/EPHIN Level3 data product</Name>
  21 + <URL>http://ulysses.physik.uni-kiel.de/costep/level3/l3i/</URL>
  22 + </InformationURL>
  23 + <Association>
  24 + <AssociationID>soho-costep-ephin</AssociationID>
  25 + <AssociationType>PartOf</AssociationType>
  26 + <Note>EPHIN</Note>
  27 + </Association>
  28 + </ResourceHeader>
  29 + <AccessInformation>
  30 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  31 + <Availability>Online</Availability>
  32 + <AccessRights>Open</AccessRights>
  33 + <AccessURL>
  34 + <URL>http://amda.cdpp.eu</URL>
  35 + </AccessURL>
  36 + <Format>NetCDF</Format>
  37 + </AccessInformation>
  38 + <ProcessingLevel>ValueAdded</ProcessingLevel>
  39 + <ProviderName>http://ulysses.physik.uni-kiel.de/costep/level3/l3i/</ProviderName>
  40 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/SOHO/COSTEP</InstrumentID>
  41 + <MeasurementType>EnergeticParticles</MeasurementType>
  42 + <Parameter>
  43 + <Name>proton flux</Name>
  44 + <ParameterKey>soho_ephin_1minp</ParameterKey>
  45 + <Units>1/(cm**2 s sr MeV)</Units>
  46 + <Structure>
  47 + <Size>4</Size>
  48 + <Element>
  49 + <Name>4.3 - 7.8 MeV</Name>
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  51 + <ParameterKey>soho_ephin_1minp(0)</ParameterKey>
  52 + </Element>
  53 + <Element>
  54 + <Name>7.8 - 25 MeV</Name>
  55 + <Index>2</Index>
  56 + <ParameterKey>soho_ephin_1minp(1)</ParameterKey>
  57 + </Element>
  58 + <Element>
  59 + <Name>25 - 40.9 MeV</Name>
  60 + <Index>3</Index>
  61 + <ParameterKey>soho_ephin_1minp(2)</ParameterKey>
  62 + </Element>
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  69 + <FillValue>-1</FillValue>
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  71 + <ParticleType>Proton</ParticleType>
  72 + <ParticleQuantity>NumberFlux</ParticleQuantity>
  73 + </Particle>
  74 + </Parameter>
  75 + <Parameter>
  76 + <Name>He flux</Name>
  77 + <ParameterKey>soho_ephin_1minhe</ParameterKey>
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  102 + <FillValue>-1</FillValue>
  103 + <Particle>
  104 + <ParticleType>AlphaParticle</ParticleType>
  105 + <ParticleQuantity>NumberFlux</ParticleQuantity>
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  107 + </Parameter>
  108 + </NumericalData>
  109 +</Spase>
... ...
NumericalData/CDPP-AMDA/SOHO/COSTEP/soho-ephin-60min.xml 0 → 100644
... ... @@ -0,0 +1,109 @@
  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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/SOHO/COSTEP/soho-ephin-60min</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>1 hour</ResourceName>
  8 + <ReleaseDate>2022-01-17T00:00:00Z</ReleaseDate>
  9 + <Description>1 hour Level3 intensity data of protons at four energies between 4.3 and 53 Mev,
  10 +and of alpha particles at four energies between 4.3 and 53 MeV/n.</Description>
  11 + <Contact>
  12 + <PersonID>spase://CNES/Person/Patrick.Kuhl</PersonID>
  13 + <Role>DataProducer</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/Bernd.Heber</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <InformationURL>
  20 + <Name>SOHO/EPHIN Level3 data product</Name>
  21 + <URL>http://ulysses.physik.uni-kiel.de/costep/level3/l3i/</URL>
  22 + </InformationURL>
  23 + <Association>
  24 + <AssociationID>soho-costep-ephin</AssociationID>
  25 + <AssociationType>PartOf</AssociationType>
  26 + <Note>EPHIN</Note>
  27 + </Association>
  28 + </ResourceHeader>
  29 + <AccessInformation>
  30 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  31 + <Availability>Online</Availability>
  32 + <AccessRights>Open</AccessRights>
  33 + <AccessURL>
  34 + <URL>http://amda.cdpp.eu</URL>
  35 + </AccessURL>
  36 + <Format>NetCDF</Format>
  37 + </AccessInformation>
  38 + <ProcessingLevel>ValueAdded</ProcessingLevel>
  39 + <ProviderName>http://ulysses.physik.uni-kiel.de/costep/level3/l3i/</ProviderName>
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  41 + <MeasurementType>EnergeticParticles</MeasurementType>
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  43 + <Name>proton flux</Name>
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... ...
NumericalData/CDPP-AMDA/SOHO/ERNE/soho-erne-hed.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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
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  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/SOHO/ERNE/soho-erne-hed</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>HED</ResourceName>
  8 + <AlternateName>HED detector</AlternateName>
  9 + <AlternateName>High Energy Detector</AlternateName>
  10 + <ReleaseDate>2021-11-09T00:00:00Z</ReleaseDate>
  11 + <Description>High Energy Detector consist of 7 detector layers and an anticoincidence
  12 +(AC) shield. First 4 layers are position sensitive silicon strip detectors
  13 +(S1x, S1y, S2x, S2y), they are followed by an other silicon detector (D1),
  14 +a CsI scintillator (D2) and a BGO-scintillator (D3).</Description>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/Rami.Vainio</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/Esa.Riihonen</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <Name>SOHO/ERNE Export data archive</Name>
  25 + <URL>https://srl.utu.fi/export/</URL>
  26 + </InformationURL>
  27 + </ResourceHeader>
  28 + <AccessInformation>
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  30 + <Availability>Online</Availability>
  31 + <AccessRights>Open</AccessRights>
  32 + <AccessURL>
  33 + <URL>http://amda.cdpp.eu</URL>
  34 + </AccessURL>
  35 + <Format>NetCDF</Format>
  36 + </AccessInformation>
  37 + <ProcessingLevel>Calibrated</ProcessingLevel>
  38 + <ProviderName>https://srl.utu.fi/export/</ProviderName>
  39 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/SOHO/ERNE</InstrumentID>
  40 + <MeasurementType>EnergeticParticles</MeasurementType>
  41 + <Parameter>
  42 + <Name>proton flux</Name>
  43 + <ParameterKey>soho_erne_hedp</ParameterKey>
  44 + <Units>1/(cm**2 sr s MeV)</Units>
  45 + <Structure>
  46 + <Size>10</Size>
  47 + <Element>
  48 + <Name>13 - 16 MeV</Name>
  49 + <Index>1</Index>
  50 + <ParameterKey>soho_erne_hedp(0)</ParameterKey>
  51 + </Element>
  52 + <Element>
  53 + <Name>16 - 20 MeV</Name>
  54 + <Index>2</Index>
  55 + <ParameterKey>soho_erne_hedp(1)</ParameterKey>
  56 + </Element>
  57 + <Element>
  58 + <Name>20 - 25 MeV</Name>
  59 + <Index>3</Index>
  60 + <ParameterKey>soho_erne_hedp(2)</ParameterKey>
  61 + </Element>
  62 + <Element>
  63 + <Name>25 - 32 MeV</Name>
  64 + <Index>4</Index>
  65 + <ParameterKey>soho_erne_hedp(3)</ParameterKey>
  66 + </Element>
  67 + <Element>
  68 + <Name>32 - 40 MeV</Name>
  69 + <Index>5</Index>
  70 + <ParameterKey>soho_erne_hedp(4)</ParameterKey>
  71 + </Element>
  72 + <Element>
  73 + <Name>40 - 50 MeV</Name>
  74 + <Index>6</Index>
  75 + <ParameterKey>soho_erne_hedp(5)</ParameterKey>
  76 + </Element>
  77 + <Element>
  78 + <Name>50 - 64 MeV</Name>
  79 + <Index>7</Index>
  80 + <ParameterKey>soho_erne_hedp(6)</ParameterKey>
  81 + </Element>
  82 + <Element>
  83 + <Name>64 - 80 MeV</Name>
  84 + <Index>8</Index>
  85 + <ParameterKey>soho_erne_hedp(7)</ParameterKey>
  86 + </Element>
  87 + <Element>
  88 + <Name>80 - 100 MeV</Name>
  89 + <Index>9</Index>
  90 + <ParameterKey>soho_erne_hedp(8)</ParameterKey>
  91 + </Element>
  92 + <Element>
  93 + <Name>100 - 130 MeV</Name>
  94 + <Index>10</Index>
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  96 + </Element>
  97 + </Structure>
  98 + <FillValue>-1</FillValue>
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  100 + <ParticleType>Proton</ParticleType>
  101 + <ParticleQuantity>NumberFlux</ParticleQuantity>
  102 + </Particle>
  103 + </Parameter>
  104 + <Parameter>
  105 + <Name>4He flux</Name>
  106 + <ParameterKey>soho_erne_heda</ParameterKey>
  107 + <Units>1/(cm**2 sr s MeV/n)</Units>
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  119 + </Element>
  120 + <Element>
  121 + <Name>20 - 25 MeV/n</Name>
  122 + <Index>3</Index>
  123 + <ParameterKey>soho_erne_heda(2)</ParameterKey>
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  125 + <Element>
  126 + <Name>25 - 32 MeV/n</Name>
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  129 + </Element>
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  131 + <Name>32 - 40 MeV/n</Name>
  132 + <Index>5</Index>
  133 + <ParameterKey>soho_erne_heda(4)</ParameterKey>
  134 + </Element>
  135 + <Element>
  136 + <Name>40 - 50 MeV/n</Name>
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  138 + <ParameterKey>soho_erne_heda(5)</ParameterKey>
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  141 + <Name>50 - 64 MeV/n</Name>
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  144 + </Element>
  145 + <Element>
  146 + <Name>64 - 80 MeV/n</Name>
  147 + <Index>8</Index>
  148 + <ParameterKey>soho_erne_heda(7)</ParameterKey>
  149 + </Element>
  150 + <Element>
  151 + <Name>80 - 100 MeV/n</Name>
  152 + <Index>9</Index>
  153 + <ParameterKey>soho_erne_heda(8)</ParameterKey>
  154 + </Element>
  155 + <Element>
  156 + <Name>100 - 130 MeV/n</Name>
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  158 + <ParameterKey>soho_erne_heda(9)</ParameterKey>
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  163 + <ParticleType>AlphaParticle</ParticleType>
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  165 + </Particle>
  166 + </Parameter>
  167 + </NumericalData>
  168 +</Spase>
... ...
NumericalData/CDPP-AMDA/SOHO/ERNE/soho-erne-led.xml 0 → 100644
... ... @@ -0,0 +1,167 @@
  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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/SOHO/ERNE/soho-erne-led</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>LED</ResourceName>
  8 + <AlternateName>LED detector</AlternateName>
  9 + <AlternateName>Low Energy Detector</AlternateName>
  10 + <ReleaseDate>2021-11-09T00:00:00Z</ReleaseDate>
  11 + <Description>Low Energy Detector is a two-layer semiconductor (silicon) detector, with
  12 +an anticoincidence (AC) shield at the bottom. The upper layer consist of 7
  13 +segments (D11-D17). The common lower layer is called D2.</Description>
  14 + <Contact>
  15 + <PersonID>spase://CNES/Person/Rami.Vainio</PersonID>
  16 + <Role>DataProducer</Role>
  17 + </Contact>
  18 + <Contact>
  19 + <PersonID>spase://CNES/Person/Esa.Riihonen</PersonID>
  20 + <Role>DataProducer</Role>
  21 + </Contact>
  22 + <InformationURL>
  23 + <Name>SOHO/ERNE Export data archive</Name>
  24 + <URL>https://srl.utu.fi/export/</URL>
  25 + </InformationURL>
  26 + </ResourceHeader>
  27 + <AccessInformation>
  28 + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
  29 + <Availability>Online</Availability>
  30 + <AccessRights>Open</AccessRights>
  31 + <AccessURL>
  32 + <URL>http://amda.cdpp.eu</URL>
  33 + </AccessURL>
  34 + <Format>NetCDF</Format>
  35 + </AccessInformation>
  36 + <ProcessingLevel>Calibrated</ProcessingLevel>
  37 + <ProviderName>https://srl.utu.fi/export/</ProviderName>
  38 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/SOHO/ERNE</InstrumentID>
  39 + <MeasurementType>EnergeticParticles</MeasurementType>
  40 + <Parameter>
  41 + <Name>proton flux</Name>
  42 + <ParameterKey>soho_erne_ledp</ParameterKey>
  43 + <Units>1/(cm**2 sr s MeV)</Units>
  44 + <Structure>
  45 + <Size>10</Size>
  46 + <Element>
  47 + <Name>1.3 - 1.6 MeV</Name>
  48 + <Index>1</Index>
  49 + <ParameterKey>soho_erne_ledp(0)</ParameterKey>
  50 + </Element>
  51 + <Element>
  52 + <Name>1.6 - 2.0 MeV</Name>
  53 + <Index>2</Index>
  54 + <ParameterKey>soho_erne_ledp(1)</ParameterKey>
  55 + </Element>
  56 + <Element>
  57 + <Name>2.0 - 2.5 MeV</Name>
  58 + <Index>3</Index>
  59 + <ParameterKey>soho_erne_ledp(2)</ParameterKey>
  60 + </Element>
  61 + <Element>
  62 + <Name>2.5 - 3.2 MeV</Name>
  63 + <Index>4</Index>
  64 + <ParameterKey>soho_erne_ledp(3)</ParameterKey>
  65 + </Element>
  66 + <Element>
  67 + <Name>3.2 - 4.0 MeV</Name>
  68 + <Index>5</Index>
  69 + <ParameterKey>soho_erne_ledp(4)</ParameterKey>
  70 + </Element>
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  72 + <Name>4.0 - 5.0 MeV</Name>
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  74 + <ParameterKey>soho_erne_ledp(5)</ParameterKey>
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  78 + <Index>7</Index>
  79 + <ParameterKey>soho_erne_ledp(6)</ParameterKey>
  80 + </Element>
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  82 + <Name>6.4 - 8.0 MeV</Name>
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  102 + </Parameter>
  103 + <Parameter>
  104 + <Name>4He flux</Name>
  105 + <ParameterKey>soho_erne_leda</ParameterKey>
  106 + <Units>1/(cm**2 sr s MeV/n)</Units>
  107 + <Structure>
  108 + <Size>10</Size>
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  110 + <Name>1.3 - 1.6 MeV/n</Name>
  111 + <Index>1</Index>
  112 + <ParameterKey>soho_erne_leda(0)</ParameterKey>
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  129 + <Element>
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  131 + <Index>5</Index>
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  134 + <Element>
  135 + <Name>4.0 - 5.0 MeV/n</Name>
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  147 + <ParameterKey>soho_erne_leda(7)</ParameterKey>
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... ...
Observatory/CDPP-AMDA/SOHO.xml 0 → 100644
... ... @@ -0,0 +1,43 @@
  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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  3 + <Version>2.3.1</Version>
  4 + <Observatory>
  5 + <ResourceID>spase://CNES/Observatory/CDPP-AMDA/SOHO</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>SOHO</ResourceName>
  8 + <AlternateName>1995-065A</AlternateName>
  9 + <AlternateName>Solar and Heliospheric Observatory</AlternateName>
  10 + <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
  11 + <Description>The primary scientific aims of the Solar and Heliospheric Observatory mission (SOHO) were to investigate: (1) the physical processes that form and heat the Sun's corona, maintain it and give rise to the expanding solar wind; and, (2) the interior structure of the Sun. Imaging and collection of spectroscopic plasma diagnostics of the solar chromosphere, transition region and corona, as well as in situ solar-wind measurements are used to study the corona and solar wind. Solar interior structure is investigated by helioseismological means and by the observation of variations in solar irradiance. SOHO was part of the International Solar-Terrestrial Physics Program (ISTP).
  12 +
  13 +The SOHO spacecraft was three-axis stabilized and pointed towards the Sun with an accuracy of +/- 10 arcsec per 15 min. It consisted of a Payload Module to accommodate the instruments and a Service Module carrying the spacecraft subsystems and solar arrays. SOHO occupied a halo orbit at the Earth-Sun L1 Lagrangian point to obtain uninterrupted sunlight. The design life was two years, but on-board consumables were sufficient for an extra four years of operations.
  14 +
  15 +Twelve instruments comprised the payload, producing a continuous stream of data at 40 kbs, except whenever the solar oscillations imager Michelson Doppler Imager (MDI) was operated in high-bit-rate mode, producing 160 kbs. The high-bit-rate mode was used during scheduled daily eight-hour periods or during dedicated campaigns. Magnetic tape stored data between telemetry contacts with the Experiment Operations Facility, located at NASA-GSFC. For more information, see B. Fleck, V. Domingo, and A. I. Poland, eds., Solar Physics, V. 162, 1995.
  16 +
  17 +SOHO was a joint mission of the European Space Agency and NASA. It was launched aboard an Atlas IIAS rocket from Cape Canaveral Air Station, FL, on Dec. 2, 1995, and mission operations were directed from NASA's Goddard Space Flight Center, Greenbelt, MD.
  18 +
  19 +In April 1998, SOHO successfully completed its nominal two-year mission to study the Sun's atmosphere, surface and interior. Major science highlights include the detection of rivers of plasma beneath the surface of the Sun; the discovery of a magnetic "carpet" on the solar surface that seems to account for a substantial part of the energy that is needed to cause the very high temperature of the corona, the Sun's outermost layer; the first detection of flare-induced solar quakes; the discovery of more than 50 sungrazing comets; the most detailed view to date of the solar atmosphere; and spectacular images and movies of coronal mass ejections, which were being used to improve the ability to forecast space weather.
  20 +
  21 +Contact with SOHO was lost at 23:16 GMT on June 24, 1998 during maintenance operations. The spacecraft went into emergency sun reacquisition mode, which is activated when an anomaly occurs and the spacecraft loses its orientation toward the Sun. When this happened, the spacecraft automatically tried to point itself toward the Sun again by firing its attitude control thrusters under the guidance of an onboard Sun sensor. Efforts to re-establish contact with SOHO did not succeed and telemetry was lost, not to be reestablished for several weeks.
  22 +
  23 +Attitude analysis led to the conclusion that SOHO went into a spin such that the solar panels were nearly edge-on towards the Sun, and thus did not generate any power. Because the spin axis is fixed in space, as the spacecraft progressed in its orbit the orientation of the panels with respect to the Sun gradually changed, resulting in increased solar illumination of the solar arrays as time progressed. On August 3, contact was re-established with SOHO following six weeks of silence. After a lengthy recovery process, on September 16 the spacecraft again locked onto the Sun, and experiment heaters were switched on. After recommissioning of various subsystems, and an orbit correction maneuver, SOHO was finally brought back to normal mode on 25 September at 19:52:58 GMT. Instrument switch-on started October 5, 1998, and by November 4 all instruments were back to normal.
  24 +</Description>
  25 + <Contact>
  26 + <PersonID>spase://SMWG/Person/Arthur.I.Poland</PersonID>
  27 + <Role>ProjectScientist</Role>
  28 + </Contact>
  29 + <InformationURL>
  30 + <Name>NSSDC's Master Catalog</Name>
  31 + <URL>https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1995-065A</URL>
  32 + <Description>Information about the SOHO mission
  33 +</Description>
  34 + </InformationURL>
  35 + </ResourceHeader>
  36 + <Location>
  37 + <ObservatoryRegion>Heliosphere.NearEarth</ObservatoryRegion>
  38 + </Location>
  39 + <OperatingSpan>
  40 + <StartDate>1995-12-02T00:00:00Z</StartDate>
  41 + </OperatingSpan>
  42 + </Observatory>
  43 +</Spase>
... ...