CDPP / CNES

Commit 1d0d149350437ecce63f4ae03b3433913a3fb8f5

Authored by Elena.Budnik
1 parent b57ed075
Exists in master and in 12 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, branch_q, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

TIMED SEE

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Instrument/AMDA/TIMED/SEE.xml 0 → 100644
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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://www.spase-group.org/data/schema/spase-2_2_6.xsd">
  3 + <Version>2.2.6</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CDPP/Instrument/AMDA/TIMED/SEE</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>SEE</ResourceName>
  8 + <AlternateName>Solar EUV Experiment</AlternateName>
  9 + <ReleaseDate>2019-05-20T21:10:13Z</ReleaseDate>
  10 + <Description>One of the fundamental TIMED mission objectives is to understand the energetics in the mesosphere,
  11 + lower thermosphere and ionosphere (MLTI). Solar radiation below 200 nm is completely absorbed in the Earth’s
  12 + mesosphere and thermosphere. Changes in the amount of solar radiation, which range from 20% at the longer wavelengths
  13 + to factors as much as 1000 at the shorter wavelengths, result in corresponding changes in the photochemistry,
  14 + dynamics, and energy balance of the upper atmosphere. A detailed quantitative understanding of atmospheric radiative
  15 + processes, including changes in the solar ultraviolet irradiance arising from flares, solar rotation (27 day), or
  16 + the 11 year solar cycle, is fundamental to the TIMED investigations. The daily measurement of the full-disk solar
  17 + vacuum ultraviolet (VUV) irradiance by the SEE directly supports the TIMED mission requirement to measure the
  18 + sources of energy into the MLTI.
  19 +
  20 +The primary science objectives for SEE are to accurately and precisely determine the solar VUV absolute irradiance and
  21 +variability during the TIMED mission, to study the solar-terrestrial relationships utilizing atmospheric models, and to
  22 +improve proxy models of the solar VUV irradiance. The VUV range of 0 to 200 nm includes the soft x-ray (XUV) from 0 to 30 nm,
  23 +the extreme ultraviolet (EUV) from 0 to 120 nm, and the far ultraviolet (FUV) from 120 to 200 nm.
  24 +
  25 +Solar irradiance data will be provided to the TIMED science team and the solar-terrestrial community in general, and will be
  26 +integrated into the NCAR Thermosphere-Ionosphere-Mesosphere-Electrodynamics General Circulation Model (TIME-GCM) for
  27 +solar-terrestrial studies. The primary SEE data product is its Level 3 data product which includes a solar irradiance
  28 +spectrum in 1 nm intervals on 0.5 nm centers and the irradiance of the brighter 52 emissions in the solar VUV spectrum.
  29 +
  30 +For normal operations, SEE observes the Sun for about 3 minutes
  31 +every orbit (97 minutes), which usually gives 14-15 measurements
  32 +per day. The SEE Level 3 data are time averaged over the entire
  33 +day, after applying corrections for atmospheric absorption,
  34 +degradation, flare removal, and to 1-AU. A suborbital (sounding
  35 +rocket) payload is flown approximately once a year for TIMED SEE
  36 +absolute calibrations. The first SEE suborbital calibration flight was
  37 +on Feb. 8, 2002, the second was on Aug. 12, 2003, the third was
  38 +on Oct. 15, 2004, the fourth was on Oct. 28, 2006, and the final
  39 +SEE calibration flight was on Apr. 14, 2008. There are also three
  40 +SDO EVE calibration flights used for checking SEE degradation trends -
  41 +May 3, 2010, Mar. 23, 2011, June 23, 2012, Oct 21, 2013, and
  42 +June 1, 2016.
  43 +</Description>
  44 + <Contact>
  45 + <PersonID>spase://CDPP/Person/T.Woods</PersonID>
  46 + <Role>PrincipalInvestigator</Role>
  47 + </Contact>
  48 + <InformationURL>
  49 + <Name>SEE home</Name>
  50 + <URL>http://lasp.colorado.edu/home/see/documents/instrument</URL>
  51 + </InformationURL>
  52 + </ResourceHeader>
  53 + <InstrumentType>Photometer</InstrumentType>
  54 + <InvestigationName/>
  55 + <ObservatoryID>spase://CDPP/Observatory/AMDA/TIMED</ObservatoryID>
  56 + </Instrument>
  57 +</Spase>
... ...
NumericalData/AMDA/TIMED/SEE/timed-see-l3.xml 0 → 100644
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  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://cdpp.irap.omp.eu/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
  3 + <Version>2.2.6</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CDPP/NumericalData/AMDA/TIMED/SEE/timed-see-l3</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>daily averages</ResourceName>
  8 + <AlternateName>daily averages / level3 / flares excluded</AlternateName>
  9 + <ReleaseDate>2019-03-10T21:03:59Z</ReleaseDate>
  10 + <Description>
  11 + SEE Level 3 OVERVIEW:
  12 + The Solar EUV Experiment (SEE) is comprised of two science components:
  13 +* the EUV Grating Spectrograph (EGS) component covers the wavelength range from approximately 26 to 190 nm
  14 +* the X-Ray Photometer System (XPS) component covers the wavelength range from approximately 0.5 to 34 nm
  15 +
  16 +Level 3 data has flares removed, is useful for long-term climatological study.
  17 + </Description>
  18 + <Acknowledgement>
  19 + Users that wish to publish the results derived from TIMED
  20 +data should normally offer co-authorship to the PI or
  21 +his/her designated team member. Co-authorship may be
  22 +declined. Appropriate acknowledgement to institutions,
  23 +personnel, and funding agencies should be given.
  24 + </Acknowledgement>
  25 + <Contact>
  26 + <PersonID>spase://CDPP/Person/T.Woods</PersonID>
  27 + <Role>PrincipalInvestigator</Role>
  28 + </Contact>
  29 + <InformationURL>
  30 + <Name>Dataset description</Name>
  31 + <URL>http://lasp.colorado.edu/data/timed_see/level3/README_SEE_L3_012.TXT</URL>
  32 + <Description/>
  33 + </InformationURL>
  34 + <Association>
  35 + <AssociationID>timed-see-flux</AssociationID>
  36 + <AssociationType>PartOf</AssociationType>
  37 + <Note>EUV / X ray</Note>
  38 + </Association>
  39 + </ResourceHeader>
  40 + <AccessInformation>
  41 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  42 + <Availability>Online</Availability>
  43 + <AccessRights>Open</AccessRights>
  44 + <AccessURL>
  45 + <Name>AMDA at CDPP</Name>
  46 + <URL>http://amda.cdpp.eu</URL>
  47 + </AccessURL>
  48 + <Format>Text</Format>
  49 + <Acknowledgement>AMDA is a science analysis system provided by the Centre de Donnees de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Universite Paul Sabatier, Toulouse</Acknowledgement>
  50 + </AccessInformation>
  51 + <ProviderName>http://lasp.colorado.edu/data</ProviderName>
  52 + <ProviderResourceName>level3</ProviderResourceName>
  53 + <InstrumentID>spase://CDPP/Instrument/AMDA/TIMED/SEE</InstrumentID>
  54 + <MeasurementType>Irradiance</MeasurementType>
  55 + <TemporalDescription>
  56 + <TimeSpan>
  57 + <StartDate>1997-09-02T00:00:12Z</StartDate>
  58 + <StopDate>2019-03-02T23:59:47Z</StopDate>
  59 + </TimeSpan>
  60 + <Cadence>PT24H</Cadence>
  61 + </TemporalDescription>
  62 + <ObservedRegion>Earth.NearSurface.Ionosphere</ObservedRegion>
  63 + <Caveats>SEE Level 3 data files contain one daily averaged solar irradiance spectrum in 1 nm intervals extracted
  64 + from the EGS Level 2 and XPS Level 2 data products. Shortward of 27 nm, a solar model is scaled to match the
  65 + XPS broadband data. SEE Level 3 data files also contain 38 emission lines extracted from EGS Level 2 spectra,
  66 + and the XPS Level 2 diode irradiances.
  67 +
  68 +For normal operations, SEE observes the Sun for about 3 minutes every orbit (97 minutes), which usually gives 14-15
  69 +measurements per day. The SEE Level 3 data are time averaged over the entire day, after applying corrections for atmospheric
  70 +absorption, degradation, flare removal, and to 1 AU.
  71 + </Caveats>
  72 + <Parameter>
  73 + <Name>flux : spectra</Name>
  74 + <ParameterKey>timed_sp_daily</ParameterKey>
  75 + <Description>Merged median solar irradiance for XPS and EGS flux at 1nm bins</Description>
  76 + <Ucd/>
  77 + <Units>W/m**2/nm</Units>
  78 + <UnitsConversion></UnitsConversion>
  79 + <RenderingHints>
  80 + <DisplayType>Spectrogram</DisplayType>
  81 + </RenderingHints>
  82 + <FillValue>-1</FillValue>
  83 + </Parameter>
  84 + <Parameter>
  85 + <Name>flux : lines</Name>
  86 + <ParameterKey>timed_ln_daily</ParameterKey>
  87 + <Description>Integrated median spectral line irradiance</Description>
  88 + <Ucd/>
  89 + <Units>W/m**2/nm</Units>
  90 + <UnitsConversion></UnitsConversion>
  91 + <RenderingHints>
  92 + <DisplayType>TimeSeries</DisplayType>
  93 + </RenderingHints>
  94 + <FillValue>-1</FillValue>
  95 + </Parameter>
  96 +</NumericalData>
  97 +</Spase>
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NumericalData/AMDA/TIMED/SEE/timed-see-l3a.xml 0 → 100644
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  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://cdpp.irap.omp.eu/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
  3 + <Version>2.2.6</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CDPP/NumericalData/AMDA/TIMED/SEE/timed-see-l3</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>3 min avarages</ResourceName>
  8 + <AlternateName>3 min averages / level3a / flares included</AlternateName>
  9 + <ReleaseDate>2019-03-10T21:03:59Z</ReleaseDate>
  10 + <Description>
  11 + SEE Level 3A OVERVIEW:
  12 + The Solar EUV Experiment (SEE) is comprised of two science components:
  13 +* the EUV Grating Spectrograph (EGS) component covers the wavelength range from approximately 26 to 190 nm
  14 +* the X-Ray Photometer System (XPS) component covers the wavelength range from approximately 0.5 to 34 nm
  15 +
  16 +The Level 3A data product
  17 +contains irradiances for each observation average (~3 min). Level 3A does
  18 +not remove flares, so it is useful for short-term flare studies.
  19 + </Description>
  20 + <Acknowledgement>
  21 + Users that wish to publish the results derived from TIMED
  22 +data should normally offer co-authorship to the PI or
  23 +his/her designated team member. Co-authorship may be
  24 +declined. Appropriate acknowledgement to institutions,
  25 +personnel, and funding agencies should be given.
  26 + </Acknowledgement>
  27 + <Contact>
  28 + <PersonID>spase://CDPP/Person/T.Woods</PersonID>
  29 + <Role>PrincipalInvestigator</Role>
  30 + </Contact>
  31 + <InformationURL>
  32 + <Name>Dataset description</Name>
  33 + <URL>http://lasp.colorado.edu/data/timed_see/level3a/README_SEE_L3A_012.TXT</URL>
  34 + <Description/>
  35 + </InformationURL>
  36 + <Association>
  37 + <AssociationID>timed-see-flux</AssociationID>
  38 + <AssociationType>PartOf</AssociationType>
  39 + <Note>EUV / X ray</Note>
  40 + </Association>
  41 + </ResourceHeader>
  42 + <AccessInformation>
  43 + <RepositoryID>spase://SMWG/Repository/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>AMDA is a science analysis system provided by the Centre de Donnees de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Universite Paul Sabatier, Toulouse</Acknowledgement>
  52 + </AccessInformation>
  53 + <ProviderName>http://lasp.colorado.edu/data</ProviderName>
  54 + <ProviderResourceName>level3a</ProviderResourceName>
  55 + <InstrumentID>spase://CDPP/Instrument/AMDA/TIMED/SEE</InstrumentID>
  56 + <MeasurementType>Irradiance</MeasurementType>
  57 + <TemporalDescription>
  58 + <TimeSpan>
  59 + <StartDate>1997-09-02T00:00:12Z</StartDate>
  60 + <StopDate>2019-03-02T23:59:47Z</StopDate>
  61 + </TimeSpan>
  62 + <Cadence>PT90M</Cadence>
  63 + </TemporalDescription>
  64 + <ObservedRegion>Earth.NearSurface.Ionosphere</ObservedRegion>
  65 + <Caveats>SEE Level 3A data files contain observation averaged solar irradiance
  66 +spectra in 1 nm intervals extracted from the EGS Level 2A and XPS
  67 +Level 2A data products. Shortward of 27 nm, a solar model is scaled
  68 +to match the XPS broadband data. SEE Level 3A data files also contain
  69 +38 emission lines extracted from EGS Level 2A spectra, and the XPS
  70 +Level 2A diode irradiances.
  71 +
  72 +For normal operations, SEE observes the Sun for about 3 minutes every orbit (97 minutes), which usually gives 14-15
  73 +measurements per day. The SEE Level 3A data are time averaged over each observation,
  74 +after applying corrections for atmospheric absorption,
  75 +degradation, and to 1-AU (no flare removal). A suborbital (sounding
  76 +rocket) payload is flown approximately once a year for TIMED SEE
  77 +absolute calibrations. The first SEE suborbital calibration flight was
  78 +on Feb. 8, 2002, the second was on Aug. 12, 2003, the third was
  79 +on Oct. 15, 2004, the fourth was on Oct. 28, 2006, and the final
  80 +SEE calibration flight was on Apr. 14, 2008. There are also three
  81 +SDO EVE calibration flights used for checking SEE degradation trends -
  82 +May 3, 2010, Mar. 23, 2011, June 23, 2012, Oct 21, 2013, and
  83 +June 1, 2016.
  84 + </Caveats>
  85 + <Parameter>
  86 + <Name>flux : spectra</Name>
  87 + <ParameterKey>timed_sp_high</ParameterKey>
  88 + <Description>Merged median solar irradiance for XPS and EGS flux at 1nm bins</Description>
  89 + <Ucd/>
  90 + <Units>W/m**2/nm</Units>
  91 + <UnitsConversion></UnitsConversion>
  92 + <RenderingHints>
  93 + <DisplayType>Spectrogram</DisplayType>
  94 + </RenderingHints>
  95 + <FillValue>-1</FillValue>
  96 + </Parameter>
  97 + <Parameter>
  98 + <Name>flux : lines</Name>
  99 + <ParameterKey>timed_ln_high</ParameterKey>
  100 + <Description>Integrated median spectral line irradiance</Description>
  101 + <Ucd/>
  102 + <Units>W/m**2/nm</Units>
  103 + <UnitsConversion></UnitsConversion>
  104 + <RenderingHints>
  105 + <DisplayType>TimeSeries</DisplayType>
  106 + </RenderingHints>
  107 + <FillValue>-1</FillValue>
  108 + </Parameter>
  109 +</NumericalData>
  110 +</Spase>
... ...
Observatory/AMDA/Solar.xml 0 → 100644
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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://www.spase-group.org/data/schema/spase-2_2_6.xsd">
  3 + <Version>2.2.6</Version>
  4 + <Observatory>
  5 + <ResourceID>spase://CDPP/Observatory/AMDA/Solar</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>Solar Irradiance</ResourceName>
  8 + <AlternateName>Solar Irradiance : Different Missions : Different Locations</AlternateName>
  9 + <ReleaseDate>2019-05-27T18:45:12Z</ReleaseDate>
  10 + <Description>Solar Irradiance obtained from different missions :
  11 + * EUV / Xray - TIMED / SEE ( Dr. Thomas Woods )
  12 + * Gamma - Fermi / LAT
  13 + </Description>
  14 + <Contact>
  15 + <PersonID>spase://CDPP/Person/T.Woods</PersonID>
  16 + <Role>PrincipalInvestigator</Role>
  17 + </Contact>
  18 + <InformationURL>
  19 + <Name>TIMED home</Name>
  20 + <URL>http://www.timed.jhuapl.edu/WWW/index.php</URL>
  21 + </InformationURL>
  22 + </ResourceHeader>
  23 + <ObservatoryGroupID>spase://CDPP/Observatory/AMDA/Solar</ObservatoryGroupID>
  24 + <Location>
  25 + <ObservatoryRegion>Sun</ObservatoryRegion>
  26 + </Location>
  27 + <OperatingSpan>
  28 + <StartDate>2002-01-22T00:00:00</StartDate>
  29 + </OperatingSpan>
  30 + </Observatory>
  31 +</Spase>
... ...
Observatory/AMDA/TIMED.xml 0 → 100644
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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://www.spase-group.org/data/schema/spase-2_2_6.xsd">
  3 + <Version>2.2.6</Version>
  4 + <Observatory>
  5 + <ResourceID>spase://CDPP/Observatory/AMDA/TIMED</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>TIMED</ResourceName>
  8 + <AlternateName>Thermosphere Ionosphere Mesosphere Energetics and Dynamics</AlternateName>
  9 + <ReleaseDate>2019-05-27T18:45:12Z</ReleaseDate>
  10 + <Description>The TIMED (Thermosphere Ionosphere Mesosphere Energetics and Dynamics) mission is studying the influences
  11 + of the Sun and humans on the least explored and understood region of Earth's atmosphere - the Mesosphere and Lower
  12 + Thermosphere/Ionosphere (MLTI).
  13 + The MLTI region is a gateway between Earth's environment and space, where the Sun's energy is first
  14 + deposited into Earth's environment. TIMED is focusing on a portion of this atmospheric region located approximately
  15 + 40-110 miles (60-180 kilometers) above the surface.</Description>
  16 + <Contact>
  17 + <PersonID>spase://CDPP/Person/Diego.Janches</PersonID>
  18 + <Role>ProjectScientist</Role>
  19 + </Contact>
  20 + <InformationURL>
  21 + <Name>TIMED home</Name>
  22 + <URL>http://www.timed.jhuapl.edu/WWW/index.php</URL>
  23 + </InformationURL>
  24 + </ResourceHeader>
  25 + <ObservatoryGroupID>spase://CDPP/Observatory/AMDA/Solar</ObservatoryGroupID>
  26 + <Location>
  27 + <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion>
  28 + </Location>
  29 + <OperatingSpan>
  30 + <StartDate>2001-12-07T00:00:00</StartDate>
  31 + </OperatingSpan>
  32 + </Observatory>
  33 +</Spase>
... ...