diff --git a/Instrument/AMDA/TIMED/SEE.xml b/Instrument/AMDA/TIMED/SEE.xml new file mode 100644 index 0000000..704b92d --- /dev/null +++ b/Instrument/AMDA/TIMED/SEE.xml @@ -0,0 +1,57 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <Instrument> + <ResourceID>spase://CDPP/Instrument/AMDA/TIMED/SEE</ResourceID> + <ResourceHeader> + <ResourceName>SEE</ResourceName> + <AlternateName>Solar EUV Experiment</AlternateName> + <ReleaseDate>2019-05-20T21:10:13Z</ReleaseDate> + <Description>One of the fundamental TIMED mission objectives is to understand the energetics in the mesosphere, + lower thermosphere and ionosphere (MLTI). Solar radiation below 200 nm is completely absorbed in the Earth’s + mesosphere and thermosphere. Changes in the amount of solar radiation, which range from 20% at the longer wavelengths + to factors as much as 1000 at the shorter wavelengths, result in corresponding changes in the photochemistry, + dynamics, and energy balance of the upper atmosphere. A detailed quantitative understanding of atmospheric radiative + processes, including changes in the solar ultraviolet irradiance arising from flares, solar rotation (27 day), or + the 11 year solar cycle, is fundamental to the TIMED investigations. The daily measurement of the full-disk solar + vacuum ultraviolet (VUV) irradiance by the SEE directly supports the TIMED mission requirement to measure the + sources of energy into the MLTI. + +The primary science objectives for SEE are to accurately and precisely determine the solar VUV absolute irradiance and +variability during the TIMED mission, to study the solar-terrestrial relationships utilizing atmospheric models, and to +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, +the extreme ultraviolet (EUV) from 0 to 120 nm, and the far ultraviolet (FUV) from 120 to 200 nm. + +Solar irradiance data will be provided to the TIMED science team and the solar-terrestrial community in general, and will be +integrated into the NCAR Thermosphere-Ionosphere-Mesosphere-Electrodynamics General Circulation Model (TIME-GCM) for +solar-terrestrial studies. The primary SEE data product is its Level 3 data product which includes a solar irradiance +spectrum in 1 nm intervals on 0.5 nm centers and the irradiance of the brighter 52 emissions in the solar VUV spectrum. + +For normal operations, SEE observes the Sun for about 3 minutes +every orbit (97 minutes), which usually gives 14-15 measurements +per day. The SEE Level 3 data are time averaged over the entire +day, after applying corrections for atmospheric absorption, +degradation, flare removal, and to 1-AU. A suborbital (sounding +rocket) payload is flown approximately once a year for TIMED SEE +absolute calibrations. The first SEE suborbital calibration flight was +on Feb. 8, 2002, the second was on Aug. 12, 2003, the third was +on Oct. 15, 2004, the fourth was on Oct. 28, 2006, and the final +SEE calibration flight was on Apr. 14, 2008. There are also three +SDO EVE calibration flights used for checking SEE degradation trends - +May 3, 2010, Mar. 23, 2011, June 23, 2012, Oct 21, 2013, and +June 1, 2016. +</Description> + <Contact> + <PersonID>spase://CDPP/Person/T.Woods</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <InformationURL> + <Name>SEE home</Name> + <URL>http://lasp.colorado.edu/home/see/documents/instrument</URL> + </InformationURL> + </ResourceHeader> + <InstrumentType>Photometer</InstrumentType> + <InvestigationName/> + <ObservatoryID>spase://CDPP/Observatory/AMDA/TIMED</ObservatoryID> + </Instrument> +</Spase> diff --git a/NumericalData/AMDA/TIMED/SEE/timed-see-l3.xml b/NumericalData/AMDA/TIMED/SEE/timed-see-l3.xml new file mode 100644 index 0000000..2d00da1 --- /dev/null +++ b/NumericalData/AMDA/TIMED/SEE/timed-see-l3.xml @@ -0,0 +1,97 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <NumericalData> + <ResourceID>spase://CDPP/NumericalData/AMDA/TIMED/SEE/timed-see-l3</ResourceID> + <ResourceHeader> + <ResourceName>daily averages</ResourceName> + <AlternateName>daily averages / level3 / flares excluded</AlternateName> + <ReleaseDate>2019-03-10T21:03:59Z</ReleaseDate> + <Description> + SEE Level 3 OVERVIEW: + The Solar EUV Experiment (SEE) is comprised of two science components: +* the EUV Grating Spectrograph (EGS) component covers the wavelength range from approximately 26 to 190 nm +* the X-Ray Photometer System (XPS) component covers the wavelength range from approximately 0.5 to 34 nm + +Level 3 data has flares removed, is useful for long-term climatological study. + </Description> + <Acknowledgement> + Users that wish to publish the results derived from TIMED +data should normally offer co-authorship to the PI or +his/her designated team member. Co-authorship may be +declined. Appropriate acknowledgement to institutions, +personnel, and funding agencies should be given. + </Acknowledgement> + <Contact> + <PersonID>spase://CDPP/Person/T.Woods</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <InformationURL> + <Name>Dataset description</Name> + <URL>http://lasp.colorado.edu/data/timed_see/level3/README_SEE_L3_012.TXT</URL> + <Description/> + </InformationURL> + <Association> + <AssociationID>timed-see-flux</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>EUV / X ray</Note> + </Association> + </ResourceHeader> + <AccessInformation> + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> + <Availability>Online</Availability> + <AccessRights>Open</AccessRights> + <AccessURL> + <Name>AMDA at CDPP</Name> + <URL>http://amda.cdpp.eu</URL> + </AccessURL> + <Format>Text</Format> + <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> + </AccessInformation> + <ProviderName>http://lasp.colorado.edu/data</ProviderName> + <ProviderResourceName>level3</ProviderResourceName> + <InstrumentID>spase://CDPP/Instrument/AMDA/TIMED/SEE</InstrumentID> + <MeasurementType>Irradiance</MeasurementType> + <TemporalDescription> + <TimeSpan> + <StartDate>1997-09-02T00:00:12Z</StartDate> + <StopDate>2019-03-02T23:59:47Z</StopDate> + </TimeSpan> + <Cadence>PT24H</Cadence> + </TemporalDescription> + <ObservedRegion>Earth.NearSurface.Ionosphere</ObservedRegion> + <Caveats>SEE Level 3 data files contain one daily averaged solar irradiance spectrum in 1 nm intervals extracted + from the EGS Level 2 and XPS Level 2 data products. Shortward of 27 nm, a solar model is scaled to match the + XPS broadband data. SEE Level 3 data files also contain 38 emission lines extracted from EGS Level 2 spectra, + and the XPS Level 2 diode irradiances. + +For normal operations, SEE observes the Sun for about 3 minutes every orbit (97 minutes), which usually gives 14-15 +measurements per day. The SEE Level 3 data are time averaged over the entire day, after applying corrections for atmospheric +absorption, degradation, flare removal, and to 1 AU. + </Caveats> + <Parameter> + <Name>flux : spectra</Name> + <ParameterKey>timed_sp_daily</ParameterKey> + <Description>Merged median solar irradiance for XPS and EGS flux at 1nm bins</Description> + <Ucd/> + <Units>W/m**2/nm</Units> + <UnitsConversion></UnitsConversion> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <FillValue>-1</FillValue> + </Parameter> + <Parameter> + <Name>flux : lines</Name> + <ParameterKey>timed_ln_daily</ParameterKey> + <Description>Integrated median spectral line irradiance</Description> + <Ucd/> + <Units>W/m**2/nm</Units> + <UnitsConversion></UnitsConversion> + <RenderingHints> + <DisplayType>TimeSeries</DisplayType> + </RenderingHints> + <FillValue>-1</FillValue> + </Parameter> +</NumericalData> +</Spase> diff --git a/NumericalData/AMDA/TIMED/SEE/timed-see-l3a.xml b/NumericalData/AMDA/TIMED/SEE/timed-see-l3a.xml new file mode 100644 index 0000000..06de460 --- /dev/null +++ b/NumericalData/AMDA/TIMED/SEE/timed-see-l3a.xml @@ -0,0 +1,110 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <NumericalData> + <ResourceID>spase://CDPP/NumericalData/AMDA/TIMED/SEE/timed-see-l3</ResourceID> + <ResourceHeader> + <ResourceName>3 min avarages</ResourceName> + <AlternateName>3 min averages / level3a / flares included</AlternateName> + <ReleaseDate>2019-03-10T21:03:59Z</ReleaseDate> + <Description> + SEE Level 3A OVERVIEW: + The Solar EUV Experiment (SEE) is comprised of two science components: +* the EUV Grating Spectrograph (EGS) component covers the wavelength range from approximately 26 to 190 nm +* the X-Ray Photometer System (XPS) component covers the wavelength range from approximately 0.5 to 34 nm + +The Level 3A data product +contains irradiances for each observation average (~3 min). Level 3A does +not remove flares, so it is useful for short-term flare studies. + </Description> + <Acknowledgement> + Users that wish to publish the results derived from TIMED +data should normally offer co-authorship to the PI or +his/her designated team member. Co-authorship may be +declined. Appropriate acknowledgement to institutions, +personnel, and funding agencies should be given. + </Acknowledgement> + <Contact> + <PersonID>spase://CDPP/Person/T.Woods</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <InformationURL> + <Name>Dataset description</Name> + <URL>http://lasp.colorado.edu/data/timed_see/level3a/README_SEE_L3A_012.TXT</URL> + <Description/> + </InformationURL> + <Association> + <AssociationID>timed-see-flux</AssociationID> + <AssociationType>PartOf</AssociationType> + <Note>EUV / X ray</Note> + </Association> + </ResourceHeader> + <AccessInformation> + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> + <Availability>Online</Availability> + <AccessRights>Open</AccessRights> + <AccessURL> + <Name>AMDA at CDPP</Name> + <URL>http://amda.cdpp.eu</URL> + </AccessURL> + <Format>Text</Format> + <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> + </AccessInformation> + <ProviderName>http://lasp.colorado.edu/data</ProviderName> + <ProviderResourceName>level3a</ProviderResourceName> + <InstrumentID>spase://CDPP/Instrument/AMDA/TIMED/SEE</InstrumentID> + <MeasurementType>Irradiance</MeasurementType> + <TemporalDescription> + <TimeSpan> + <StartDate>1997-09-02T00:00:12Z</StartDate> + <StopDate>2019-03-02T23:59:47Z</StopDate> + </TimeSpan> + <Cadence>PT90M</Cadence> + </TemporalDescription> + <ObservedRegion>Earth.NearSurface.Ionosphere</ObservedRegion> + <Caveats>SEE Level 3A data files contain observation averaged solar irradiance +spectra in 1 nm intervals extracted from the EGS Level 2A and XPS +Level 2A data products. Shortward of 27 nm, a solar model is scaled +to match the XPS broadband data. SEE Level 3A data files also contain +38 emission lines extracted from EGS Level 2A spectra, and the XPS +Level 2A diode irradiances. + +For normal operations, SEE observes the Sun for about 3 minutes every orbit (97 minutes), which usually gives 14-15 +measurements per day. The SEE Level 3A data are time averaged over each observation, +after applying corrections for atmospheric absorption, +degradation, and to 1-AU (no flare removal). A suborbital (sounding +rocket) payload is flown approximately once a year for TIMED SEE +absolute calibrations. The first SEE suborbital calibration flight was +on Feb. 8, 2002, the second was on Aug. 12, 2003, the third was +on Oct. 15, 2004, the fourth was on Oct. 28, 2006, and the final +SEE calibration flight was on Apr. 14, 2008. There are also three +SDO EVE calibration flights used for checking SEE degradation trends - +May 3, 2010, Mar. 23, 2011, June 23, 2012, Oct 21, 2013, and +June 1, 2016. + </Caveats> + <Parameter> + <Name>flux : spectra</Name> + <ParameterKey>timed_sp_high</ParameterKey> + <Description>Merged median solar irradiance for XPS and EGS flux at 1nm bins</Description> + <Ucd/> + <Units>W/m**2/nm</Units> + <UnitsConversion></UnitsConversion> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <FillValue>-1</FillValue> + </Parameter> + <Parameter> + <Name>flux : lines</Name> + <ParameterKey>timed_ln_high</ParameterKey> + <Description>Integrated median spectral line irradiance</Description> + <Ucd/> + <Units>W/m**2/nm</Units> + <UnitsConversion></UnitsConversion> + <RenderingHints> + <DisplayType>TimeSeries</DisplayType> + </RenderingHints> + <FillValue>-1</FillValue> + </Parameter> +</NumericalData> +</Spase> diff --git a/Observatory/AMDA/Solar.xml b/Observatory/AMDA/Solar.xml new file mode 100644 index 0000000..b645ec2 --- /dev/null +++ b/Observatory/AMDA/Solar.xml @@ -0,0 +1,31 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <Observatory> + <ResourceID>spase://CDPP/Observatory/AMDA/Solar</ResourceID> + <ResourceHeader> + <ResourceName>Solar Irradiance</ResourceName> + <AlternateName>Solar Irradiance : Different Missions : Different Locations</AlternateName> + <ReleaseDate>2019-05-27T18:45:12Z</ReleaseDate> + <Description>Solar Irradiance obtained from different missions : + * EUV / Xray - TIMED / SEE ( Dr. Thomas Woods ) + * Gamma - Fermi / LAT + </Description> + <Contact> + <PersonID>spase://CDPP/Person/T.Woods</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <InformationURL> + <Name>TIMED home</Name> + <URL>http://www.timed.jhuapl.edu/WWW/index.php</URL> + </InformationURL> + </ResourceHeader> + <ObservatoryGroupID>spase://CDPP/Observatory/AMDA/Solar</ObservatoryGroupID> + <Location> + <ObservatoryRegion>Sun</ObservatoryRegion> + </Location> + <OperatingSpan> + <StartDate>2002-01-22T00:00:00</StartDate> + </OperatingSpan> + </Observatory> +</Spase> diff --git a/Observatory/AMDA/TIMED.xml b/Observatory/AMDA/TIMED.xml new file mode 100644 index 0000000..ae32eaa --- /dev/null +++ b/Observatory/AMDA/TIMED.xml @@ -0,0 +1,33 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <Observatory> + <ResourceID>spase://CDPP/Observatory/AMDA/TIMED</ResourceID> + <ResourceHeader> + <ResourceName>TIMED</ResourceName> + <AlternateName>Thermosphere Ionosphere Mesosphere Energetics and Dynamics</AlternateName> + <ReleaseDate>2019-05-27T18:45:12Z</ReleaseDate> + <Description>The TIMED (Thermosphere Ionosphere Mesosphere Energetics and Dynamics) mission is studying the influences + of the Sun and humans on the least explored and understood region of Earth's atmosphere - the Mesosphere and Lower + Thermosphere/Ionosphere (MLTI). + The MLTI region is a gateway between Earth's environment and space, where the Sun's energy is first + deposited into Earth's environment. TIMED is focusing on a portion of this atmospheric region located approximately + 40-110 miles (60-180 kilometers) above the surface.</Description> + <Contact> + <PersonID>spase://CDPP/Person/Diego.Janches</PersonID> + <Role>ProjectScientist</Role> + </Contact> + <InformationURL> + <Name>TIMED home</Name> + <URL>http://www.timed.jhuapl.edu/WWW/index.php</URL> + </InformationURL> + </ResourceHeader> + <ObservatoryGroupID>spase://CDPP/Observatory/AMDA/Solar</ObservatoryGroupID> + <Location> + <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion> + </Location> + <OperatingSpan> + <StartDate>2001-12-07T00:00:00</StartDate> + </OperatingSpan> + </Observatory> +</Spase> -- libgit2 0.21.2