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ARTEMIS SPASE metadata
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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/ARTEMIS/P1/ESA</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>ESA</ResourceName> | |
| 8 | + <ReleaseDate>2017-03-20T21:10:04Z</ReleaseDate> | |
| 9 | + <Description>The THEMIS Electrostatic Analyzers (ESAs) measures the flux of thermal particles in a 360° field of view over the energy range from ~3 eV to 30 keV. There are two ESAs on each THEMIS spacecraft, one measures ions, the other electrons. The ESA measures the full 3-D distributions, as well as the density, velocity, and temperature of the ambient electrons and ions.</Description> | |
| 10 | + <Acknowledgement> NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: C. W. Carlson and J. P. McFadden for use of ESA data. </Acknowledgement> | |
| 11 | + <Contact> | |
| 12 | + <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> | |
| 13 | + <Role>CoInvestigator</Role> | |
| 14 | + </Contact> | |
| 15 | + <Contact> | |
| 16 | + <PersonID>spase://SMWG/Person/James.P.McFadden</PersonID> | |
| 17 | + <Role>CoInvestigator</Role> | |
| 18 | + </Contact> | |
| 19 | + <InformationURL> | |
| 20 | + <Name>NSSDC description</Name> | |
| 21 | + <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2007-004A-02</URL> | |
| 22 | + <Description>Instrument description from NSSDC database</Description> | |
| 23 | + </InformationURL> | |
| 24 | + <InformationURL> | |
| 25 | + <Name>UCLA description</Name> | |
| 26 | + <URL>http://themis.igpp.ucla.edu/instrument_esa.shtml</URL> | |
| 27 | + <Description>Instrument description from UCLA</Description> | |
| 28 | + </InformationURL> | |
| 29 | + <PriorID>spase://SMWG/Instrument/ARTEMIS-P1/ESA</PriorID> | |
| 30 | + </ResourceHeader> | |
| 31 | + <InstrumentType>ElectrostaticAnalyser</InstrumentType> | |
| 32 | + <InvestigationName/> | |
| 33 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1</ObservatoryID> | |
| 34 | + <Caveats/> | |
| 35 | + </Instrument> | |
| 36 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,22 @@ |
| 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/ARTEMIS/P1/Ephemeris</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>Ephemeris</ResourceName> | |
| 8 | + <AlternateName>ARTEMIS-P1 Positions</AlternateName> | |
| 9 | + <ReleaseDate>2009-05-20T21:10:04Z</ReleaseDate> | |
| 10 | + <Description>ARTEMIS-P1 probe status (including position)</Description> | |
| 11 | + <Contact> | |
| 12 | + <!-- Vassilis Angelopoulos --> | |
| 13 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 14 | + <Role>PrincipalInvestigator</Role> | |
| 15 | + </Contact> | |
| 16 | + <PriorID>spase://SMWG/Instrument/ARTEMIS-P1/Ephemeris</PriorID> | |
| 17 | + </ResourceHeader> | |
| 18 | + <InstrumentType>Platform</InstrumentType> | |
| 19 | + <InvestigationName>Spacecraft position</InvestigationName> | |
| 20 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1</ObservatoryID> | |
| 21 | + </Instrument> | |
| 22 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,54 @@ |
| 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/ARTEMIS/P1/FGM</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>FGM</ResourceName> | |
| 8 | + <AlternateName>Tri-axial Fluxgate Magnetometer</AlternateName> | |
| 9 | + <ReleaseDate>2017-01-20T21:10:04Z</ReleaseDate> | |
| 10 | + <Description>THEMIS Flux Gate Magnetometer (FGM) measures the background magnetic field and any low frequency (to 64 Hz) fluctuations superimposed upon it. The FGM can detect variations in the magnetic field within the accuracy of 0.01 nT. The THEMIS FGM uses an updated technology developed in Germany that digitizes the sensor signals directly and replaces the analog hardware by software. Using the digital fluxgate technology results in lower mass of the instruments and improved robustness. | |
| 11 | + | |
| 12 | +Development Institution: Technical University of Braunschweig, (TU-BS), Germany | |
| 13 | +FGM Lead: K. H. Glassmeier (TUBS) | |
| 14 | + | |
| 15 | +The data are transimitted as several different types that vary in time resolution and availability. The fluxgate magnetometer engineering (FGE) quantity is available only during enginneering triggers(typically during perigee). FGE is provided at 1/8 second resolution, but is generally not processed to scientific quality standards. The fluxgate magnetometer low resolution data (FGL) is available during THEMIS fast survey mode. FGL is provided at 1/4 second time resolution. The FGL data is spin-phase corrected and calibrated on the ground for use in scientific data analysis. The fluxgate magnetometer high resolution data is available during THEMIS particle burst mode. It is provided at 1/128 second resolution. The FGH data is spin-phase corrected and calibrated on the ground for use in scientific data analysis. The fluxgate magnetometer spin fit data (FGS) is available at all times. It is provided at 3 second resolution; the nominal period of one THEMIS spacecraft resolution. FGS data is spin-phase corrected on-board. The equatorial correction is done using an A+B*sin(theta)+C*cos(theta) correction. Theta is the spinphase and a 0 spinphase is defined to be at the sunpulse. The Coefficients A,B, & C that were used in spin-phase correction can be found in the THEMIS level 1 FIT data CDF. The axial component of the FGS data is generated by taking the average of the z measurements over each spin. Additional calibrations and cleanup of FGS data may also be performed on the ground. All data types are provided in Despun Spacecraft L-Vector Corrected (DSL), Geocentric Solar Eclipitic(GSE), and Geocentric Solar Magnetospheric(GSM) coordinates. Information about the requested spacecraft mode can be found associated with the THEMIS housekeeping data CDF. The housekeeping cdf stores engineering quantities.</Description> | |
| 16 | + <Acknowledgement>NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission, K. H. Glassmeier, U. Auster and W. Baumjohann for the use of FGM data provided under the lead of the Technical University of Braunschweig and with financial support through the German Ministry for Economy and Technology and the German Center for Aviation and Space (DLR) under contract 50 OC 0302</Acknowledgement> | |
| 17 | + <Contact> | |
| 18 | + <!--Vassilis Angelopoulos --> | |
| 19 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 20 | + <Role>PrincipalInvestigator</Role> | |
| 21 | + </Contact> | |
| 22 | + <Contact> | |
| 23 | + <!-- Rumi Nakamura --> | |
| 24 | + <PersonID>spase://SMWG/Person/Rumi.Nakamura</PersonID> | |
| 25 | + <Role>CoInvestigator</Role> | |
| 26 | + </Contact> | |
| 27 | + <Contact> | |
| 28 | + <!-- Wolfgang Baumjohann --> | |
| 29 | + <PersonID>spase://SMWG/Person/Wolfgang.Baumjohann</PersonID> | |
| 30 | + <Role>CoInvestigator</Role> | |
| 31 | + </Contact> | |
| 32 | + <Contact> | |
| 33 | + <!-- Karl-Heinz Glassmeier --> | |
| 34 | + <PersonID>spase://SMWG/Person/Karl-Heinz.Glassmeier</PersonID> | |
| 35 | + <Role>CoInvestigator</Role> | |
| 36 | + </Contact> | |
| 37 | + <Contact> | |
| 38 | + <!-- Uli Auster --> | |
| 39 | + <PersonID>spase://SMWG/Person/Uli.Auster</PersonID> | |
| 40 | + <Role>TechnicalContact</Role> | |
| 41 | + </Contact> | |
| 42 | + <InformationURL> | |
| 43 | + <Name>THEMIS-B Fluxgate Magnetometer</Name> | |
| 44 | + <URL>http://nssdc.gsfc.nasa.gov/nmc/masterCatalog.do?sc=2007-004B</URL> | |
| 45 | + <Description>Instrument description from NSSDC database</Description> | |
| 46 | + </InformationURL> | |
| 47 | + <PriorID>spase://SMWG/Instrument/ARTEMIS-B/FGM</PriorID> | |
| 48 | + </ResourceHeader> | |
| 49 | + <InstrumentType>Magnetometer</InstrumentType> | |
| 50 | + <InvestigationName></InvestigationName> | |
| 51 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1</ObservatoryID> | |
| 52 | + <Caveats/> | |
| 53 | + </Instrument> | |
| 54 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,19 @@ |
| 1 | +<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"> | |
| 2 | + <Version>2.3.1</Version> | |
| 3 | + <Instrument> | |
| 4 | + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/ARTEMIS/P1/Models</ResourceID> | |
| 5 | + <ResourceHeader> | |
| 6 | + <ResourceName>Analytical Models</ResourceName> | |
| 7 | + <AlternateName>ThemisB different magnetospheric analytical models</AlternateName> | |
| 8 | + <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate> | |
| 9 | + <Description/> | |
| 10 | + <Contact> | |
| 11 | + <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID> | |
| 12 | + <Role>TechnicalContact</Role> | |
| 13 | + </Contact> | |
| 14 | + </ResourceHeader> | |
| 15 | + <InstrumentType>Platform</InstrumentType> | |
| 16 | + <InvestigationName/> | |
| 17 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1</ObservatoryID> | |
| 18 | + </Instrument> | |
| 19 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,36 @@ |
| 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/ARTEMIS/P2/ESA</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>ESA</ResourceName> | |
| 8 | + <ReleaseDate>2017-03-20T21:10:04Z</ReleaseDate> | |
| 9 | + <Description>The THEMIS Electrostatic Analyzers (ESAs) measures the flux of thermal particles in a 360° field of view over the energy range from ~3 eV to 30 keV. There are two ESAs on each THEMIS spacecraft, one measures ions, the other electrons. The ESA measures the full 3-D distributions, as well as the density, velocity, and temperature of the ambient electrons and ions.</Description> | |
| 10 | + <Acknowledgement> NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: C. W. Carlson and J. P. McFadden for use of ESA data. </Acknowledgement> | |
| 11 | + <Contact> | |
| 12 | + <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> | |
| 13 | + <Role>CoInvestigator</Role> | |
| 14 | + </Contact> | |
| 15 | + <Contact> | |
| 16 | + <PersonID>spase://SMWG/Person/James.P.McFadden</PersonID> | |
| 17 | + <Role>CoInvestigator</Role> | |
| 18 | + </Contact> | |
| 19 | + <InformationURL> | |
| 20 | + <Name>NSSDC description</Name> | |
| 21 | + <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2007-004A-02</URL> | |
| 22 | + <Description>Instrument description from NSSDC database</Description> | |
| 23 | + </InformationURL> | |
| 24 | + <InformationURL> | |
| 25 | + <Name>UCLA description</Name> | |
| 26 | + <URL>http://themis.igpp.ucla.edu/instrument_esa.shtml</URL> | |
| 27 | + <Description>Instrument description from UCLA</Description> | |
| 28 | + </InformationURL> | |
| 29 | + <PriorID>spase://SMWG/Instrument/ARTEMIS-P2/ESA</PriorID> | |
| 30 | + </ResourceHeader> | |
| 31 | + <InstrumentType>ElectrostaticAnalyser</InstrumentType> | |
| 32 | + <InvestigationName/> | |
| 33 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP2</ObservatoryID> | |
| 34 | + <Caveats/> | |
| 35 | + </Instrument> | |
| 36 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,22 @@ |
| 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/ARTEMIS/P2/Ephemeris</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>Ephemeris</ResourceName> | |
| 8 | + <AlternateName>ARTEMIS-P2 Positions</AlternateName> | |
| 9 | + <ReleaseDate>2009-05-20T21:10:04Z</ReleaseDate> | |
| 10 | + <Description>THEMIS-B probe status (including position)</Description> | |
| 11 | + <Contact> | |
| 12 | + <!-- Vassilis Angelopoulos --> | |
| 13 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 14 | + <Role>PrincipalInvestigator</Role> | |
| 15 | + </Contact> | |
| 16 | + <PriorID>spase://SMWG/Instrument/ARTEMIS-P2/Ephemeris</PriorID> | |
| 17 | + </ResourceHeader> | |
| 18 | + <InstrumentType>Platform</InstrumentType> | |
| 19 | + <InvestigationName>Spacecraft position</InvestigationName> | |
| 20 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP2</ObservatoryID> | |
| 21 | + </Instrument> | |
| 22 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,54 @@ |
| 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/ARTEMIS/P2/FGM</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>FGM</ResourceName> | |
| 8 | + <AlternateName>Tri-axial Fluxgate Magnetometer</AlternateName> | |
| 9 | + <ReleaseDate>2017-01-20T21:10:04Z</ReleaseDate> | |
| 10 | + <Description>THEMIS Flux Gate Magnetometer (FGM) measures the background magnetic field and any low frequency (to 64 Hz) fluctuations superimposed upon it. The FGM can detect variations in the magnetic field within the accuracy of 0.01 nT. The THEMIS FGM uses an updated technology developed in Germany that digitizes the sensor signals directly and replaces the analog hardware by software. Using the digital fluxgate technology results in lower mass of the instruments and improved robustness. | |
| 11 | + | |
| 12 | +Development Institution: Technical University of Braunschweig, (TU-BS), Germany | |
| 13 | +FGM Lead: K. H. Glassmeier (TUBS) | |
| 14 | + | |
| 15 | +The data are transimitted as several different types that vary in time resolution and availability. The fluxgate magnetometer engineering (FGE) quantity is available only during enginneering triggers(typically during perigee). FGE is provided at 1/8 second resolution, but is generally not processed to scientific quality standards. The fluxgate magnetometer low resolution data (FGL) is available during THEMIS fast survey mode. FGL is provided at 1/4 second time resolution. The FGL data is spin-phase corrected and calibrated on the ground for use in scientific data analysis. The fluxgate magnetometer high resolution data is available during THEMIS particle burst mode. It is provided at 1/128 second resolution. The FGH data is spin-phase corrected and calibrated on the ground for use in scientific data analysis. The fluxgate magnetometer spin fit data (FGS) is available at all times. It is provided at 3 second resolution; the nominal period of one THEMIS spacecraft resolution. FGS data is spin-phase corrected on-board. The equatorial correction is done using an A+B*sin(theta)+C*cos(theta) correction. Theta is the spinphase and a 0 spinphase is defined to be at the sunpulse. The Coefficients A,B, & C that were used in spin-phase correction can be found in the THEMIS level 1 FIT data CDF. The axial component of the FGS data is generated by taking the average of the z measurements over each spin. Additional calibrations and cleanup of FGS data may also be performed on the ground. All data types are provided in Despun Spacecraft L-Vector Corrected (DSL), Geocentric Solar Eclipitic(GSE), and Geocentric Solar Magnetospheric(GSM) coordinates. Information about the requested spacecraft mode can be found associated with the THEMIS housekeeping data CDF. The housekeeping cdf stores engineering quantities.</Description> | |
| 16 | + <Acknowledgement>NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission, K. H. Glassmeier, U. Auster and W. Baumjohann for the use of FGM data provided under the lead of the Technical University of Braunschweig and with financial support through the German Ministry for Economy and Technology and the German Center for Aviation and Space (DLR) under contract 50 OC 0302</Acknowledgement> | |
| 17 | + <Contact> | |
| 18 | + <!--Vassilis Angelopoulos --> | |
| 19 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 20 | + <Role>PrincipalInvestigator</Role> | |
| 21 | + </Contact> | |
| 22 | + <Contact> | |
| 23 | + <!-- Rumi Nakamura --> | |
| 24 | + <PersonID>spase://SMWG/Person/Rumi.Nakamura</PersonID> | |
| 25 | + <Role>CoInvestigator</Role> | |
| 26 | + </Contact> | |
| 27 | + <Contact> | |
| 28 | + <!-- Wolfgang Baumjohann --> | |
| 29 | + <PersonID>spase://SMWG/Person/Wolfgang.Baumjohann</PersonID> | |
| 30 | + <Role>CoInvestigator</Role> | |
| 31 | + </Contact> | |
| 32 | + <Contact> | |
| 33 | + <!-- Karl-Heinz Glassmeier --> | |
| 34 | + <PersonID>spase://SMWG/Person/Karl-Heinz.Glassmeier</PersonID> | |
| 35 | + <Role>CoInvestigator</Role> | |
| 36 | + </Contact> | |
| 37 | + <Contact> | |
| 38 | + <!-- Uli Auster --> | |
| 39 | + <PersonID>spase://SMWG/Person/Uli.Auster</PersonID> | |
| 40 | + <Role>TechnicalContact</Role> | |
| 41 | + </Contact> | |
| 42 | + <InformationURL> | |
| 43 | + <Name>THEMIS-B Fluxgate Magnetometer</Name> | |
| 44 | + <URL>http://nssdc.gsfc.nasa.gov/nmc/masterCatalog.do?sc=2007-004B</URL> | |
| 45 | + <Description>Instrument description from NSSDC database</Description> | |
| 46 | + </InformationURL> | |
| 47 | + <PriorID>spase://SMWG/Instrument/ARTEMIS-P2/FGM</PriorID> | |
| 48 | + </ResourceHeader> | |
| 49 | + <InstrumentType>Magnetometer</InstrumentType> | |
| 50 | + <InvestigationName></InvestigationName> | |
| 51 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP2</ObservatoryID> | |
| 52 | + <Caveats/> | |
| 53 | + </Instrument> | |
| 54 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,19 @@ |
| 1 | +<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"> | |
| 2 | + <Version>2.3.1</Version> | |
| 3 | + <Instrument> | |
| 4 | + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/ARTEMIS/P2/Models</ResourceID> | |
| 5 | + <ResourceHeader> | |
| 6 | + <ResourceName>Analytical Models</ResourceName> | |
| 7 | + <AlternateName>Artemis-P2 different magnetospheric analytical models</AlternateName> | |
| 8 | + <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate> | |
| 9 | + <Description/> | |
| 10 | + <Contact> | |
| 11 | + <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID> | |
| 12 | + <Role>TechnicalContact</Role> | |
| 13 | + </Contact> | |
| 14 | + </ResourceHeader> | |
| 15 | + <InstrumentType>Platform</InstrumentType> | |
| 16 | + <InvestigationName/> | |
| 17 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP2</ObservatoryID> | |
| 18 | + </Instrument> | |
| 19 | +</Spase> | ... | ... |
NumericalData/CDPP-AMDA/THEMIS/C/ESA/thc-esa-l2i.xml
| ... | ... | @@ -2,7 +2,7 @@ |
| 2 | 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 | 3 | <Version>2.3.1</Version> |
| 4 | 4 | <NumericalData> |
| 5 | - <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/thaMIS/C/ESA/thc-esa-l2i</ResourceID> | |
| 5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/ESA/thc-esa-l2i</ResourceID> | |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>ion full mode</ResourceName> |
| 8 | 8 | <ReleaseDate>2019-03-10T21:08:42Z</ReleaseDate> | ... | ... |
| ... | ... | @@ -0,0 +1,63 @@ |
| 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 | + <Observatory> | |
| 5 | + <ResourceID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>ARTEMIS-P1</ResourceName> | |
| 8 | + <AlternateName>Explorer 86</AlternateName> | |
| 9 | + <AlternateName>2007-004B</AlternateName> | |
| 10 | + <AlternateName>MIDEX/THEMIS</AlternateName> | |
| 11 | + <AlternateName>THEMIS-P1</AlternateName> | |
| 12 | + <AlternateName>ARTEMIS-P1</AlternateName> | |
| 13 | + <AlternateName>30581</AlternateName> | |
| 14 | + <ReleaseDate>2011-02-23T22:23:40Z</ReleaseDate> | |
| 15 | + <Description>The NASA/ARTEMIS mission include 2 satellites orbiting around the Moon. These satellites were initially part of the THEMIS mission. | |
| 16 | + | |
| 17 | +The Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission is a five-satellite Explorer mission whose primary objective is to understand the onset and macroscale evolution of magnetospheric substorms. Most importantly, THEMIS will find out which magnetotail process is responsible for substorm onset: (a) a local disruption of the plasma sheet current; or, (b) that current's interaction with the rapid influx of plasma emanating from lobe flux annihilation at ~25Re. Three inner probes at ~10Re will monitor current disruption onset, while two outer probes, at 20 and 30Re respectively, will remotely monitor plasma acceleration due to lobe flux dissipation. The five small satellites were launched together on a Delta II rocket and they carry identical sets of instruments including an electric field instrument (EFI), a flux gate magnetometer (FGM), a search coil magnetometer (SCM), a electro-static analyzer, and solid state telescopes (SST). The mission consists of several phases. In the first phase, the spacecraft will all orbit as a tight cluster in the same orbital plane with apogee at 15.4 Earth radii (RE). In the second phase, also called the Dawn Phase, the satellites will be placed in their orbits and during this time their apogees will be on the dawn side of the magnetosphere. During the third phase (also known as the Tail Science Phase) the apogees will be in the magnetotail. The fourth phase is called the Dusk Phase or Radiation Belt Science Phase, with all apogees on the dusk side. In the fifth and final phase, the apogees will shift to the sunward side (Dayside Science Phase). | |
| 18 | + | |
| 19 | +All five satellites will have similar perigee altitudes (1.16-1.5 Re) but varying apogee altitudes (P1: ~30 RE, P2: ~20 RE, P3 & P4: ~12 RE, P5: ~10RE) with corresponding orbital periods of ~4, 2, and 1 days, respectively. This results in multi-point magnetic conjunctions. Every four days the satellites will line up along the Earth's magnetic tail with magnetic foot points in the North American sector, allowing the tracking of disturbances through different geospace regions from tail to ground. | |
| 20 | + | |
| 21 | +The satellite data will be combined with observations of the aurora from a network of 20 ground observatories (all sky imagers, magnetometers) across the North American continent. In addition to its primary goal, THEMIS will answer critical questions in radiation belt physics and solar wind - magnetosphere energy coupling. THEMIS is complementary to MMS in terms of the temporal and spatial scales of the phenomena observed by these two constellation missions. THEMIS's focus is macroscale, whereas MMS will observe micro/meso scale features. </Description> | |
| 22 | + <Acknowledgement>National Aeronautics and Space Administration/United States</Acknowledgement> | |
| 23 | + <Contact> | |
| 24 | + <!-- Vassilis Angelopoulos --> | |
| 25 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 26 | + <Role>PrincipalInvestigator</Role> | |
| 27 | + </Contact> | |
| 28 | + <Contact> | |
| 29 | + <!-- David Sibeck --> | |
| 30 | + <PersonID>spase://SMWG/Person/David.G.Sibeck</PersonID> | |
| 31 | + <Role>ProjectScientist</Role> | |
| 32 | + </Contact> | |
| 33 | + <InformationURL> | |
| 34 | + <Name>Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission </Name> | |
| 35 | + <URL>http://themis.ssl.berkeley.edu/index.shtml</URL> | |
| 36 | + <Description>THEMIS Mission Homepage</Description> | |
| 37 | + </InformationURL> | |
| 38 | + <InformationURL> | |
| 39 | + <Name>Information on Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission </Name> | |
| 40 | + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2007-004B</URL> | |
| 41 | + <Description>NSSDC Master Catalog information on the THEMIS Mission</Description> | |
| 42 | + </InformationURL> | |
| 43 | + </ResourceHeader> | |
| 44 | + <ObservatoryGroupID>spase://CNES/Observatory/CDPP-AMDA/Artemis</ObservatoryGroupID> | |
| 45 | + | |
| 46 | + <Location> | |
| 47 | + <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion> | |
| 48 | + <ObservatoryRegion>Heliosphere.NearEarth</ObservatoryRegion> | |
| 49 | + <ObservatoryRegion>Earth.Magnetosphere.Magnetotail</ObservatoryRegion> | |
| 50 | + <ObservatoryRegion>Earth.Magnetosphere.Main</ObservatoryRegion> | |
| 51 | + <ObservatoryRegion>Earth.Magnetosheath</ObservatoryRegion> | |
| 52 | + </Location> | |
| 53 | + <OperatingSpan> | |
| 54 | + <StartDate>2007-02-15T00:00:00</StartDate> | |
| 55 | + <Note>Initial phase : apogee 15.4Re : 2007-02-15 - 2007-09-15</Note> | |
| 56 | + <Note>Orbit Placement Phase: 2007-09-15 - 2007-12-15</Note> | |
| 57 | + <Note>Full constellation phase: 1.3 x 30 Re : 2007-12-15 - 2009-09-30</Note> | |
| 58 | + <Note>ARTEMIS: Translunar Injection Phase: complex orbits, deep tail and solar wind : 2009-10-01 – 2010-10-01</Note> | |
| 59 | + <Note>ARTEMIS: Lunar Lissajous: orbiting around lunar L1 and L2 Lagrangian points : 2010-10-01 – 2011-04-01</Note> | |
| 60 | + <Note>ARTEMIS: Lunar Orbit Phase: Equatorial orbit; 100 km x 19,000 km altitude, 26 hours period, 500 km - 5 Re probe separation : 2011-07-01 – present</Note> | |
| 61 | + </OperatingSpan> | |
| 62 | + </Observatory> | |
| 63 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,63 @@ |
| 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 | + <Observatory> | |
| 5 | + <ResourceID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP2</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>ARTEMIS-P2</ResourceName> | |
| 8 | + <AlternateName>Explorer 87</AlternateName> | |
| 9 | + <AlternateName>2007-004C</AlternateName> | |
| 10 | + <AlternateName>MIDEX/THEMIS</AlternateName> | |
| 11 | + <AlternateName>THEMIS-P2</AlternateName> | |
| 12 | + <AlternateName>ARTEMIS-P2</AlternateName> | |
| 13 | + <AlternateName>30582</AlternateName> | |
| 14 | + <ReleaseDate>2011-02-23T22:23:15Z</ReleaseDate> | |
| 15 | + <Description>The NASA/ARTEMIS mission include 2 satellites orbiting around the Moon. These satellites were initially part of the THEMIS mission. | |
| 16 | + | |
| 17 | +The Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission is a five-satellite Explorer mission whose primary objective is to understand the onset and macroscale evolution of magnetospheric substorms. Most importantly, THEMIS will find out which magnetotail process is responsible for substorm onset: (a) a local disruption of the plasma sheet current; or, (b) that current's interaction with the rapid influx of plasma emanating from lobe flux annihilation at ~25Re. Three inner probes at ~10Re will monitor current disruption onset, while two outer probes, at 20 and 30Re respectively, will remotely monitor plasma acceleration due to lobe flux dissipation. The five small satellites were launched together on a Delta II rocket and they carry identical sets of instruments including an electric field instrument (EFI), a flux gate magnetometer (FGM), a search coil magnetometer (SCM), a electro-static analyzer, and solid state telescopes (SST). The mission consists of several phases. In the first phase, the spacecraft will all orbit as a tight cluster in the same orbital plane with apogee at 15.4 Earth radii (RE). In the second phase, also called the Dawn Phase, the satellites will be placed in their orbits and during this time their apogees will be on the dawn side of the magnetosphere. During the third phase (also known as the Tail Science Phase) the apogees will be in the magnetotail. The fourth phase is called the Dusk Phase or Radiation Belt Science Phase, with all apogees on the dusk side. In the fifth and final phase, the apogees will shift to the sunward side (Dayside Science Phase). | |
| 18 | + | |
| 19 | +All five satellites will have similar perigee altitudes (1.16-1.5 Re) but varying apogee altitudes (P1: ~30 RE, P2: ~20 RE, P3 & P4: ~12 RE, P5: ~10RE) with corresponding orbital periods of ~4, 2, and 1 days, respectively. This results in multi-point magnetic conjunctions. Every four days the satellites will line up along the Earth's magnetic tail with magnetic foot points in the North American sector, allowing the tracking of disturbances through different geospace regions from tail to ground. | |
| 20 | + | |
| 21 | +The satellite data will be combined with observations of the aurora from a network of 20 ground observatories (all sky imagers, magnetometers) across the North American continent. In addition to its primary goal, THEMIS will answer critical questions in radiation belt physics and solar wind - magnetosphere energy coupling. THEMIS is complementary to MMS in terms of the temporal and spatial scales of the phenomena observed by these two constellation missions. THEMIS's focus is macroscale, whereas MMS will observe micro/meso scale features. </Description> | |
| 22 | + <Acknowledgement>National Aeronautics and Space Administration/United States</Acknowledgement> | |
| 23 | + <Contact> | |
| 24 | + <!-- Vassilis Angelopoulos --> | |
| 25 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 26 | + <Role>PrincipalInvestigator</Role> | |
| 27 | + </Contact> | |
| 28 | + <Contact> | |
| 29 | + <!-- David Sibeck --> | |
| 30 | + <PersonID>spase://SMWG/Person/David.G.Sibeck</PersonID> | |
| 31 | + <Role>ProjectScientist</Role> | |
| 32 | + </Contact> | |
| 33 | + <InformationURL> | |
| 34 | + <Name>Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission </Name> | |
| 35 | + <URL>http://themis.ssl.berkeley.edu/index.shtml</URL> | |
| 36 | + <Description>THEMIS Mission Homepage</Description> | |
| 37 | + </InformationURL> | |
| 38 | + <InformationURL> | |
| 39 | + <Name>Information on Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission </Name> | |
| 40 | + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2007-004C</URL> | |
| 41 | + <Description>NSSDC Master Catalog information on the THEMIS Mission</Description> | |
| 42 | + </InformationURL> | |
| 43 | + </ResourceHeader> | |
| 44 | + <ObservatoryGroupID>spase://CNES/Observatory/CDPP-AMDA/Artemis</ObservatoryGroupID> | |
| 45 | + | |
| 46 | + <Location> | |
| 47 | + <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion> | |
| 48 | + <ObservatoryRegion>Heliosphere.NearEarth</ObservatoryRegion> | |
| 49 | + <ObservatoryRegion>Earth.Magnetosphere.Magnetotail</ObservatoryRegion> | |
| 50 | + <ObservatoryRegion>Earth.Magnetosphere.Main</ObservatoryRegion> | |
| 51 | + <ObservatoryRegion>Earth.Magnetosheath</ObservatoryRegion> | |
| 52 | + </Location> | |
| 53 | + <OperatingSpan> | |
| 54 | + <StartDate>2007-02-15T00:00:00</StartDate> | |
| 55 | + <Note>Initial phase : apogee 15.4Re : 2007-02-15 - 2007-09-15</Note> | |
| 56 | + <Note>Orbit Placement Phase: 2007-09-15 - 2007-12-15</Note> | |
| 57 | + <Note>Full constellation phase: 1.2 x 20 Re : 2007-12-15 - 2009-09-30</Note> | |
| 58 | + <Note>ARTEMIS: Translunar Injection Phase: complex orbits, deep tail and solar wind : 2009-10-01 – 2010-10-01</Note> | |
| 59 | + <Note>ARTEMIS: Lunar Lissajous: orbiting around lunar L1 and L2 Lagrangian points : 2010-10-01 – 2011-04-01</Note> | |
| 60 | + <Note>ARTEMIS: Lunar Orbit Phase: Equatorial orbit; 100 km x 19,000 km altitude, 26 hours period, 500 km - 5 Re probe separation : 2011-07-01 – present</Note> | |
| 61 | + </OperatingSpan> | |
| 62 | + </Observatory> | |
| 63 | +</Spase> | ... | ... |
| ... | ... | @@ -0,0 +1,54 @@ |
| 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 | + <Observatory> | |
| 5 | + <ResourceID>spase://CNES/Observatory/CDPP-AMDA/Artemis</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>ARTEMIS</ResourceName> | |
| 8 | + <AlternateName>Time History of Events and Macroscale Interactions during Substorms; NASA Magnetospheric Mission</AlternateName> | |
| 9 | + <ReleaseDate>2010-09-24T21:35:00Z</ReleaseDate> | |
| 10 | + <Description>THEMIS answers longstanding fundamental questions concerning the nature of the substorm instabilities that abruptly and explosively release solar wind energy stored within the Earth’s magnetotail. The primary objectives of the mission are to | |
| 11 | + | |
| 12 | + * Establish when and where substorms begin | |
| 13 | + * Determine how the individual components of the substorm interact | |
| 14 | + * Determine how substorms power the aurora, and | |
| 15 | + * Identify how local current disruption mechanisms couple to the more global substorm phenomena | |
| 16 | + | |
| 17 | +THEMIS accomplishes these tasks by employing 5 identically-instrumented spacecraft in carefully chosen orbits whose apogees line up once every 4 days over a dedicated array of ground observatories located in Canada and the northern United States. | |
| 18 | + | |
| 19 | +Three inner probes ~10 Earth radii (RE) from Earth monitor current disruption onset, while two outer probes at 20 and 30RE remotely monitor plasma acceleration due to lobe flux dissipation. Magnetic field lines map phenomena occurring at the inner spacecraft to the ground arrays, where they can be observed as nightside auroral displays and geomagnetic perturbations. | |
| 20 | + | |
| 21 | +The array of spacecraft and ground observations will enable researchers to pinpoint when and where substorms begin, thereby distinguishing between models that begin with current disruption in the near-Earth magnetotail and those that begin with magnetic reconnection in the distant magnetotail. The same array of spacecraft and ground observatories permits researchers to link phenomena observed in the magnetotail to those observed in the ionosphere. | |
| 22 | + | |
| 23 | +THEMIS employs flight-proven instruments and subsystems, yet demonstrates spacecraft design strategies ideal for Constellation class missions. THEMIS complements MMS and serves as a science and a technology pathfinder for future STP missions. THEMIS was launched on February 17, 2007.</Description> | |
| 24 | + <Acknowledgement>National Aeronautics and Space Administration/United States</Acknowledgement> | |
| 25 | + <Contact> | |
| 26 | + <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID> | |
| 27 | + <Role>PrincipalInvestigator</Role> | |
| 28 | + </Contact> | |
| 29 | + <Contact> | |
| 30 | + <PersonID>spase://SMWG/Person/David.G.Sibeck</PersonID> | |
| 31 | + <Role>ProjectScientist</Role> | |
| 32 | + </Contact> | |
| 33 | + <InformationURL> | |
| 34 | + <Name>Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission </Name> | |
| 35 | + <URL>http://themis.ssl.berkeley.edu/index.shtml</URL> | |
| 36 | + <Description>THEMIS Mission Homepage</Description> | |
| 37 | + </InformationURL> | |
| 38 | + </ResourceHeader> | |
| 39 | + <Location> | |
| 40 | + <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion> | |
| 41 | + <ObservatoryRegion>Earth.Magnetosphere.Magnetotail</ObservatoryRegion> | |
| 42 | + <ObservatoryRegion>Earth.Magnetosphere.Main</ObservatoryRegion> | |
| 43 | + <ObservatoryRegion>Earth.Magnetosheath</ObservatoryRegion> | |
| 44 | + <ObservatoryRegion>Heliosphere.NearEarth</ObservatoryRegion> | |
| 45 | + </Location> | |
| 46 | + <OperatingSpan> | |
| 47 | + <StartDate>2007-02-17T00:00:00</StartDate> | |
| 48 | + <Note>Initial phase: 2007-02-15 - 2007-09-15</Note> | |
| 49 | + <Note>Orbit Placement Phase: 2007-09-15 - 2007-12-15</Note> | |
| 50 | + <Note>Full constellation phase: 2007-12-15 - 2009-09-30</Note> | |
| 51 | + <Note>THEMIS and ARTEMIS: 2009-10-01 - present</Note> | |
| 52 | + </OperatingSpan> | |
| 53 | + </Observatory> | |
| 54 | +</Spase> | ... | ... |