ESA.xml
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<?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/THEMIS/A/ESA</ResourceID>
<ResourceHeader>
<ResourceName>ESA</ResourceName>
<ReleaseDate>2009-05-20T21:10:04Z</ReleaseDate>
<Description>The THEMIS Electrostatic Analyzers (ESAs) measure 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>
<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>
<Contact>
<!--Vassilis Angelopoulos -->
<PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<Contact>
<!--Charles Carlson -->
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
<Role>CoInvestigator</Role>
</Contact>
<Contact>
<!--James Mcfadden -->
<PersonID>spase://SMWG/Person/James.P.McFadden</PersonID>
<Role>CoInvestigator</Role>
</Contact>
<InformationURL>
<Name>THEMIS-A Electrostatic Analyzers</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2007-004A-02</URL>
<Description>Instrument description from NSSDC database</Description>
</InformationURL>
<PriorID>spase://SMWG/Instrument/THEMIS-A/ESA</PriorID>
</ResourceHeader>
<InstrumentType>ElectrostaticAnalyser</InstrumentType>
<InvestigationName>Dual Full Distribution Electrostatic Analyzers</InvestigationName>
<ObservatoryID>spase://CDPP/Observatory/AMDA/THEMIS/A</ObservatoryID>
<Caveats/>
</Instrument>
</Spase>