<?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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  <Version>2.3.1</Version>
  <Instrument>
    <ResourceID>spase://CNES/Instrument/CDPP-AMDA/MAVEN/EUV</ResourceID>
    <ResourceHeader>
      <ResourceName>EUV</ResourceName>
      <AlternateName>Extreme UltraViolet Monitor</AlternateName>
      <ReleaseDate>2016-08-01T22:37:00Z</ReleaseDate>
      <Description>The Extreme Ultraviolet (EUV) monitor is part of the Langmuir Probe and Waves (LPW) instrument and measures solar 
	      EUV input and variability, and wave heating of the Martian upper atmosphere. 
	      
	      Goals:

    * Measure solar emissions from different regions of the Sun in three distinct EUV bands
    * Three channels provide a complete EUV spectrum (0.1-190 nm) to serve as a proxy for
      input to the Flare Irradiance Spectral Model (FISM) model
      </Description>
      <Contact>       
        <PersonID>spase://CNES/Person/Frank.Eparvier</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <InformationURL>
        <Name>EUV web page, Summary sheet </Name>
        <URL>http://lasp.colorado.edu/home/maven/science/instrument-package/lpw/extreme-ultraviolet-euv-monitor/</URL>
      </InformationURL>      
    </ResourceHeader>
   <InstrumentType>Photometer</InstrumentType>
    <InvestigationName/>
    <OperatingSpan>
      <StartDate>2013-11-18T13:28:00</StartDate>
      <!--StopDate>2014-12-16T00:00:00</StopDate-->
      <!-- Note :  Mission phases : multiple tags possible -->
      <Note>Mars arrival : 2014-09-28T19:24:00</Note>
    </OperatingSpan>
    <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/MAVEN</ObservatoryID>
  </Instrument>
</Spase>