<?xml version="1.0" encoding="UTF-8"?>

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  <Version>2.4.1</Version>

  <Instrument>

    <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MGF</ResourceID>

    <ResourceHeader>
      <ResourceName>MGF</ResourceName>

      <AlternateName>Mercury Fluxgate Magnetometer</AlternateName>

      <ReleaseDate>2020-09-22T16:02:13Z</ReleaseDate>

      <Description>The Fluxgate Magnetometer onboard Mio (MGF) measures the magnetic field to study various magnetospheric processes 
      (such as magnetic reconnection, field-aligned currents etc.) in Mercury’s magnetosphere, physics of bowshock and magnetosheath, 
      also magnetic field properties in the inner-heliosphere. It consists of two tir-axial fluxgate magnetometers and power supply units. 
      The magnetometer is able to observe the magnetic field with a vector rate of maximum 128 Hz. </Description>

       <Contact>       

         <PersonID>spase://SMWG/Person/Wolfgang.Baumjohann</PersonID> 

         <Role>PrincipalInvestigator</Role>
       </Contact>   
      <Contact>       

        <PersonID>spase://SMWG/Person/Ayako.Matsuoka</PersonID> 

        <Role>CoPI</Role>

      </Contact>

      <InformationURL>
        <Name>Mio Science Center</Name>
        <URL>https://miosc.isee.nagoya-u.ac.jp/about/satellite/mgf.php</URL>
      </InformationURL>
      <InformationURL>
        <Name>Baumjohann, W., Matsuoka, A., Narita, Y. et al. The BepiColombo–Mio Magnetometer en Route to Mercury. Space Sci Rev 216, 125 (2020).</Name>
        <URL>https://doi.org/10.1007/s11214-020-00754-y</URL>
        <Description>Reference paper</Description>
      </InformationURL>

    </ResourceHeader>
    <InstrumentType>Magnetometer</InstrumentType>

    <InvestigationName>Mercury Magnetometer on Mio</InvestigationName>

    <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/BepiColombo/Mio</ObservatoryID>

    </Instrument>

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