<?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-2.4.1.xsd">
  <Version>2.4.1</Version>

  <Instrument>

    <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Rosetta/MAG</ResourceID>

    <ResourceHeader>
      <ResourceName>MAG</ResourceName>

      <AlternateName>Fluxgate Magnetometer</AlternateName>

      <ReleaseDate>2017-01-01T21:10:13Z</ReleaseDate>
      <Description>The fluxgate magnetometer experiment onboard the ROSETTA spacecraft aims to measure
the magnetic field in the interaction region of the solar wind plasma with comet 67P/Churyumov-
Gerasimenko. It consists of a system of two ultra light (about 28 g each ) triaxial fluxgate magnetometer
sensors, mounted on the 1.5 m long spacecraft boom. The measurement range of each sensor is
±16384 nT with quantization steps of 31 pT. The magnetometer sensors are operated with a time
resolution of up to 0.05 s, corresponding to a bandwidth of 0–10 Hz. This performance of the RPC-
MAG sensors allows detailed analyses of magnetic field variations in the cometary environment. RPC-
MAG furthermore is designed to study possible remnant magnetic fields of the nucleus, measurements
which will be done in close cooperation with the ROSETTA lander magnetometer experiment ROMAP.
</Description>

      <Contact>       

        <PersonID>spase://SMWG/Person/Karl-Heinz.Glassmeier</PersonID>
        <Role>PrincipalInvestigator</Role>

      </Contact>
    </ResourceHeader>

    <InstrumentType>Magnetometer</InstrumentType>

    <InvestigationName>Fluxgate Magnetometer</InvestigationName>

    <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Rosetta</ObservatoryID>

  </Instrument>
</Spase>