MAG.xml 1.77 KB
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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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
  <Version>2.3.1</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/>
    <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Rosetta</ObservatoryID>
  </Instrument>
</Spase>