MGF.xml
2.07 KB
<?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/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>
</Spase>