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Measurement of Magnetic Field Fluctuations in the Parker Solar Probe and Solar Orbiter Missions


AuthorJannet, G.; de Wit, Dudok; Krasnoselskikh, V.; Kretzschmar, M.; Fergeau, P.; Bergerard-Timofeeva, M.; Agrapart, C.; Brochot, J; Chalumeau, G.; Martin, P.; Revillet, C.; Bale, S.; Maksimovic, M.; Bowen, T.; Brysbaert, C.; Goetz, K.; Guilhem, E.; Harvey, P.; Leray, V.; Lorfèvre, E.;
KeywordsParker Data Used; magnetometer; parker solar probe; search coil; Solar Orbiter
AbstractThe search coil magnetometer (SCM) measures the magnetic signature of solar wind fluctuations with three components in the 3 Hz-50 kHz range and one single component in the 1 kHz-1 MHz range. This instrument is important for providing in situ observations of transients caused by interplanetary shocks and reconnection, for the identification of electromagnetic wave modes in plasmas and the determination of their characteristics (planarity, polarization, ellipticity, and k vector) and for studying the turbulent cascade in the kinetic range. Two similar triaxial search coils have been built for the Parker Solar Probe and Solar Orbiter missions. Here we describe the science objectives of both missions which led to the SCM design and present the characteristics of the two instruments.
Year of Publication2021
JournalJournal of Geophysical Research (Space Physics)
Volume126
Number of Pagese28543
Section
Date Published02/2021
ISBN
URLhttps://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2020JA028543
DOI10.1029/2020JA028543