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First results of the MAVEN magnetic field investigation
Journal article   Open access   Peer reviewed

First results of the MAVEN magnetic field investigation

J. E. P Connerney, J. R Espley, G. A DiBraccio, J. R Gruesbeck, R. J Oliversen, D. L Mitchell, J Halekas, C Mazelle, D Brain and B. M Jakosky
Geophysical research letters, Vol.42(21), pp.8819-8827
11/16/2015
DOI: 10.1002/2015GL065366
url
https://doi.org/10.1002/2015GL065366View
Published (Version of record) Open Access

Abstract

Two Mars Atmosphere and Volatile EvolutioN magnetic field sensors sample the ambient magnetic field at the outer edge of each solar array. We characterized relatively minor spacecraft‐generated magnetic fields using in‐flight subsystem tests and spacecraft maneuvers. Dynamic spacecraft fields associated with the power subsystem (≤1 nT) are compensated for using spacecraft engineering telemetry to identify active solar array circuits and monitor their electrical current production. Static spacecraft magnetic fields are monitored using spacecraft roll maneuvers. Accuracy of measurement of the environmental magnetic field is demonstrated by comparison with field directions deduced from the symmetry properties of the electron distribution function measured by the Solar Wind Electron Analyzer. We map the bow shock, magnetic pileup boundary, the V × B convection electric field and ubiquitous proton cyclotron, and 1 Hz waves in the ion foreshock region. Key Points We observe, analyze, model, and mitigate spacecraft‐generated magnetic fields Measured field vectors are independently validated using electron analyzer observations We map the Mars magnetosphere, convection electric field, foreshock waves, and magnetotail
bow shock magnetic fields magnetometers magnetosheath magnetotail Mars

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