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Implications of MAVEN Mars near-wake measurements and models
Journal article   Open access   Peer reviewed

Implications of MAVEN Mars near-wake measurements and models

J. G. Luhmann, Chuanfei Dong, Yingjuan Ma, S. M. Curry, D. Mitchell, J. Espley, J. Connerney, J. Halekas, D. A. Brain, B. M. Jakosky, …
Geophysical research letters, Vol.42(21), pp.9087-9094
11/16/2015
DOI: 10.1002/2015GL066122
url
https://doi.org/10.1002/2015GL066122View
Published (Version of record) Open Access

Abstract

Mars is typically viewed as a member of the category of weakly magnetized planets, with a largely induced magnetosphere and magnetotail produced by the draped fields of the solar wind interaction. However, selected Mars Atmosphere and Volatile EvolutioN Mission (MAVEN) suprathermal electron and magnetic field observations in the near wake, sampled along its elliptical orbit during the early prime mission at altitudes ranging from its ~150 km periapsis to the tail magnetosheath, reinforce a picture seen in an MHD model where magnetic fields are rooted in the planet throughout much of the Martian magnetotail.
induced magnetosphere Mars magnetotail Mars-solar wind interaction

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