Journal article
Implications of MAVEN Mars near-wake measurements and models
Geophysical research letters, Vol.42(21), pp.9087-9094
11/16/2015
DOI: 10.1002/2015GL066122
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.
Details
- Title: Subtitle
- Implications of MAVEN Mars near-wake measurements and models
- Creators
- J. G. Luhmann - University of California, BerkeleyChuanfei Dong - University of MichiganYingjuan Ma - Planetary Science InstituteS. M. Curry - University of California, BerkeleyD. Mitchell - University of California, BerkeleyJ. Espley - Goddard Space Flight CenterJ. Connerney - NASA/Goddard Space Flight Center, Maryland, Greenbelt, USAJ. Halekas - University of IowaD. A. Brain - Laboratory for Atmospheric and Space PhysicsB. M. Jakosky - Laboratory for Atmospheric and Space PhysicsC. Mazelle - Institut de Recherche en Astrophysique et Planétologie
- Resource Type
- Journal article
- Publication Details
- Geophysical research letters, Vol.42(21), pp.9087-9094
- DOI
- 10.1002/2015GL066122
- ISSN
- 0094-8276
- eISSN
- 1944-8007
- Publisher
- Blackwell Publishing Ltd
- Number of pages
- 8
- Grant note
- DOI: 10.13039/100000104, name: National Aeronautics and Space Administration
- Language
- English
- Date published
- 11/16/2015
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984428680702771
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