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Large‐amplitude compressive “sawtooth” magnetic field oscillations in the Martian magnetosphere
Journal article   Open access   Peer reviewed

Large‐amplitude compressive “sawtooth” magnetic field oscillations in the Martian magnetosphere

J. S Halekas, D. A Brain and J. P Eastwood
Journal of Geophysical Research: Space Physics, Vol.116(A7), pp.1-n/a
07/2011
DOI: 10.1029/2011JA016590
url
https://doi.org/10.1029/2011JA016590View
Published (Version of record) Open Access

Abstract

We present Mars Global Surveyor mapping observations of large‐amplitude “sawtooth” magnetic field oscillations in the induced magnetosphere of Mars and discuss their possible origin. These highly compressive, linearly polarized, quasiperiodic features occur above the sunlit hemisphere of Mars, below the magnetosheath, but outside of photoelectron‐dominated regions. The correlation between solar zenith angle and estimated solar wind dynamic pressure at the sawtooth observation time and location at ∼400 km altitude suggests an association with a flared boundary, possibly the ionopause. Magnetic reconnection, ionospheric instabilities and/or irregularities, and crustal magnetic field effects may all play a role in generating these compressional features, with individual observations suggesting that each may at times prove important. These processes each have implications for magnetospheric dynamics and nonthermal ion escape from the Martian system. Key Points MGS observes large‐amplitude linearly polarized compressive oscillations at Mars Reconnection, ionospheric instabilities, and crustal fields may play a role These processes have important implications for nonthermal atmospheric loss
atmospheric loss ionospheric instabilities Mars reconnection

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