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The spatial distribution of planetary ion fluxes near Mars observed by MAVEN
Journal article   Open access   Peer reviewed

The spatial distribution of planetary ion fluxes near Mars observed by MAVEN

David A. Brain, J. P. Mcfadden, Jasper S. Halekas, J. E. P. Connerney, Stephen W. Bougher, Shannon Curry, C. F. Dong, Y. Dong, F. Eparvier, Xiaohua Fang, …
Geophysical research letters, Vol.42(21), pp.9142–9148-9148
11/16/2015
DOI: 10.1002/2015GL065293
url
https://doi.org/10.1002/2015GL065293View
Published (Version of record) Open Access

Abstract

We present the results of an initial effort to statistically map the fluxes of planetary ions on a closed surface around Mars. Choosing a spherical shell ~1000 km above the planet, we map both outgoing and incoming ion fluxes (with energies >25 eV) over a 4 month period. The results show net escape of planetary ions behind Mars and strong fluxes of escaping ions from the northern hemisphere with respect to the solar wind convection electric field. Planetary ions also travel toward the planet, and return fluxes are particularly strong in the southern electric field hemisphere. We obtain a lower bound estimate for planetary ion escape of ~3 × 1024 s−1, accounting for the ~10% of ions that return toward the planet and assuming that the ~70% of the surface covered so far is representative of the regions not yet visited by Mars Atmosphere and Volatile EvolutioN (MAVEN).
Astrophysics Earth and Planetary Astrophysics Sciences of the Universe Solar and Stellar Astrophysics

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