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MESSENGER observations of the spatial distribution of planetary ions near Mercury
Authors:Zurbuchen Thomas H  Raines Jim M  Slavin James A  Gershman Daniel J  Gilbert Jason A  Gloeckler George  Anderson Brian J  Baker Daniel N  Korth Haje  Krimigis Stamatios M  Sarantos Menelaos  Schriver David  McNutt Ralph L  Solomon Sean C
Affiliation:Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, USA. thomasz@umich.edu
Abstract:Global measurements by MESSENGER of the fluxes of heavy ions at Mercury, particularly sodium (Na(+)) and oxygen (O(+)), exhibit distinct maxima in the northern magnetic-cusp region, indicating that polar regions are important sources of Mercury's ionized exosphere, presumably through solar-wind sputtering near the poles. The observed fluxes of helium (He(+)) are more evenly distributed, indicating a more uniform source such as that expected from evaporation from a helium-saturated surface. In some regions near Mercury, especially the nightside equatorial region, the Na(+) pressure can be a substantial fraction of the proton pressure.
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