MESSENGER Observations of the Spatial Distribution of Planetary Ions Near Mercury

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 spu...

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Veröffentlicht in:Science (American Association for the Advancement of Science) 2011-09, Vol.333 (6051), p.1862-1865
Hauptverfasser: 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.
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Sprache:eng
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Zusammenfassung: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.
ISSN:0036-8075
1095-9203
DOI:10.1126/science.1211302