The sodium exosphere of Mercury: Comparison between observations during Mercury's transit and model results

Details The sodium exosphere of Mercury: Comparison between observations during Mercury's transit and model results The sodium exosphere of Mercury: Comparison between observations during Mercury's transit and model results

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009icar..200....1m&link_type=abstract

Icarus, Volume 200, Issue 1, p. 1-11.

Astronomy and Astrophysics

Astrophysics

18

Scientific paper

In this study we compare the sodium exosphere observations made by Schleicher et al. [Schleicher, H., and 4 colleagues, 2004. Astron. Astrophys. 425, 1119 1124] with the result of a detailed numerical simulation. The observations, made during the transit of Mercury across the solar disk on 7 May 2003, show a maximum of sodium emission near the polar regions, with north prevalence, and the presence of a dawn dusk asymmetry. We interpret this distribution as the resulting effect of two combined processes: the solar wind proton precipitation causing chemical alteration of the surface, freeing the sodium atoms from their bounds in the crystalline structure on the surface, and the subsequent photon-stimulated and thermal desorption of the sodium atoms. While we find that the velocity distribution of photon desorbed sodium can explain the observed exosphere population, thermal desorption seems to play a minor role only causing a smearing at the locations where Na atoms are released on the dayside. The observed and simulated distributions agree very well with this hypothesis and indicate that the combination of the proposed processes is able to explain the observed features.

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