Ultra-violet argon dayglow lines in the atmosphere of mercury

Details Ultra-violet argon dayglow lines in the atmosphere of mercury Ultra-violet argon dayglow lines in the atmosphere of mercury

Mar 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21..383z&link_type=abstract

Planetary and Space Science, Volume 21, Issue 3, p. 383-389.

Physics

Scientific paper

We investigate the response of an atmosphere of argon to solar ultra-violet radiation. With the assumption that Mercury has an argon atmosphere that is optically thick to ionizing radiation the intensities of the ultra-violet dayglow lines resulting from photoelectron impact are calculated. For most of the model atmospheres, the predicted intensities are above the detection threshold of the 1973 Venus-Mercury ultra-violet spectrometer of Broadfoot, McElroy and Belton.

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