Does a region of the resonance fluorescence of atoms and ions around the sun exist?

Details Does a region of the resonance fluorescence of atoms and ions around the sun exist? Does a region of the resonance fluorescence of atoms and ions around the sun exist?

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..550s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, June 1990, p. 550-559. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

5

Interplanetary Dust, Metal Ions, Resonance Fluorescence, Solar Neighborhood, Calcium, Emission Spectra, Ion Atom Interactions, Line Spectra, Magnesium

Scientific paper

Based on data on the the average chemical composition and density of interplanetary dust, it is concluded that resonance fluorescence of the most abundant atoms and their first ions in the dust sublimation regions near the sun is possible. The intensities of the strongest lines in the visible and near-UV regions for Na, Ca, and Mg atoms and Ca II and Mg II ions are estimated. It is shown that the spectral intensity of the K Ca II line has the same order of magniutde (under the adopted assumptions) as the spectral intensity of the continuous daytime sky background in the vicinity of this line.

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