Solar photo rates for planetary atmospheres and atmospheric pollutants

Details Solar photo rates for planetary atmospheres and atmospheric pollutants Solar photo rates for planetary atmospheres and atmospheric pollutants

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.195....1h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 195, no. 1, p. 1-289, 291-294.

Astronomy and Astrophysics

Astrophysics

272

Air Pollution, Photochemical Reactions, Planetary Atmospheres, Reaction Kinetics, Hydrogen Atoms, Hydrogen Ions, Negative Ions, Solar Activity Effects, Solar Flux Density

Scientific paper

Unattenuated solar photo rate coefficients and excess energies for dissociation, ionization, and dissociative ionization are presented for atomic and molecular species that have been identified or are suspected to exist in the atmospheres of planets, satellites (moons), comets, or as pollutants in the Earth atmosphere. The branching ratios and cross-sections with resonances have been tabulated to the greatest detail possible and the rate coefficients and excess energies have been calculated from them on a grid of small wavelength bins for the quiet and the active sun at 1 AU heliocentric distance.

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