Get 20M+ Full-Text Papers For Less Than $1.50/day. Subscribe now for You or Your Team.

Learn More →

Solar photo rates for planetary atmospheres and atmospheric pollutants

Solar photo rates for planetary atmospheres and atmospheric pollutants 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. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Astrophysics and Space Science Springer Journals

Solar photo rates for planetary atmospheres and atmospheric pollutants

Astrophysics and Space Science , Volume 195 (1) – Oct 29, 2004

Loading next page...
 
/lp/springer-journals/solar-photo-rates-for-planetary-atmospheres-and-atmospheric-pollutants-trNcE319vs

References (219)

Publisher
Springer Journals
Copyright
Copyright
Subject
Physics; Astrophysics and Astroparticles; Astronomy, Observations and Techniques; Cosmology; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics); Astrobiology
ISSN
0004-640X
eISSN
1572-946X
DOI
10.1007/BF00644558
Publisher site
See Article on Publisher Site

Abstract

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.

Journal

Astrophysics and Space ScienceSpringer Journals

Published: Oct 29, 2004

There are no references for this article.