The H Lyman-a actinic flux in the middle atmosphere T. Reddmann and R. Uhl Institute of Meteorology and Climate Research, Forschungszentrum Karlsruhe und Universität Karlsruhe, Germany
Abstract. The penetration of solar H
Lyman-a radiation into the
terrestrial middle atmosphere is studied in detail. The Lyman-a
actinic flux is calculated with a Monte Carlo approach including multiple resonance scattering of
photons within the terrestrial atmosphere and a temperature dependent absorption cross section of molecular oxygen. The
dependence of the actinic flux on the temperature profile is significant for
O2 column densities greater than about 1024 m-2. For column densities greater than about
5 · 1024 m-2 resonance scattering becomes important at solar zenith angles
> 60°. The O(1D) quantum yield of the O2 dissociation by
photons is found to decrease from 0.58 in the lower thermosphere to 0.48 in
the lower mesosphere. Parameterisations for Lyman-a
actinic flux, mean O2 absorption cross section and O(1D)
quantum yield including temperature dependence and resonance scattering are given valid up to a
O2 column density of about 1025 m-2.
Citation: Reddmann, T. and Uhl, R.: The H Lyman-a actinic flux in the middle atmosphere, Atmos. Chem. Phys., 3, 225-231, doi:10.5194/acp-3-225-2003, 2003.