Atmos. Chem. Phys. Discuss., 10, 22317-22337, 2010
© Author(s) 2010. This work is distributed
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This discussion paper has been under review for the journal Atmospheric Chemistry and Physics (ACP). Please refer to the corresponding final paper in ACP.
Hydroxyl in the stratosphere and mesosphere – Part 1: Diurnal variability
K. Minschwaner1, G. L. Manney1,2, S. H. Wang2, and R. S. Harwood3
1Department of Physics, New Mexico Institute of Mining and Technology, Socorro, USA
2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, USA
3University of Edinburgh, Edinburgh, UK

Abstract. Diurnal variations in hydroxyl (OH) in the stratosphere and mesosphere are analyzed using measurements from the Aura Microwave Limb Sounder (MLS). The primary driver for OH diurnal variations is the ultraviolet actinic flux that initiates photochemical reactions which produce OH. The magnitude of this flux is governed largely by changes in solar zenith angle (SZA) throughout the day, and OH diurnal variations are well approximated by an exponential function of the secant of SZA. Measured OH concentrations are fit to a function of the form exp[−βsec(SZA)], where the parameter β is a function of altitude. We examine the magnitude of β and show that it is related to the optical depths of ultraviolet absorption by ozone and oxygen. Comparison of β values obtained from SLIMCAT model simulations with those derived from MLS observations shows very good agreement. The vertical profile of β from MLS can be represented by a simple analytic formulation involving the ozone and water vapor photodissociation rates. This formulation is used to infer the altitude dependence of the primary production mechanisms for OH: the reaction of excited-state atomic oxygen with water vapor versus the direct photodissociation of water vapor.

Citation: Minschwaner, K., Manney, G. L., Wang, S. H., and Harwood, R. S.: Hydroxyl in the stratosphere and mesosphere – Part 1: Diurnal variability, Atmos. Chem. Phys. Discuss., 10, 22317-22337, doi:10.5194/acpd-10-22317-2010, 2010.
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