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Title: Response of middle atmosphere to short-term solar ultraviolet variations: 2. Theory

Journal Article · · J. Geophys. Res.; (United States)

Ozone and temperature responses to solar variability, based on satellite data, have been reported in a companion paper (Keating et. al., this issue). The present is intended to present a theoretical interpretation of this analysis with the purpose of better understanding the chemical behavior of the stratosphere and the coupling between temperature and ozone concentration, when a periodic forcing is applied to the solar ultraviolet (UV) flux. The response of the temperature and of the trace species concentrations, including ozone, to short-term variations in the solar UV irradiance is calculated by a one-dimensional chemical-radiative time-dependent model. The applied solar variability is assumed to be sinusoidal with a period of 27 days (in accordance with the rotation period of the sun) of 13.5 days (when two active regions are on opposite sides of the sun). The amplitude varies with wavelength, which is consistent with observations made by the Nimbus 7 solar backscattered ultraviolet (SBUV) experiment. The maximum ozone sensitivity in the stratosphere appears to be located near 3 mbar. The calculated amplitude and phase of the ozone response are significantly modified when the feedback between ozone and temperature is taken into account. The ozone/temperature coupling tends to modify the ozone phase lag such that, in the upper stratosphere and in the mesosphere, the ozone peak occurs a few days before the UV peak.

Research Organization:
National Center for Atmospheric Research, Boulder, Colorado
OSTI ID:
6695208
Journal Information:
J. Geophys. Res.; (United States), Vol. 92:D1, Issue D1
Country of Publication:
United States
Language:
English