Atmospheric temperature response to solar cycle UV flux variations

Details Atmospheric temperature response to solar cycle UV flux variations Atmospheric temperature response to solar cycle UV flux variations

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..108..403v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 108, no. 2, 1987, p. 403-410.

Physics

1

Atmospheric Temperature, Periodic Variations, Radiant Flux Density, Solar Cycles, Solar Terrestrial Interactions, Ultraviolet Spectra, Atmospheric Models, Climatology, Convective Heat Transfer, Ozone, Radiative Heat Transfer, Solar Activity Effects, Stratospheric Warming

Scientific paper

A radiative-convective climate model was used to explore the response of the mean global vertical temperature structure to a variation in the solar UV flux over the solar cycle. The model predicted a cooling of the troposphere and a warming of the stratosphere from solar minimum to solar maximum. The response of the atmopsheric temperature to solar UV variations was found to be moderated by a concomitant change in the mean global stratospheric ozone content.

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