Inferring solar UV variability from the atmospheric tide

Details Inferring solar UV variability from the atmospheric tide Inferring solar UV variability from the atmospheric tide

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982natur.296..131c&link_type=abstract

Nature, vol. 296, Mar. 11, 1982, p. 131, 132. Research supported by the Natural Environment Research Council and Science Researc

Computer Science

8

Atmospheric Effects, Atmospheric Tides, Periodic Variations, Solar Radiation, Sunspot Cycle, Ultraviolet Radiation, Atmospheric Attenuation, Ozone, Stratosphere

Scientific paper

Solar UV output variations are determined by a novel method based on the fact that the 12-hour atmospheric tide is dominated by the component that is forced by ozone's UV absorption. Because this tide shows little interannual variability, and it can be shown that a change of 20% in UV would result in a 12% change in the 12-hour tide, the failure to find any solar cycle-related variation in this tide suggests a UV variation of less than 2% over the course of the sunspot cycle.

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