Increase in the response of the earth's atmosphere to the sunspot cycle with height above sea level

Details Increase in the response of the earth's atmosphere to the sunspot cycle with height above sea level Increase in the response of the earth's atmosphere to the sunspot cycle with height above sea level

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...74..355s&link_type=abstract

(ESA and European Physical Society, ESLAB Symposium on Physics for Solar Variations, 14th, Scheveningen, Netherlands, Sept. 16-1

Physics

12

Atmospheric Effects, Atmospheric Temperature, Solar Activity Effects, Solar Cycles, Sunspots, Ionospheric Electron Density, Radiation Effects, Solar Flux, Solar Spectra, Stratosphere, Thermosphere, Troposphere

Scientific paper

An increase of effects on the earth atmosphere with height is demonstrated for the sunspot cycle. The solar flux is integrated to show constancy over a decade, and this is taken to imply that reductions in any wavelengths produce corresponding energy increases in other wavelengths; the highest variations occur at wavelengths below 175 nm. The necessity to record minute atmospheric variations over an entire sunspot cycle is stressed as necessary for firm correlations. Relations are expressed for the thermospheric and ionospheric influences of the sunspot cycle, the solar energy spectrum required for the formation of the daytime E-region is defined, and stratospheric and tropospheric temperature changes are compared. The total responses of the earth atmosphere to the sunspot cycle are found to be greater in winter than summer, greater effects are shown to be present in gradients outward from the planet, and directions for further, more precise characterizations are offered.

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