Abstract
We study the possibilities of the separation of solar electromagnetic and corpuscular impacts on the terrestrial lower atmosphere by examining their characteristic differences. We focus on the behaviour of the solar-meteorological correlation with respect to characteristic magnetic properties. Examples are given that the solar meteorological correlation — the efficiency of the solar impact — depends on the Sun-Earth attitude, the polarity of the solar main dipole field (and IMF) and the type of the geomagnetic events. This can explain the virtual disappearance or reversal of certain solar-meteorological effects.
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© 1994 Springer Science+Business Media Dordrecht
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Baranyi, T., Ludmány, A. (1994). Distinction between the Climatic Effects of the Solar Corpuscular and Electromagnetic Radiation. In: Pap, J.M., Fröhlich, C., Hudson, H.S., Tobiska, W.K. (eds) The Sun as a Variable Star: Solar and Stellar Irradiance Variations. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0950-5_44
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DOI: https://doi.org/10.1007/978-94-011-0950-5_44
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