Time evolution of the temperature altitudinal profile in the lower atmosphere during solar proton events

Details Time evolution of the temperature altitudinal profile in the lower atmosphere during solar proton events Time evolution of the temperature altitudinal profile in the lower atmosphere during solar proton events

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997jastp..59.2159p&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, v. 59, p. 2159-2166.

Physics

5

Scientific paper

Time variations of the temperature height profile in the lower atmosphere in the subauroral zone during Solar Proton Events (SPE) are calculated. The SPE situation is modelled by introducing a reflecting solar radiation layer at the upper tropospheric/lower stratospheric level. The characteristic time of the temperature variations is calculated. A comparison of model calculation results with experimental data on the temperature profile shows that the gross features of the observed variations of that profile may be reasonably explained by the model under consideration.

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