Evaluation of the Atmospheric Aerosol Particle Size in the Reflective Layer Produced by Strong Solar Flares.

摘要

It is well known, that nowadays one of the actual problem in the troposphere investigation is to connect solar activity with meteorological processes in the troposphere. But to present day there is no model. which explains all problem of solar terrestrial links. Investigation of influence of variation solar and cosmic rays on condition in the low and middle atmosphere take a significant part in determination parameters of this model. Experimental measurements of the low and middle atmosphere temperature profile 1 show, that it was changed after strong solar flares (Fig. 1). Theoretical model proposed in 1 explains this phenomena using atmospheric absorbent or reflective layer with heights from 5 till 20 km. Good agreement between experimental data and numerical simulation was achieved for layers with 14-16 and 8-9 km height respectively and coefficient of transparency about 90%.