Abstract
Abstract This article has two main objectives: (i) to elucidate the impact of non-dipolar part of geomagnetic field on the spatial distribution of cosmic radiation received over the globe, and (ii) to establish the influence of particles (with different origin and energies) on the atmospheric ozone profile. Our analyses show more evidence that lower stratospheric ozone at subtropics is sensitive to the radiation trapped by geomagnetic filed in Van-Allen radiation belts. At the same time, the high latitude ozone is vulnerable to the solar plasma, hitting the Earth after solar proton events.
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