Solar-Terrestrial Physics Solar-Terrestrial Physics Solar-Terrestrial Physics 2500-0535 30598 10.12737/stp-53201908 Results of current research Results of current research Results of current research Calculating the ionization rate induced by GCR and SCR protons in Earth’s atmosphere Calculating the ionization rate induced by GCR and SCR protons in Earth’s atmosphere Маурчев Евгений Александрович Maurchev Evgeniy Aleksandrovich maurchev@pgia.ru Балабин Юрий Васильевич Balabin Yuriy Vasilyevich balabin@pgia.ru

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 Германенко Алексей Владимирович Germanenko Aleksey Vladimirovich alex.germanenko@gmail.com

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 Михалко Евгения Александровна Mikhalko Evgeniya Aleksandrovna mikhalko@pgia.ru Гвоздевский Борис Борисович Gvozdevsky Boris Borisovich gvozdevsky@pgia.ru

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 Полярный геофизический институт КНЦ РАН Апатиты Россия Polar Geophysical Institute KSC RAS Apatity Russian Federation Полярный геофизический институт КНЦ РАН Апатиты Россия Polar Geophysical Institute KSC RAS Apatity Russian Federation Полярный геофизический институт КНЦ РАН Апатиты Россия Polar Geophysical Institute KSC RAS Apatity Russian Federation Полярный геофизический институт Россия Полярный геофизический институт Russian Federation Полярный геофизический институт КНЦ РАН Апатиты Россия Polar Geophysical Institute KSC RAS Apatity Russian Federation 5 3 68 74 https://zh-szf.ru/en/nauka/article/30598/view

This paper explores the applied use of the RUSCOSMICS software package [http://ruscosmics.ru] designed to simulate propagation of primary cosmic ray (CR) particles through Earth’s atmosphere and collect information about characteristics of their secondary component. We report the results obtained for proton fluxes with energy distributions corresponding to the differential spectra of galactic CR (GCR) and solar CR (SCR) during ground level enhancement (GLE) events GLE65 and GLE67. We examine features of the geometry of Earth’s atmosphere, parametrization methods, and describe a primary particle generator. The typical energy spectra of electrons obtained both for GCR and for GLE65 provide information that allows us to quantitatively estimate the SCR contribution to the enhancement of secondary CR fluxes. We also present altitude dependences of ionization rate for GCR and both the GLE events for several geomagnetic cutoff rigidity values. The conclusion summarizes and discusses the prospects for future research.

This paper explores the applied use of the RUSCOSMICS software package [http://ruscosmics.ru] designed to simulate propagation of primary cosmic ray (CR) particles through Earth’s atmosphere and collect information about characteristics of their secondary component. We report the results obtained for proton fluxes with energy distributions corresponding to the differential spectra of galactic CR (GCR) and solar CR (SCR) during ground level enhancement (GLE) events GLE65 and GLE67. We examine features of the geometry of Earth’s atmosphere, parametrization methods, and describe a primary particle generator. The typical energy spectra of electrons obtained both for GCR and for GLE65 provide information that allows us to quantitatively estimate the SCR contribution to the enhancement of secondary CR fluxes. We also present altitude dependences of ionization rate for GCR and both the GLE events for several geomagnetic cutoff rigidity values. The conclusion summarizes and discusses the prospects for future research.

 cosmic rays astrophysics Monte Carlo method GEANT4 particle physics numerical simulation cosmic rays astrophysics Monte Carlo method GEANT4 particle physics numerical simulation

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