Solar-Terrestrial Physics Solar-Terrestrial Physics Solar-Terrestrial Physics 2500-0535 15165 10.12737/24269 Results of current research Results of current research Results of current research RUSCOSMIC — the new software toolbox for detailed analysis of cosmic ray interactions with matter RUSCOSMIC — the new software toolbox for detailed analysis of cosmic ray interactions with matter 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;

 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 23 01 2017 23 01 2017 2 4 3 10 https://zh-szf.ru/en/nauka/article/15165/view

At present, cosmic ray (CR) physics uses a considerable variety of methods for studying CR characteristics of both primary and secondary fluxes. Experimental methods make the main contribution, using various types of detectors, but numerical methods increasingly complement it due to the active development in computer technology. This approach provides researchers with the most extensive information about details of the process or phenomenon and allows us to make the most competent conclusions. This paper presents a concept of the RUSCOSMIC © software package based on the GEANT4 toolkit and representing a range of different numerical models for studying CR propagation through medium of different systems (radiation detectors, Earth’s atmosphere). The obtained results represent response functions of the main radiation detectors as well as some typical characteristics of secondary CR fluxes. Comparative results also show the operation of the module verification of calculations with experimental data.

At present, cosmic ray (CR) physics uses a considerable variety of methods for studying CR characteristics of both primary and secondary fluxes. Experimental methods make the main contribution, using various types of detectors, but numerical methods increasingly complement it due to the active development in computer technology. This approach provides researchers with the most extensive information about details of the process or phenomenon and allows us to make the most competent conclusions. This paper presents a concept of the RUSCOSMIC © software package based on the GEANT4 toolkit and representing a range of different numerical models for studying CR propagation through medium of different systems (radiation detectors, Earth’s atmosphere). The obtained results represent response functions of the main radiation detectors as well as some typical characteristics of secondary CR fluxes. Comparative results also show the operation of the module verification of calculations with experimental data.

 Cosmic rays Experimental techniques Numerical methods Monte Carlo method Radiation detectors Particle interaction with matter Cosmic rays Experimental techniques Numerical methods Monte Carlo method Radiation detectors Particle interaction with matter

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