Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Evgeniya Mikhalko"'
Publikováno v:
Solnechno-Zemnaya Fizika. 8:29-34
The paper reports the results of simulation of cosmic ray proton transport through Earth’s atmosphere. The main objective of this work is to obtain characteristics of secondary particle fluxes at different altitudes and to convert them to equivalen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e93d77d99c2993526d7aadf724f1cc2
https://doi.org/10.12737/szf-83202204
https://doi.org/10.12737/szf-83202204
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 3, Pp 68-74 (2019)
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 se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7fc479a11fb155708d909b9a5587e601
https://doi.org/10.12737/szf-53201908
https://doi.org/10.12737/szf-53201908
Publikováno v:
Solar-Terrestrial Physics, Vol 4, Iss 1, Pp 71-74 (2018)
In the interaction of cosmic rays (CRs) with Earth’s atmosphere, neutrons are formed in a wide range of energies: from thermal (E≈0.025 eV) to ultrarelativistic (E>1 GeV). To detect and study CRs, Polar Geophysical Institute (PGI) uses a complex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97f0961c7a81eb2d1fa570b9e3e17b8b
https://doi.org/10.12737/stp-41201808
https://doi.org/10.12737/stp-41201808