Calculations of temperature and barometric effects for cosmic ray flux on the Earth surface using the CORSIKA code. Journal of Physics: Conference Series Volume 409, Issue 1, 2013, Article number 012128

14 сентября 2018
128
Предметная область
Выходные данные
Ключевые слова
Вид публикации Статья
Контактные данные автора публикации Kovylyaeva, A.A. , Dmitrieva, A.N., Tolkacheva, N.V., Yakovleva, E.I. National Research Nuclear University MEPhI
Ссылка на публикацию в интернете www.scopus.com/record/display.url?origin=recordpage&eid=2-s2.0-84874329825&citeCnt=3&noHighlight=false&sort=plf-f&src=s&st1=MEPhI&nlo=&nlr=&nls=&sid=F0743CC1BB1CEC168410A18CB87C48A7.Vdktg6RVtMfaQJ4pNTCQ:6500&sot=b&sdt=b&sl=31&s=AFFIL(MEPhI) AND PU

Аннотация

Results of simulation of the spectra of cosmic rays (CR) on the Earth surface by means of the CORSIKA code are presented. For simulation, a standard model of the atmosphere and additional ones (with changed temperature profile and changed values of pressure at sea level) were used. Spectra of particles were obtained in the energy range 0.1 - 100 GeV for five values of zenith angle (0, 15, 30, 45 and 60 degrees) and, for the vertical direction, for several altitudes (0 m, 500 m, 1000 m and 1500 m above sea level). Barometric and temperature coefficients for various components of CR were estimated from the simulation data.



--------------------------------------------------------------------------------


Indexed keywords

Cosmic ray flux; Earth surface; Energy ranges; Simulation data; Standard model; Temperature coefficient; Temperature profiles; Vertical direction; Zenith angle
Подробнее
Для того чтобы оставить комментарий необходимо авторизоваться.