Investigation of spatial distribution of solar cosmic rays

Authors

  • G.G. Kantay Al-Farabi Kazakh National University, Kazakstan, Almaty
  • I.E. Kenzhina Al-Farabi Kazakh National University, Kazakstan, Almaty
  • E.A. Chebakova Al-Farabi Kazakh National University, Kazakstan, Almaty
  • O.M. Boretskiy Al-Farabi Kazakh National University, Kazakstan, Almaty

Keywords:

solar flare, N-S asymmetry, radial gradients

Abstract

In this paper N-S asymmetry of solar cosmic rays (SCR) change were investigated during solar flares and radial density gradients for solar flares of 23-24 cycles of solar activity were calculated. Investigation of SCR propagation in interplanetary magnetic field (IMF) showed that the radial density gradients of SCR repeated stroke N-S asymmetry for flares with negative and zero anisotropy and for flares with positive values for N-S asymmetry - radial gradients and N-S asymmetry varies in anti-phase.

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Published

2016-09-12

Issue

Vol. 2016 No. 3 (2016): Recent Contributions to Physics

Section

Nonlinear Physics. Radiophysics

How to Cite

Investigation of spatial distribution of solar cosmic rays. (2016). Recent Contributions to Physics, 2016(3), 106-111. https://bph.kaznu.kz/index.php/zhuzhu/article/view/920

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