Investigation of spatial distribution of solar cosmic rays
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Keywords:
solar flare, N-S asymmetry, radial gradientsAbstract
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.
References
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2 A.I. Kupchishin, A.Zh. Nauryzbaeva, E.A. Chebakova, Izvestija NAN RK. Serija fiz.-mat., 2,48-52, (2006) (in russ).
3 G. Erdos, J. Kota, Central Research Institute For Physics, Budapest, 16th International Cosmic ray Conference Kyoto, Japan, 6-18 August 1979.
4 Murzin V.S. Astrofizika kosmicheskih luchej / /Uchebnoe posobie dlja vuzov. - M: Universitetskaja kniga. Logos, 2007. – 488s. (in russ).
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How to Cite
Kantay, G., Kenzhina, I., Chebakova, E., & Boretskiy, O. (2016). Investigation of spatial distribution of solar cosmic rays. Recent Contributions to Physics (Rec.Contr.Phys.), 58(3), 106–111. Retrieved from https://bph.kaznu.kz/index.php/zhuzhu/article/view/920
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Section
Nonlinear Physics. Radiophysics
