Investigation of spatial distribution of solar cosmic rays

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.