544 research outputs found
On the Relationship of the Interplanetary Magnetic Field Turbulence and the Energy Spectrum of the Forbush Effects
On the expected deviation of the interplanetary magnetic field lines From the helioequatorial plane and the anisotropic diffusion tensor of galactic cosmic rays
The Galactic Cosmic Ray Intensity and Anisotrophy Variations for Different Ascending and Descending Epochs of Solar Activity
27-Day Variations Of The Galactic Cosmic Ray Intensity And Anisotropy In Different Solar Magnetic Cycles (1964-2004)
The expected cosmic ray density and stream distributions at the heliolatitudinal asymmetry of solar wind
The results of the spatial distribution of cosmic ray density, gradients, and anisotropy obtained on the basis of the numerical solution of the anisotropic diffusion equation with an account of solar wind velocity change depending on the latitudinal angle theta of the form U=u sub oe sup alpha theta and the diffusion coefficient depending on the spatial coordinates and the particle rigidity are presented. It is shown that the increase of the solar wind velocity and the diffusion coefficient with heliolatitude leads to gradient distributions that are in accord with experimental data observed in space. The results of the energetic spectrum of 11 and 22-year cosmic ray variations obtained with an account of direction of the general magnetic field of the Sun are presented are given
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