Investigation of cosmic ray propagation in interplanetary space
It was established experimentally that propagation of solar cosmic rays (scr) in interplanetary space up to 1 AU in most cases was of diffusion character.
Engineering topics
Publications and source records attributed to Kolomeets, E. V..
It was established experimentally that propagation of solar cosmic rays (scr) in interplanetary space up to 1 AU in most cases was of diffusion character.
Aspects of the problem of galactic cosmic ray propagation, including inversion of the solar total magnetic field and an analysis of data related to the heliomagnetic cycle are discussed. It is noted that the global structure of the solar magnetic field results in an additional flux of galactic cosmic rays generated by curvature and gradient drifts. An analysis of heliomagnetic cycle data shows that the latitudinal gradient results in a N-S asymmetry, with the amplitude of the effect growing with depth in the atmosphere. The inversion of the solar total magnetic field, drift effects, and other space distributions are found to contribute to a 22-year cycle of solar activity.
The results are presented of the Monte Carlo simulation of albedo flux from the dense layers of the Earth's atmosphere and the dependence of angular distribution on the rigidity of geomagnetic cut off and additional flux of particles at the depth in the atmosphere 15-20 g/sq sm. Influence of geomagnetic field on the propagation of charged particles was not taken into account.
Cosmic ray intensity increase during Forbush decrease and reduction of geomagnetic horizontal component
Coupling coefficients for mesons passing through atmosphere taking into account nuclear interactions
Neutron monitor modifications and muon telescope design for cosmic ray studies