Abstract
It is shown that the behavior of the cosmic ray density in a magnetic cloud near the Earth can for most events be described by a simple parabolic dependence on a distance to the cloud’s center, measured in gyro radii. Most magnetic clouds modulate cosmic rays, lowering their density. However, there are events (approximately 1/5) in which the cosmic ray density rises in a magnetic cloud. Events with the positive effect usually have a maximum in the leading part of the cloud. Several factors are considered that contribute to a model description, and these contributions are estimated.
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Original Russian Text © A.V. Belov, A.A. Abunin, M.A. Abunina, E.A. Eroshenko, V.A. Oleneva, V.G. Yanke, 2015, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2015, Vol. 79, No. 5, pp. 691–693.
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Belov, A.V., Abunin, A.A., Abunina, M.A. et al. Modeling variations in CR density in magnetic clouds. Bull. Russ. Acad. Sci. Phys. 79, 637–639 (2015). https://doi.org/10.3103/S1062873815050159
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DOI: https://doi.org/10.3103/S1062873815050159