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On a connection between the characteristics of solar cosmic rays and the structure of the coronal magnetic field.

N. K. Pereyaslova, M. N. Nazarova, N. A. Mikirova

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Key concepts: Connection (principal bundle), Cosmic ray, Astronomy, Physics, Field (mathematics), Magnetic field, Nanoflares, Coronal mass ejection

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On a connection between the characteristics of solar cosmic rays and the structure of the coronal magnetic field. — Research Paper | ScholarLens