Titlebook: Comic Rays in Interplanetary Magnetics Fields; I. N. Toptygin Book 1985 D. Reidel Publishing Company, Dordrecht, Holland 1985 Corona.Plane

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Homeownership and Wealth Accumulation,of solar wind plasma particles. The energy of the most energetic particles detected in extensive atmospheric showers exceeds 10. eV. In this enormous energy range it is impossible to determine the exact critical energy which separates solar and galactic cosmic rays. However, since particles with T >

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https://doi.org/10.1007/978-94-009-5257-7Corona; Planet; Solar flare; Solar wind; solar

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Propagation of Energetic Solar Particles,article propagation in interplanetary space. The data presented are only basic and not totally complete. More detailed data may be found in the monograph by Dorman and Miroshnichenko (1968), and in the review by Dorman (1978).

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Physical Properties of the Interplanetary Medium,circumsolar space. This is a more or less continuous plasma flow which is generated in the upper corona of the Sun and carries magnetic fields of solar origin. The first indications of the existence of some corpuscular flow, directed from the Sun, in interplanetary space were obtained in the last ce

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Particle Acceleration Processes in Interplanetary Space,ses of particle energy variations have been considered, such as adiabatic deceleration in expanding streams of magnetic inhomogeneities (§8,1, 12, 13) and in large-scale magnetic fields frozen into the plasma (§8.4), as well as the Fermi acceleration by large-scale regular plasma motions (§8.3). Thi

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