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Heliospheric structure due to magnetic fields and neutral particles from the three- dimensional MHD-kinetic model

Nikolai V. Pogorelov, J. Heerikhuisen, Iver H. Cairns, Gary Paul Zank, Sergey N. Borovikov, V. Florinski, Igor A. Kryukov

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Key concepts: Magnetohydrodynamics, Kinetic energy, Physics, Magnetic field, Classical mechanics, Quantum mechanics

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Heliospheric structure due to magnetic fields and neutral particles from the three- dimensional MHD-kinetic model — Research Paper | ScholarLens