Heating of astrophysical plasma by mildly-relativistic non-thermal protons

DOI10.1007/BF00643845zbMath0724.76100OpenAlexW2051872989MaRDI QIDQ2277115

B. N. Dwivedi, A. L. Mackinnon

Publication date: 1991

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00643845

zbMATH Keywords

homogeneous magnetic fieldsolar atmospheremildly-relativistic, non-thermal protonsmonodirectional protons

Mathematics Subject Classification ID

Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

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