Euler potential method in three-dimensional stellar wind problems

DOI10.1007/BF00668417zbMath0616.76055OpenAlexW2005500487MaRDI QIDQ1821654

Osamu Kaburaki

Publication date: 1985

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

Full work available at URL: https://doi.org/10.1007/bf00668417

zbMATH Keywords

electromagnetic fieldone-component plasmaMaxwell's equationsflat space-timerotating frameelectron-proton plasmarelativistic Euler equationEuler-type potentialsideal-MHD conditionintegrated Ohm's lawisentropic and quasi-stationary conditionslimit of vanishing mass ratioproblems of stellar windsrelativistic fluid equationsscalar super-potentialvector super-potential

Mathematics Subject Classification ID

Statistical mechanics of plasmas (82D10) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Planetary atmospheres (85A20) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

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