Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Saint Andrews, University, Scotland
Steady flows in solar magnetic structures - a class of exact MHD solutions.
The nonuniform magnetohydrodynamic nature of the solar corona. II - Generalization of basic solutions
The nonuniform magnetohydrodynamic nature of the solar corona. III - Cylindrical geometry
The nonuniform magnetohydrodynamic nature of the solar corona. IV - Effect of magnetogravity interactions
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