A model of plasma sheath of magnetized planets: Self-similar case

In studying processes during solar flares or during the explosive phase of a substorm, problems of equilibrium and non-equilibrium configurations of magnetized plasma arise. First of all, it is extremely important to know a stationary state of the system in order to further study of it’s evolution....

Ausführliche Beschreibung

Bibliographische Detailangaben

Hauptverfasser:	Efremova, Svetlana A., Krymsky, Germogen F., Romashchenko, Yurii A.
Format:	Tagungsbericht
Sprache:	eng
Schlagworte:	Computational fluid dynamics Configurations Current distribution Dependence Equilibrium Fluid flow Magnetic flux Magnetohydrodynamics Magnetospheres Plasma sheaths Pulsars Ring structures Self-similarity Solar flares
Online-Zugang:	Volltext
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