On MHD stability of gravitating plasmas with field aligned flows
H. Tasso, G. N. Throumoulopoulos

TL;DR
This paper extends a known MHD stability condition for incompressible plasmas with field aligned flows to include self-gravitation, showing that gravity influences stability through equilibrium parameters.
Contribution
It introduces a modified stability criterion for gravitating plasmas, incorporating self-gravity effects into existing stability analysis.
Findings
Stability condition is affected by gravitation via equilibrium values.
Extension of previous stability criteria to include self-gravitation.
Gravity influences plasma stability through equilibrium parameters.
Abstract
A previous stability condition (see Throumoulopoulos and Tasso, Physics of Plasmas 14, 122104 (2007)) for incompressible plasmas with field aligned flows is extended to gravitating plasmas including self-gravitation. It turns out that the stability condition is affected by gravitation through the equilibrium values only.
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Fluid Dynamics and Turbulent Flows
