Parker Problem in Hall Magnetohydrodynamics

Abstract

Parker problem in Hall magnetohydrodynamics (MHD) is considered. Poloidal shear into the toroidal flow generated by the Hall effect is incorporated. This is found to lead to a {\it triple deck} structure for the Parker problem in Hall MHD, with the magnetic field falling off in the intermediate Hall-resistive region more steeply (like \normalfont $1/x^3$) than that (like \normalfont$1/x$) in the outer ideal MHD region.

References in corpus (2)

• Steady Hall Magnetohydrodynamics Near a X-type Magnetic Neutral Line
• Hall Resistive Tearing Mode: A Variational Formulation

Cited by in corpus (1)

• Hall MHD waves: A fundamental departure from their MHD counterparts