Parker Problem in Hall Magnetohydrodynamics
Space Physics
2015-05-13 v1
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 ) than that (like \normalfont) in the outer ideal MHD region.
Cite
@article{arxiv.0801.4745,
title = {Parker Problem in Hall Magnetohydrodynamics},
author = {Bhimsen K. Shivamoggi},
journal= {arXiv preprint arXiv:0801.4745},
year = {2015}
}