Abstract
When subjected to a strong magnetic field, plasmas can exhibit anisotropy in the directions parallel and perpendicular to the field. The magnetohydrodynamics (MHD) equilibrium equation under the hypothesis of Chew, Goldberger, and Low of an anisotropic pressure tensor is solved analytically, using a previously known solution of the isotropic case in oblate spheroidal coordinates. The effects of the anisotropy on the magnetic fields and on the current density are investigated, and the radial profiles of the pressures along and across the magnetic field are studied.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
