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Three-dimensional magnetized and rotating hot plasma equilibrium and stability in a gravitational field

Catto, Peter J. (author)
Massachusetts Institute of Technology (MIT)
Krasheninnikov, Sergei I. (author)
University of California
Pusztai, Istvan, 1983 (author)
Chalmers tekniska högskola,Chalmers University of Technology
 (creator_code:org_t)
ISBN 2914771983
2015
2015
English.
In: Europhysics Conference Abstracts. - 2914771983 ; 39E, s. O2.401-
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • We present analytic solutions for three-dimensional magnetized axisymmetric equilibria confining rotating hot plasma in a gravitational field. Our solution to the full Grad-Shafranov equation can exhibit strong equatorial plane localization of the plasma density and current, resulting in disk equilibria for the plasma density. Unlike in [P.J. Catto et al, 2015, J. Plasma Physics 81, 105810301], we find a toriodal magnetic field is necessary to find a equilibrium in the presence of gravity for most cases of interest. We expect our results to provide impetus to re-investigate magneto-rotational stability.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

Grad-Shafranov equation
plasma equilibrium
accretion disk

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