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- Catto, Peter J.Massachusetts Institute of Technology (MIT) (author)
Three-dimensional magnetized and rotating hot plasma equilibrium and stability in a gravitational field
- Article/chapterEnglish2015
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- 2015
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- LIBRIS-ID:oai:research.chalmers.se:a0bf6ba8-6f19-480a-9085-8b892b18d6b2
- ISBN:2914771983
- https://research.chalmers.se/publication/220531URI
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- Language:English
- Summary in:English
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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 and genre
- 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
- Grad-Shafranov equation
- plasma equilibrium
- accretion disk
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- Krasheninnikov, Sergei I.University of California (author)
- Pusztai, Istvan,1983Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)pusztai (author)
- Massachusetts Institute of Technology (MIT)University of California (creator_code:org_t)
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- In:Europhysics Conference Abstracts39E, s. O2.401-2914771983
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