Improved stability condition for rotating plasmas

Eliezer Hameiri, Hanno A. Holties

Research output: Contribution to journalArticle

Abstract

It is shown that the conservation of flow circulation along magnetic field lines can be used to improve on the δW stability criterion for rotating plasmas by adding to the energy integral a positive definite term. The improvement is most effective for ballooning modes in systems with a closed-line magnetic field. Such systems are investigated, both when the flow is sheared and when it is unsheared. In the unsheared case, instabilities grow exponentially in time, while, if the flow is sheared, an instability eventually saturates. The time-asymptotic behavior of such solutions is obtained and is different from the asymptotic behavior when the magnetic field is sheared.

Original languageEnglish (US)
Pages (from-to)3807-3813
Number of pages7
JournalPhysics of Plasmas
Volume1
Issue number12
StatePublished - 1994

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rotating plasmas
magnetic fields
ballooning modes
conservation
energy

ASJC Scopus subject areas

  • Physics and Astronomy(all)
  • Condensed Matter Physics

Cite this

Hameiri, E., & Holties, H. A. (1994). Improved stability condition for rotating plasmas. Physics of Plasmas, 1(12), 3807-3813.

Improved stability condition for rotating plasmas. / Hameiri, Eliezer; Holties, Hanno A.

In: Physics of Plasmas, Vol. 1, No. 12, 1994, p. 3807-3813.

Research output: Contribution to journalArticle

Hameiri, E & Holties, HA 1994, 'Improved stability condition for rotating plasmas', Physics of Plasmas, vol. 1, no. 12, pp. 3807-3813.
Hameiri E, Holties HA. Improved stability condition for rotating plasmas. Physics of Plasmas. 1994;1(12):3807-3813.
Hameiri, Eliezer ; Holties, Hanno A. / Improved stability condition for rotating plasmas. In: Physics of Plasmas. 1994 ; Vol. 1, No. 12. pp. 3807-3813.
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