B F McMillan et al 2004 Plasma Phys. Control. Fusion 46 1027 doi:10.1088/0741-3335/46/7/003
B F McMillan1, R L Dewar1 and R G Storer2
Show affiliationsThe constraint of incompressibility is often used to simplify the magnetohydrodynamic (MHD) description of linearized plasma dynamics because it does not affect the ideal MHD marginal stability point. In this paper two methods for introducing incompressibility are compared in a cylindrical plasma model: in the first method, the limit γ → ∞ is taken, where γ is the ratio of specific heats; in the second, an anisotropic mass tensor ρ is used, with the component parallel to the magnetic field taken to vanish, ρ
→ 0. Use of resistive MHD reveals the nature of these two limits because the Alfvén and slow magnetosonic continua of ideal MHD are converted to point spectra and moved into the complex plane. Both limits profoundly change the slow magnetosonic spectrum, but only the second limit faithfully reproduces the resistive Alfvén spectrum and its wavemodes. In ideal MHD, the slow magnetosonic continuum degenerates to the Alfvén continuum in the first method, while it is moved to infinity by the second. The degeneracy in the first is broken by finite resistivity. For numerical and semi-analytical study of these models, we choose plasma equilibria which cast light on puzzling aspects of results found in earlier literature.
52.30.Cv Magnetohydrodynamics (including electron magnetohydrodynamics)
52.55.Tn Ideal and resistive MHD modes; kinetic modes
52.35.Bj Magnetohydrodynamic waves (e.g., Alfven waves)
52.25.Os Emission, absorption, and scattering of electromagnetic radiation
Issue 7 (July 2004)
Received 1 April 2004
Published 24 May 2004
B F McMillan et al 2004 Plasma Phys. Control. Fusion 46 1027
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