Finite-\(\beta\) effects on the radiative thermal instability in magnetized plasmas. (English) Zbl 0678.76037
Summary: The radiative thermal instability is investigated taking into account finite-\(\beta\), or electromagnetic, effects. The two-fluid model for magnetized plasmas together with the Maxwell equations are used to derive a general dispersion relation valid for compressional perturbations with frequency below the electron-cyclotron frequency. The growth rates of the radiative thermal instabilities involving fast magnetosonic flute-like and low-frequency hydromagnetic perturbations are presented.
MSC:
76E25 | Stability and instability of magnetohydrodynamic and electrohydrodynamic flows |
76X05 | Ionized gas flow in electromagnetic fields; plasmic flow |
Keywords:
radiative thermal instability; two-fluid model; magnetized plasmas; Maxwell equations; electron-cyclotron frequency; radiative thermal instabilities; fast magnetosonic flute-like and low-frequency hydromagnetic perturbationsReferences:
[1] | Braginskii, S. I.: 1965,Reviews of Plasma Physics, Vol. 1, Consultants Bureau, New York, p. 205. |
[2] | Drake, J. F., Sparks, L., and Van Hoven, G.: 1988,Phys. Fluids 31, 813. · Zbl 0644.76061 · doi:10.1063/1.866817 |
[3] | Field, G. B.: 1965,Astrophys. J. 142, 531. · doi:10.1086/148317 |
[4] | Lipschultz, B.: 1987,J. Nucl. Mat. 145-147, 15. · doi:10.1016/0022-3115(87)90306-0 |
[5] | Lipschultz, B., LaBombard, B., Marmar, E. S., Pickrell, M. M., Terry, J. L., Watterson, R., and Wolfe, S. M.: 1984,Nucl. Fusion 24, 977. · doi:10.1088/0029-5515/24/8/002 |
[6] | Parker, E. N.: 1953,Astrophys. J. 117, 431. · doi:10.1086/145707 |
[7] | Sakai, J., Colin, A., and Priest, E.: 1987,Solar Phys. 114, 253. · doi:10.1007/BF00167345 |
[8] | Stenflo, L., Yu, M. Y., and Shukla, P. K.: 1986,J. Plasma Phys. 36, 447. · Zbl 0601.76130 · doi:10.1017/S0022377800011892 |
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.