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m=1 ideal kink modes in a line-tied screw pinch with finite plasma pressure

Phys. Plasmas 15, 092106 (2008); doi:10.1063/1.2977985

Published 11 September 2008

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V. A. Svidzinski,1 V. V. Mirnov,2 and H. Li1
1Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
2Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA

A new method for computing ideal magnetohydrodynamic linear eigenmodes in a cylindrical screw pinch with line-tying boundary conditions at the axial ends is presented. In this method, plasma volume is reflected over one of the end planes, and equations and field components are continued into the extended volume with the continuation rules prescribed by the line-tying boundary conditions. Field components in the combined volume are expanded in Fourier series in the axial coordinate. The resulting set of coupled differential equations is solved numerically in the radial coordinate by a finite difference method yielding growth rates and eigenmodes for the system. An example of an m=1 (m is the poloidal wave number) internal kink instability in a force-free plasma equilibrium with uniform pressure is considered. In contrast to a periodic screw pinch, marginally stable perturbations are essentially compressible in the line-tied geometry. Finite compressibility makes the mode more stable in addition to the usual line-tying stabilization in zero pressure plasma. The critical length corresponding to the marginal stability increases with the increase of plasma beta. A universal axial dependence for marginally stable density perturbations rho(r,z)=rho(r)exp[−izµ(r)] is predicted analytically and confirmed numerically, where µ(r) depends on the equilibrium magnetic field components as µ(r)=[overline B]theta/r[overline B]z. ©2008 American Institute of Physics
History: Received 2 June 2008; accepted 12 August 2008; published 11 September 2008
Permalink: http://link.aip.org/link/?PHPAEN/15/092106/1
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KEYWORDS and PACS

Keywords
PACS
  • 52.35.Py
    Plasma macroinstabilities (hydromagnetic)
  • 52.58.Lq
    Z-pinches, plasma focus and other pinch devices
  • 52.30.Cv
    Plasma magnetohydrodynamics
  • 52.65.-y
    Plasma simulation
  • 02.30.Jr
    Partial differential equations
  • 02.10.Ud
    Linear algebra
  • YEAR: 2008

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ISSN:
1070-664X (print)   1089-7674 (online)
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REFERENCES (34)

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  1. V. D. Shafranov, Sov. Phys. Tech. Phys. 15, 175 (1970).
  2. M. N. Rosenbluth, R. Y. Dagazian, and P. H. Rutherford, Phys. Fluids 16, 1984 (1973).
  3. E. N. Parker, Astrophys. J. 174, 499 (1972).
  4. Z. Mikić, D. D. Schnack, and G. Van Hoven, Astrophys. J. 338, 1148 (1989).
  5. K. Galsgaard and A. Nordlund, J. Geophys. Res. 101, 13445, DOI: 10.1029/96JA00428 (1996).
  6. A. W. Longbottom, G. J. Rickard, I. J. D. Craig, and A. D. Sneyd, Astrophys. J. 500, 471 (1998).
  7. C. S. Ng and A. Bhattacharjee, Phys. Plasmas 5, 4028 (1998).
  8. M. A. Raadu, Sol. Phys. 22, 425 (1972).
  9. A. W. Hood and E. P. Priest, Geophys. Astrophys. Fluid Dyn. 17, 297 (1981).
  10. G. Einaudi and G. Van Hoven, Sol. Phys. 88, 163 (1983).
  11. L. S. Solov'ev, At. Energ. 30, 14 (1971).
  12. M. Velli, G. Einaudi, and A. W. Hood, Astrophys. J. 350, 428 (1990).
  13. R. A. M. Van der Linden, M. Goosens, and W. Kerner, Comput. Phys. Commun. 59, 61 (1990).
  14. R. A. M. Van der Linden and A. W. Hood, Astron. Astrophys. 339, 887 (1998).
  15. H. Baty, G. Einaudi, R. Lionello, and M. Velli, Astron. Astrophys. 333, 131 (1998).
  16. R. Lionello, D. D. Schnack, and G. Einaudi, and M. Velli, Phys. Plasmas 5, 3722 (1998).
  17. J. P. Goedbloed and G. Halberstadt, Astron. Astrophys. 286, 275 (1994).
  18. C. C. Hegna, Phys. Plasmas 11, 4230 (2004).
  19. D. D. Ryutov, R. H. Cohen, and L. D. Pearlstein, Phys. Plasmas 11, 4740 (2004).
  20. Y. Huang, E. G. Zweibel, and C. R. Sovinec, Phys. Plasmas 13, 092102 (2006).
  21. E. G. Evstatiev, G. L. Delzanno, and J. M. Finn, Phys. Plasmas 13, 072902 (2006).
  22. G. L. Delzanno, E. G. Evstatiev, and J. M. Finn, Phys. Plasmas 14, 070702 (2007).
  23. G. L. Delzanno, E. G. Evstatiev, and J. M. Finn, Phys. Plasmas 14, 092901 (2007).
  24. G. L. Delzanno and J. M. Finn, Phys. Plasmas 15, 032904 (2008).
  25. W. F. Bergerson, C. B. Forest, G. Fiksel, D. A. Hannum, R. Kendrick, J. S. Sarff, and S. Stambler, Phys. Rev. Lett. 96, 015004 (2006).
  26. I. Furno, T. P. Intrator, D. D. Ryutov, S. Abbate, T. Madziwa-Nussinov, A. Light, L. Dorf, and G. Lapenta, Phys. Rev. Lett. 97, 015002 (2006).
  27. D. D. Ryutov, I. Furno, T. P. Intrator, S. Abbate, and T. Madziwa-Nussinov, Phys. Plasmas 13, 032105 (2006).
  28. J. P. Freidberg, Ideal Magnetohydrodynamics (Plenum, New York, 1987).
  29. A. N. Kondratenko, Sov. Phys. Tech. Phys. 11, 590 (1965).
  30. Z. Mikić, D. D. Schnack, and G. Van Hoven, Astrophys. J. 361, 690 (1990).
  31. A. D. Sneyd and I. J. D. Craig, Astrophys. Space Sci. 151, 265 (1989).
  32. V. A. Svidzinski and H. Li, Phys. Plasmas 15, 052106 (2008).
  33. A. B. Mikhailovskii, Instabilities in a Confined Plasma (Institute of Physics, Bristol, 1998).
  34. A. A. Ware, Phys. Rev. Lett. 12, 439 (1964).

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