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Capillary instability of a rotating jet with twisted magnetic field

Published online by Cambridge University Press:  28 March 2006

Pratibha Verma
Affiliation:
Department of Physics and Astrophysics, University of Delhi, Delhi-6, India
Y. K. Verma
Affiliation:
Department of Physics and Astrophysics, University of Delhi, Delhi-6, India

Abstract

The stability of a uniformly rotating and infinitely conducting jet with twisted magnetic field is discussed. The dispersion relation is obtained for the non-axisymmetric perturbations; this involves a complex and implicit function of the growth rate. The complex growth rate implies that instability develops as an overstability. The effect of axial current is destabilizing for both the instabilities m = 0 and m = 1 discussed here. The effect of rotation on the stability of the jet is as follows: (a) for the m = 0 mode, rotation always has a destabilizing effect; (b) for the m = 1 mode, rotation has a stabilizing effect for very long-wave perturbations, but for short-wave perturbations it destabilizes the jet. In particular there exists a disturbance of a particular wavelength which is unaffected by the rotation of the jet.

Type
Research Article
Copyright
© 1965 Cambridge University Press

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References

Chandrasekhar, S. 1961 Hydrodynamic and hydromagnetic stability. Oxford University Press.
Dattner, A., Lehnert, B. & Lundquist, S. 1958 2nd U. Geneva Conf. (Sweden), 325.
Gupta, A. S. 1964 Proc. Roy. Soc. A, 278, 214.
Murty, G. S. 1960 Ark. Fys. 18, 24.
Nayyar, N. K. & Trehan, S. K. 1963 Phys. Fluids 6, 1587.
Rayleigh, Lord 1899 Sci. Pap. 1, 361.
Tayler, R. J. 1960 Rev. Mod. Phys. 32, 907.