Skip to main content
Log in

Effect of viscosity on the propagation of nonlinear Alfvén waves along a tangential magnetohydrodynamic discontinuity in an incompressible fluid

  • Published:
Fluid Dynamics Aims and scope Submit manuscript

Abstract

It is proposed to consider the propagation of surface waves along a tangential magnetohydrodynamic discontinuity in the particular case where the fluid velocities on both sides of the interface are equal to zero. In [1] it was shown that waves called surface Alfvén waves may be propagated along the surface separating a semi-infinite region without a field from a region with a uniform magnetic field. The linear theory of surface Alfvén waves in a compressible medium was considered in [2]. In [3] the damping of surface Alfvén waves as a result of viscosity and heat conduction was investigated. The propagation of low-amplitude nonlinear surface Alfvén waves in an incompressible fluid in the absence of dissipative processes is described by the integrodifferential equation obtained in [4]. By means of a numerical solution of this equation it was shown that a perturbation initially in the form of a sinusoidal wave will break. The breaking time was determined. In this paper the equation derived in [4] is extended to the case of a viscous fluid. It is shown that the equation obtained does not have steady-state solutions. The propagation of periodic disturbances is investigated numerically.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

We’re sorry, something doesn't seem to be working properly.

Please try refreshing the page. If that doesn't work, please contact support so we can address the problem.

Literature cited

  1. E. N. Parker, “The nature of the sunspot phenomenon. II. Internal overstable modes,” Sol. Phys.,32, 127 (1974).

    Article  ADS  Google Scholar 

  2. B. Roberts, “Wave propagation in a magnetically structured atmosphere. I. Surface waves at a magnetic interface,” Sol. Phys.,69, 27 (1981).

    Article  ADS  Google Scholar 

  3. B. E. Gordon and J. V. Hollweg, “Collisional damping of surface waves in the solar corona,” Astrophys. J.,266, 373 (1983).

    Article  ADS  Google Scholar 

  4. M. S. Ruderman, “Propagation of nonlinear Alfvén surface waves along a tangential magnetohydrodynamic discontinuity in an incompressible fluid,” Izv. Akad. Nauk SSSR, Mekh. Zhidk. Gaza, No. 1, 98 (1985).

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Additional information

Translated from Izvestiya Akademii Nauk SSSR, Mekhanika Zhidkosti i Gaza, No. 6, pp. 94–104, November–December, 1986.

The author wishes to thank L. S. Fedorov for assisting with the calculations.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Ruderman, M.S. Effect of viscosity on the propagation of nonlinear Alfvén waves along a tangential magnetohydrodynamic discontinuity in an incompressible fluid. Fluid Dyn 21, 925–934 (1986). https://doi.org/10.1007/BF02628029

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02628029

Keywords

Navigation