Article contents
A time-dependent model of magnetic field annihilation
Published online by Cambridge University Press: 13 March 2009
Abstract
Quasi-periodic variations in the electric field intensity near the dayside magnetopause are studied within a planar, dissipative MHD model of a stagnation-line flow embedded in a rectilinear magnetic field. The model is based on an exact time-dependent solution of the resistive MHD equations applied to a Parker-type diffusion region of field-line merging. The results lead to the prediction of certain relations between physical parameters of the solar- wind plasma, and these are compared with actual measurements.
- Type
- Research Article
- Information
- Copyright
- Copyright © Cambridge University Press 1993
References
REFERENCES
- 3
- Cited by