Hall-MHD Surface Waves in Flowing Solar-Wind Plasma Slab
Abstract
We study the influence of a steady flow velocity on the dispersion characteristics of Hall- magnetohydrodynamic forward and backward sausage and kink surface waves travelling along a solar-wind plasma slab. Both surface modes, being Alfven waves in an immovable layer, become super Alvenic ones in flowing slab will increased dispersion at small wave numbers for forward waves and at large wave numbers for backward waves, respectively.
Document Details
- Document Type
- Technical Report
- Publication Date
- Jul 20, 2003
- Accession Number
- ADP014999
Entities
People
- I. Zhelyazkov
- R. Miteva
Organizations
- Sofia University