Volume 395, Number 1, November III 2002
|Page(s)||285 - 292|
|Section||Planets and planetary systems|
|Published online||29 October 2002|
A strongly nonlinear Alfvénic pulse in a transversely inhomogeneous medium
Physics Department, University of Warwick, Coventry, CV4 7AL, England, UK
Corresponding author: D. Tsiklauri, firstname.lastname@example.org
Accepted: 30 August 2002
We investigate the interaction of a plane, linearly polarized, Alfvénic pulse with a one-dimensional, perpendicular to the magnetic field, plasma density inhomogeneity in the strongly nonlinear regime. Our numerical study of the full MHD equations shows that: (i) Plasma density inhomogeneity substantially enhances (by about a factor of 2) the generation of longitudinal compressive waves. (ii) Attained maximal values of the generated transverse compressive perturbations are insensitive to the strength of the plasma density inhomogeneity, plasma β and the initial amplitude of the Alfvén wave. Typically, they reach about 40% of the initial Alfvén wave amplitude. (iii) Attained maximal values of the generated relative density perturbations are within 20–40% for . They depend upon plasma β strongly; and scale almost linearly with the initial Alfvén wave amplitude.
Key words: magnetohydrodynamics (MHD) / waves / Sun: activity / Sun: solar wind
© ESO, 2002
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