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A Three Dimensional Magnetohydrodynamic Pulse in a Transversely Inhomogeneous Medium

  • D. Tsiklauri
  • , V. M. Nakariakov

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Interaction of impulsively generated MHD waves with a one-dimensional plasma inhomogeneity, transverse to the magnetic field, is considered in the three-dimensional regime. Because of the transverse inhomogeneity, MHD fluctuations, even if they do not include initially any density perturbation, evolve toward states where the compressible components tend to become predominant. The propagating MHD pulse asymptotically reaches a quasi-steady state with the final levels of density perturbation weakly depending on the degree of non-planeness of the pulse in the homogeneous transverse direction and somewhat stronger depending on plasma β. Our study demonstrates the necessity of incorporation of compressible and 3D effects in theory of Alfvén wave phase mixing. However, as far as the dynamics of weakly non-plane Alfvén waves is concerned it can still be qualitatively understood in terms of the previous 2.5D models.

Original languageEnglish
Title of host publicationSolar Wind Ten
Subtitle of host publicationProceedings of the 10th International Solar Wind Conference
EditorsMarco Velli, Roberto Bruno, Francesco Malara
PublisherAmerican Institute of Physics Inc.
Pages570-573
Number of pages4
ISBN (Electronic)0735401489
DOIs
Publication statusPublished - 2 Sept 2003
Event10th International Solar Wind Conference - Pisa, Italy
Duration: 17 Jun 200221 Jun 2002

Publication series

NameAIP Conference Proceedings
Volume679
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

Conference10th International Solar Wind Conference
Country/TerritoryItaly
CityPisa
Period17/06/0221/06/02

Bibliographical note

Publisher Copyright:
© 2003 American Institute of Physics.

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