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Characteristics of oscillatory-wave processes in solar structures with various magnetic field topology

โœ Scribed by N. I. Kobanov; D. Yu. Kolobov; A. A. Sklyar; S. A. Chupin; V. A. Pulyaev


Book ID
111436794
Publisher
Springer
Year
2009
Tongue
English
Weight
590 KB
Volume
53
Category
Article
ISSN
1063-7729

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The structure of the turbulent shock wav
โœ V. V. Zaitsev; O. G. Parfenov; A. V. Stepanov ๐Ÿ“‚ Article ๐Ÿ“… 1978 ๐Ÿ› Springer ๐ŸŒ English โš– 625 KB

A consistent account of plasma turbulence in magnetohydrodynamics equation s describing transport processes across the magnetic field is presented. The structure of the perpendicular shock wave generated in the solar atmosphere, as a result of either local disturbance of the magnetic field or dense