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The structure of the global solar magnetic field excited by the turbulent dynamo mechanism

โœ Scribed by V. N. Krivodubskii


Book ID
110127833
Publisher
Springer
Year
2001
Tongue
English
Weight
111 KB
Volume
45
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