Turbulence Curr Sheet Shocks C
Book Details
Format
Hardback or Cased Book
ISBN-10
2881248772
ISBN-13
9782881248771
Publisher
Gordon & Breach Science Publishers SA
Imprint
Gordon & Breach Science Publishers SA
Country of Manufacture
GB
Country of Publication
GB
Publication Date
Oct 18th, 1993
Print length
398 Pages
Weight
738 grams
Product Classification:
Materials / States of matter Astrophysics
Ksh 33,300.00
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Solar activity, solar and stellar winds, accretion, turbulent regions in cosmic plasmas, particle acceleration and the formation of high-energy nonthermal components (cosmic rays), are processes characteristic of cosmic plasmas that involve fast energy transformations and nonstationary conditions.
Solar activity, solar and stellar winds, accretion, turbulent regions in cosmic plasmas, particle acceleration, and the formation of high-energy nonthermal components (cosmic rays), are processes characteristic of cosmic plasmas that involve fast energy transformations and nonstationary conditions. They all are generated, however, by the same physical mechanisms for the storage, release, and propagation of energy. It is the relation between such mechanisms and their macroscopic manifestation that Russian scientists address, in a manner suitable to graduate students and scientists in cosmic electrodynamics.
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