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Turbulence and Waves in the Solar Wind Formation Region and the Heliosphere

  • Igor Veselovsky
Conference paper

Abstract

A short review is presented of the dissipative and radiative MHD, electromagnetic and plasma kinetic scaling approaches which are useful for sorting out different physical processes according to their relative importance. The ‘velocity-emission’ ratio Ve, the Faraday number F and ‘Trieste numbers’ T are described together with more familiar dimensionless parameters. The concepts of the turbosphere and turbopause around the Sun are outlined.

Keywords

Solar Wind Strouhal Number Heliocentric Distance Quiescent Prominence Solar Wind Acceleration 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Veselovsky, I.S.: 1996, Nearly sonic and supersonic convective motions in the solar wind formation region, in: D. Winterhalter et al. (eds.), Solar Wind Eight, pp. 161–164. AIP, Woodbury, New York.Google Scholar
  2. Veselovsky, LS.: 1998, Turbosphere and turbopause in the solar wind formation region, in: S.R. Habbal et al. (eds.), Solar Wind Nine, pp. 381–384. AIP 382, Woodbury, New York.Google Scholar
  3. Veselovsky, I.S.: 1999, Scaling Approach in the Solar and Heliospheric Plasma, The Abdus Salam International Centre for Theoretical Physics. SMR 1161/10, Trieste, Italy.Google Scholar

Copyright information

© Springer Science+Business Media New York 2001

Authors and Affiliations

  • Igor Veselovsky
    • 1
  1. 1.Institute of Nuclear PhysicsMoscow State UniversityMoscowRussia

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