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Astrophysics and Space Science

, Volume 86, Issue 1, pp 209–213 | Cite as

On the screening of the interstellar electric and magnetic fields by the solar wind

  • I. S. Veselovsky
Article

Abstract

Fast-streaming solar-wind plasma with high conductivity screens the heliosphere from the penetration of the interstellar electric and magnetic fields. The simplest model with the constant solar wind conductivity and radial velocity is considered and the boundary electrodynamic problem is solved for static external fields. The results show that screening of the external fields takes place in the heliosphere according to the exponential law.

Keywords

Magnetic Field Simple Model Solar Wind Radial Velocity External Field 
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. Alexeev, I. I., Kropotkin, A. P., and Veselovsky, I. S.: 1982,Solar Phys. 79, 385.Google Scholar
  2. Axford, W. I.: 1972, inSolar Wind, NASA SP-308, p. 609.Google Scholar
  3. Baranov, W. B. and Krasnobaev, K. W.: 1977,Hydrodynamic Theory of Cosmic Plasma, Nauka, Moscow (in Russian).Google Scholar
  4. Parker, E. N.: 1963,Interplanetary Dynamical Processes, Interscience Publ., New-York, London.Google Scholar
  5. Veselovsky, I. S.: 1974,Solar Wind, ‘Itogy Nauki i Techniki’, Issledovanie kosmiczeskogo prostranstva, Vol. 4, Moscow (in Russian).Google Scholar

Copyright information

© D. Reidel Publishing Co 1982

Authors and Affiliations

  • I. S. Veselovsky
    • 1
  1. 1.Institute of Nuclear PhysicsMoscow State UniversityMoscowU.S.S.R.

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