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Cosmic Ray Nonlinear Effects in Space Plasma, 2. Dynamic Heliosphere

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Currents in High-Energy Astrophysics

Part of the book series: NATO ASI Series ((ASIC,volume 458))

Abstract

Effects of cosmic ray pressure on solar wind and interplanetary shock waves propagation and effects of kinetic stream instability of non isotropic cosmic ray fluxes on the magnetic structure of plasma in the Heliosphere are considered. These effects are important in the outer Heliosphere, where the cosmic ray pressure become comparable with dynamical pressure of solar wind and shock waves.

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Author information

Authors and Affiliations

  1. Cosmic Ray Dept. of IZMIRAN, Troitsk, Moscow, 142092, Russia

    L. I. Dorman

  2. Cosmic Ray Res. Center of MIGAL, Qazrin, 12900, POB 3593, Israel

    L. I. Dorman

Authors
  1. L. I. Dorman
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Editor information

Editors and Affiliations

  1. Department of Physics and Astronomy, University of Maryland, College Park, MD, USA

    Maurice M. Shapiro

  2. Universities Space Research Association, Washington, DC, USA

    Rein Silberberg

  3. Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA, USA

    John P. Wefel

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© 1995 Springer Science+Business Media Dordrecht

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Dorman, L.I. (1995). Cosmic Ray Nonlinear Effects in Space Plasma, 2. Dynamic Heliosphere. In: Shapiro, M.M., Silberberg, R., Wefel, J.P. (eds) Currents in High-Energy Astrophysics. NATO ASI Series, vol 458. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0253-7_16

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  • DOI: https://doi.org/10.1007/978-94-011-0253-7_16

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4112-6

  • Online ISBN: 978-94-011-0253-7

  • eBook Packages: Springer Book Archive

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