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Cosmic Ray Nonlinear Processes In Space Plasma: Applications To The Dynamic Heliosphere

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Plasma Astrophysics And Space Physics

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Abstract

Influence of cosmic ray pressure and kinetic stream instability on space plasma dynamics and magnetic structure are considered. It is shown that in the outer Heliosphere are important dynamics effects of galactic cosmic ray pressure on solar wind and interplanetary shock wave propagation as well as on the formation of terminal shock wave of the Heliosphere and subsonic region between Heliosphere and interstellar medium. Kinetic stream instability effects are important on distances more than 40–60 AU from the Sun: formation of great anisotropy of galactic cosmic rays in about spiral interplanetary magnetic field leads to the Alfven turbulence generation by non isotropic cosmic ray fluxes. Generated Alfven turbulence influences on cosmic ray propagation, increases the cosmic ray modulation, decreases the cosmic ray anisotropy and increases the cosmic ray pressure gradient in the outer Heliosphere (the later is also important for terminal shock wave formation).

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Authors and Affiliations

  1. IZMIRAN, Technion and Israel Cosmic Ray Center, Affiliated to Tel Aviv University, POB 2217, Qazrin, 12900, Israel

    Lev I. Dorman

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  1. Lev I. Dorman
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Editor information

Editors and Affiliations

  1. Max Planck Institute für Aeronomie, Lindau, Germany

    Jörg Büchner , Ian Axford , Eckart Marsch  & Vytenis Vasyliūnas , ,  & 

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© 1999 Springer Science+Business Media Dordrecht

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Dorman, L.I. (1999). Cosmic Ray Nonlinear Processes In Space Plasma: Applications To The Dynamic Heliosphere. In: Büchner, J., Axford, I., Marsch, E., Vasyliūnas, V. (eds) Plasma Astrophysics And Space Physics. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4203-8_34

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  • DOI: https://doi.org/10.1007/978-94-011-4203-8_34

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5828-5

  • Online ISBN: 978-94-011-4203-8

  • eBook Packages: Springer Book Archive

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