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Influence of interplanetary shocks on solar particle events (1977)

Morfill, G. E. ; Scholer, M.

Springer

Astrophysics and space science 46 (1977), S. 73-86

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ISSN: 1572-946X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract Energetic particles, ejected from the Sun during solar flare events, may encounter interplanetary plasma/field conditions, which deviate considerably from the quiet time values used normally to describe the particle propagation. This is due to the presence of a hydromagnetic shock, which is emitted from the Sun at the time of the explosion. In a theoretical blast wave model, which incorporates the interaction with plane polarized Alfvén waves, we have analysed the changes in different terms of the Fokker-Planck equation, which describes energetic particle propagation. In this treatment, the shock influence on energy changes and on the transport coefficients are discussed.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00643755

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