Energetic Solar Particles in the Interplanetary Medium

Axford, W. I.

doi:10.1007/978-94-009-3693-5_19

W. I. Axford^1,2

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 29))

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Abstract

Models which describe the diffusion of energetic solar particles in the interplanetary medium are reviewed. Most attention is paid to the case of impulsive emission from solar flares, taking into account the effects of the interplanetary magnetic field, diffusion near the Sun, convection, and energy losses associated with the expansion of the solar wind. The case of continuous emission is also considered briefly.

This work was supported by the National Aeronautics and Space Administration under Contract NGR-05-009-081.

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Dept. of Physics, University of Calif., San Diego, La Jolla, Calif., 92037, USA
W. I. Axford
Dept. of Applied Physics and Information Science, University of Calif, San Diego, La Jolla, Calif, 92037, USA
W. I. Axford

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E. R. Dyer

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Axford, W.I. (1972). Energetic Solar Particles in the Interplanetary Medium. In: Dyer, E.R. (eds) Solar-Terrestrial Physics/1970. Astrophysics and Space Science Library, vol 29. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3693-5_19

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DOI: https://doi.org/10.1007/978-94-009-3693-5_19
Published: 03 September 2011
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8154-2
Online ISBN: 978-94-009-3693-5
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