Energetic solar particle events in a str
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M. Scholer; G. Morfill; A. K. Richter
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Article
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1979
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Springer
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English
β 517 KB
Theoretical considerations lead to a solar cosmic ray diffusion coefficient which varies with heliolongitude in a stream-structured solar wind. By solving numerically the time dependent convectiondiffusion equation for the particle transport we investigate the effect of the azimuthal variation of th