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SELF-SIMILAR SOLUTIONS FOR THE ACCELERATION OF COSMIC RAYS AT A SUPERNOVA SHOCK PROPAGATING INTO A CIRCUMSTELLAR WIND

    https://doi.org/10.1142/S0218271808013418Cited by:0 (Source: Crossref)
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    Abstract

    Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind. Self-similar solutions for the cosmic ray distribution are derived firstly when diffusion is isotropic and secondly when the wind sustains a magnetic field in the form of a Parker spiral.

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