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Propagation model of high-energy solar cosmic rays in interplanetary space and Green function

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Based on main observational characteristics of solar flare particle transport in the coronal, a mathematical description of coronal transport is proposed. A model is presented for solar cosmic-ray propagation in solar-terrestrial space of infinite, homogeneous orthotropic medium. A Green function to the propagation equation with source is found. The integral solution to the propagation equation with the source, as well as the analytical solution to the equation for a pulse point source, is obtained by using the Green function in the medium.

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Authors and Affiliations

  1. Center for Space Science and Applied Research, Chinese Academy of Sciences, 100080, Beijing, China

    Yongnian Huang, Zhidan Wang & Yongli Wang

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  1. Yongnian Huang
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  2. Zhidan Wang
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  3. Yongli Wang
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Huang, Y., Wang, Z. & Wang, Y. Propagation model of high-energy solar cosmic rays in interplanetary space and Green function. Sci. China Ser. A-Math. 41, 1197–1205 (1998). https://doi.org/10.1007/BF02871982

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  • DOI: https://doi.org/10.1007/BF02871982

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