Abstract
The method of the numerical solution of the time and rigidity dependent three dimensional (3-D) second order partial differential equation describing the anisotropic diffusion of the galactic cosmic ray particles in the heliosphere is proposed. A good agreement between the results of the numerical solution and experimental data is demonstrated. The proposed numerical method gives a broad possibility for implementation of the parallel programming techniques, and could be successfully used to solve second order partial differential equations, among them equations describing different classes of galactic cosmic ray intensity variations observed due to anisotropic diffusion of the galactic cosmic ray particles in the heliosphere.
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Wawrzynczak, A., Alania, M.V. (2010). Numerical Solution of the Time and Rigidity Dependent Three Dimensional Second Order Partial Differential Equation. In: Wyrzykowski, R., Dongarra, J., Karczewski, K., Wasniewski, J. (eds) Parallel Processing and Applied Mathematics. PPAM 2009. Lecture Notes in Computer Science, vol 6067. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-14390-8_12
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DOI: https://doi.org/10.1007/978-3-642-14390-8_12
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