General solution of a fractional diffusion–advection equation for solar cosmic-ray transport
In this effort we exactly solve the fractional diffusion–advection equation for solar cosmic-ray transport and give its general solution in terms of hypergeometric distributions. Numerical analysis of this equation shows that its solutions resemble power-laws.
| Autores: | , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2016 |
| País: | Argentina |
| Institución: | Universidad Nacional de La Plata |
| Repositorio: | SEDICI (UNLP) |
| Idioma: | inglés |
| OAI Identifier: | oai:sedici.unlp.edu.ar:10915/130639 |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/130639 |
| Access Level: | acceso abierto |
| Palabra clave: | Ciencias Exactas Física Distributions Cosmic rays Diffusion Sun Heliosphere |
| Sumario: | In this effort we exactly solve the fractional diffusion–advection equation for solar cosmic-ray transport and give its general solution in terms of hypergeometric distributions. Numerical analysis of this equation shows that its solutions resemble power-laws. |
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