Speaker
Viacheslav Mykhailenko
(Pavol Jozef Safarik University in Kosice)
Description
The propagation of cosmic rays through the heliosphere is solved for more than half a century by stochastic methods based on Ito's lemma. This work presents the estimation of statistical error of solution of Foker – Plank equation by 1D forward stochastic differential equations method.
The error dependence on simulation statistics and energy is presented for different combinations of input parameters. The 1% precision criterium in intensities and 1% criterium in standard deviation are defined as a function of solar wind velocity and diffusion coefficient value. The implications for 1D backward and 2D models are also discussed.
Keywords
Cosmic rays, Fokker - Planck equation, heliosphere, SDE method.
| Subcategory | Theoretical Methods |
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Primary authors
Viacheslav Mykhailenko
(Pavol Jozef Safarik University in Kosice)
Dr
Pavol Bobík
(Institute of Experimental Physics Slovak Academy of Sciences)
