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Taneev, S.N. and Berezhko, E.G. (2020) Solar Cosmic Ray Acceleration at the Front of a Fast Shock in the Lower Solar Corona. Journal of Experimental and Theoretical Physics, 131, 422-431.
https://doi.org/10.1134/s1063776120080075

has been cited by the following article:

• TITLE: Transport in Astrophysics: VIII. Cosmic Ray Acceleration in the Solar Corona

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: Cosmic Rays, Particle Acceleration

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.16 No.2, May 28, 2026

  ABSTRACT: We derive the acceleration, velocity and distance of a cosmic ray (CR) due to an astrophysical electric field in the framework of special relativity. The relation between distance and time has been inverted, which allows expressing the velocity as a function of the distance. A simulation is performed for the observed spectrum of CRs adopting two distributions for them: the Maxwell Jüttner distribution and the gamma-Pareto II distribution.