May 13, 2016 · Our results are consistent with those found by Chen and Petrosian (2013) for two flares using non-parametric inversion methods, according to which we have weak diffusion conditions, and …

We show that using a more accurate treatment of the transport of the accelerated electrons to the footpoints and to Earth can account for this discrepancy.

Dec 15, 2023 · Solar Energetic Particle (SEP) events are interesting from a scientific perspective as they are the product of a broad set of physical processes from …

Abstract A knowledge of the particle escape time from the acceleration regions of many space and astrophysical sources is of critical importance in the analysis of emission signatures produced...

Jun 28, 2024 · Electrons and ions are accelerated in the solar flare re-connection sites and in the associated CME shock environments. Based on the radiative signatures of flares, stochastic …

Jul 1, 2003 · The evolution of magnetohydrodynamic turbulence resulting from magnetic reconnection will be investigated, and subsequently employed to evaluate the transport and acceleration of …

It is vital to understand both the flare and CME shock acceleration processes in order to understand the basic physics of solar eruptions and to enable predictions of energetic particle fluxes that can …

Solar flares are among the most remarkable phenomenon of energy release and particle acceleration in our solar system. A large amount of magnetic energy in the solar corona can be released and …

We outline in this review three recent observations which indicate that the following physical processes may happen during solar flares: (1) Release of energy in a large number of microflares; (2) short time …

May 13, 2016 · Our results are consistent with those found by Chen and Petrosian (2013) for two flares using non-parametric inversion methods, according to which we have weak diffusion conditions, and …