The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been
known for over 50 years and significant progress has been made in this research area. It has …

This paper outlines the current understanding of solar flares, mainly focused on
magnetohydrodynamic (MHD) processes responsible for producing a flare. Observations …

Wave and oscillatory activity of the solar corona is confidently observed with modern
imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and …

We review the physical processes of particle acceleration, injection, propagation, trap**,
and energy loss in solar flare conditions. An understanding of these basic physical …

An emerging paradigm for the dissipation of magnetic turbulence in the supersonic solar
wind is via localized small-scale reconnection processes, essentially between quasi-2D …

Quasi-periodic pulsations (QPP) are a common feature of flaring energy releases in the
solar atmosphere, observed in all bands, from radio to hard X-ray. In this review we …

We performed two-dimensional numerical simulations of solar coronal X-ray jets by solving
the resistive magnetohydrodynamic (MHD) equations. The simulations were based on the …

Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

Expanding upon the ideas first proposed in his seminal book Cosmical Magnetic Fields,
Eugene N. Parker here offers the first in-depth treatment of the magnetohydrodynamic theory …

Energetic electrons of up to tens of MeV are created during explosive phenomena in the
solar corona. While many theoretical models consider magnetic reconnection as a possible …