Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays
beyond 1 GeV. This review focuses on recent observations in EUV, soft and hard X-rays …

Impulsive solar energetic particle events are widely believed to be due to the prompt escape
into the interplanetary medium of flare-accelerated particles produced by solar eruptive …

Solar flares are powerful radiations occurring in the Sun's atmosphere. They are powered by
magnetic reconnection, a phenomenon that can convert magnetic energy into other forms of …

With an emphasis on numerical modelling, Physics of the Sun: A First Course presents a
quantitative examination of the physical structure of the Sun and the conditions of its …

Context. The standard model for eruptive flares has been extended to three dimensions (3D)
in the past few years. This model predicts typical J-shaped photospheric footprints of the …

Electric currents in Geospace and beyond Geophysical Monograph Series Page 2 Geophysical
Monograph Series 184 Carbon Cycling in Northern Peatlands Andrew J. Baird, Lisa R. Belyea …

This work is a continuation of Paper I and is devoted to the analysis of nonthermal electron
dynamics and plasma heating in the confined M1. 2 class solar flare SOL2015-03-15T22 …

There are still debates over whether particle acceleration in solar flares may occur due to
interruption of electric currents flowing along magnetic loops. To contribute to this debate …

Magnetic field line reconnection is a universal plasma process responsible for the
conversion of magnetic field energy to plasma heating and charged particle acceleration …

We present a comprehensive analysis of the formation and the evolution of a fan-spine-like
configuration that developed over a complex photospheric configuration where dispersed …