25 years of self-organized criticality: solar and astrophysics

MJ Aschwanden, NB Crosby, M Dimitropoulou… - Space Science …, 2016 - Springer
Shortly after the seminal paper “Self-Organized Criticality: An explanation of 1/f noise” by
Bak et al.(1987), the idea has been applied to solar physics, in “Avalanches and the …

The formation of kappa-distribution accelerated electron populations in solar flares

NH Bian, AG Emslie, DJ Stackhouse… - The Astrophysical …, 2014 - iopscience.iop.org
Driven by recent RHESSI observations of confined loop-top hard X-ray sources in solar
flares, we consider stochastic acceleration of electrons in the presence of Coulomb …

Test particle acceleration in three-dimensional magnetohydrodynamic turbulence

P Dmitruk, WH Matthaeus, N Seenu… - the astrophysical …, 2003 - iopscience.iop.org
We perform numerical experiments of test particle acceleration on turbulent magnetic and
electric fields obtained from pseudospectral direct numerical solutions of the compressible …

Variability of the occurrence frequency of solar flares and the statistical flare

MK Georgoulis, L Vlahos - … and Astrophysics, v. 336, p. 721-734 …, 1998 - adsabs.harvard.edu
Abstract Self-Organised Criticality (SOC), embedded in cellular automata models, has been
so far viewed as an attractive phenomenological approach for studying the statistical …

Recent progress in understanding energy conversion and particle acceleration in the solar corona

B Kliem, A MacKinnon, G Trottet, T Bastian - Energy conversion and …, 2003 - Springer
We report on results of the working group sessions at the CESRA 2001 workshop on
“Energy Conversion and Particle Acceleration in the Solar Corona” which was focused on …

Particle acceleration in a model of a turbulent reconnecting plasma: a fractional diffusion approach

NH Bian, PK Browning - The Astrophysical Journal, 2008 - iopscience.iop.org
High-energy charged particles are produced during solar flares. These may be accelerated
by the strong electric fields associated with the magnetic reconnection process which is the …

VARIABILITY AND SPECTRAL MODELING OF THE HARD X-RAY EMISSION OF GX 339− 4 IN A BRIGHT LOW/HARD STATE

R Droulans, R Belmont, J Malzac… - The Astrophysical …, 2010 - iopscience.iop.org
We study the high-energy emission of the Galactic black hole candidate GX 339− 4 using
INTEGRAL/SPI and simultaneous RXTE/PCA data. By the end of 2007 January, when it …

Effects of a velocity shear on double current sheet systems: Explosive reconnection and particle acceleration

A Paul, B Vaidya - Physics of Plasmas, 2021 - pubs.aip.org
The effect of a parallel velocity shear on the explosive phase of a double current sheet
system is investigated within the 2D resistive magnetohydrodynamic framework. We further …

Particle acceleration in stressed coronal magnetic fields

R Turkmani, L Vlahos, K Galsgaard… - The Astrophysical …, 2005 - iopscience.iop.org
This Letter presents an analysis of particle acceleration in a model of the complex magnetic
field environment in the flaring solar corona. A slender flux tube, initially in hydrodynamic …

A classification scheme for turbulent acceleration processes in solar flares

N Bian, AG Emslie, EP Kontar - The Astrophysical Journal, 2012 - iopscience.iop.org
We establish a classification scheme for stochastic acceleration models involving low-
frequency plasma turbulence in a strongly magnetized plasma. This classification takes into …