Particle acceleration and transport in reconnecting twisted loops in a stratified atmosphere

Gordovskyy, M., Browning, P.K., Kontar, E.P. and Bian, N.H. (2014) Particle acceleration and transport in reconnecting twisted loops in a stratified atmosphere. Astronomy and Astrophysics, 561, A72. (doi:10.1051/0004-6361/201321715)

Gordovskyy, M., Browning, P.K., Kontar, E.P. and Bian, N.H. (2014) Particle acceleration and transport in reconnecting twisted loops in a stratified atmosphere. Astronomy and Astrophysics, 561, A72. (doi:10.1051/0004-6361/201321715)

Full text not currently available from Enlighten.

Abstract

Context. Twisted coronal loops should be ubiquitous in the solar corona. Twisted magnetic fields contain excess magnetic energy, which can be released during magnetic reconnection, causing solar flares.<p></p> Aims. The aim of this work is to investigate magnetic reconnection, and particle acceleration and transport in kink-unstable twisted coronal loops, with a focus on the effects of resistivity, loop geometry and atmospheric stratification. Another aim is to perform forward-modelling of bremsstrahlung emission and determine the structure of hard X-ray sources.<p></p> Methods. We use a combination of magnetohydrodynamic (MHD) and test-particle methods. First, the evolution of the kinking coronal loop is considered using resistive MHD model, incorporating atmospheric stratification and loop curvature. Then, the obtained electric and magnetic fields and density distributions are used to calculate electron and proton trajectories using a guiding-centre approximation, taking into account Coulomb collisions.<p></p> Results. It is shown that electric fields in twisted coronal loops can effectively accelerate protons and electrons to energies up to 10 MeV. High-energy particles have hard, nearly power-law energy spectra. The volume occupied by high-energy particles demonstrates radial expansion, which results in the expansion of the visible hard X-ray loop and a gradual increase in hard X-ray footpoint area. Synthesised hard X-ray emission reveals strong footpoint sources and the extended coronal source, whose intensity strongly depends on the coronal loop density.<p></p>

Item Type:Articles
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Kontar, Dr Eduard and Browning, Prof Philippa and Bian, Dr Nicolas Horace
Authors: Gordovskyy, M., Browning, P.K., Kontar, E.P., and Bian, N.H.
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Astronomy and Astrophysics
Publisher:EDP Sciences
ISSN:0004-6361
ISSN (Online):1432-0746
Related URLs:

University Staff: Request a correction | Enlighten Editors: Update this record

Project CodeAward NoProject NamePrincipal InvestigatorFunder's NameFunder RefLead Dept
542081Rolling Programme in Solar and Plasma AstrophysicsLyndsay FletcherScience & Technologies Facilities Council (STFC)ST/I001808/1P&A - PHYSICS & ASTRONOMY