Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Heating of braided coronal loops.

Wilmot-Smith, A. L. and Pontin, D. I. and Yeates, A. R. and Hornig, G. (2011) 'Heating of braided coronal loops.', Astronomy & astrophysics., 536 . A67.

Abstract

Aims. We investigate the relaxation of braided magnetic loops in order to find out how the type of braiding via footpoint motions affects resultant heating of the loop. Methods. Two magnetic loops, braided in different ways, are used as initial conditions in resistive MHD simulations and their subsequent evolution is studied. Results. The fields both undergo a resistive relaxation in which current sheets form and fragment and the system evolves towards a state of lower energy. In one case this relaxation is very efficient with current sheets filling the volume and homogeneous heating of the loop occurring. In the other case fewer current sheets develop, less magnetic energy is released in the process and a patchy heating of the loop results. The two cases, although very similar in their setup, can be distinguished by the mixing properties of the photospheric driver. The mixing can be measured by the topological entropy of the plasma flow, an observable quantity.

Item Type:Article
Keywords:Magnetic fields, Magnetic reconnection, Magnetohydrodynamics (MHD), Plasmas, Sun: corona, Sun: magnetic topology.
Full text:(VoR) Version of Record
Download PDF
(3289Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1051/0004-6361/201117942
Publisher statement:Reproduced with permission from Astronomy & Astrophysics, © ESO, 2011.
Date accepted:28 October 2011
Date deposited:29 April 2015
Date of first online publication:December 2011
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar