| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1777447 | Journal of Atmospheric and Solar-Terrestrial Physics | 2011 | 6 Pages |
Abstract
An account is presented of the Flux Tube Tectonics model for heating the solar corona, in which a multitude of current sheets are continually forming and dissipating. In addition, a model is summarised for the time-dependent response of the corona to the sudden dissipation of one such current sheet.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Eric R Priest,