EDP Sciences
Free access
Issue
A&A
Volume 371, Number 1, May III 2001
Page(s) 328 - 332
Section The Sun
DOI http://dx.doi.org/10.1051/0004-6361:20010315


A&A 371, 328-332 (2001)
DOI: 10.1051/0004-6361:20010315

Solar prominence magnetic configurations derived numerically from convection

I. McKaig

Department of Mathematics, Tidewater Community College, Virginia Beach, VA 23456, USA

(Received 19 January 2001 / Accepted 28 February 2001)

Abstract
The solar convection zone may be a mechanism for generating the magnetic fields in the corona that create and thermally insulate quiescent prominences. This connection is examined here by numerically solving a diffusion equation with convection (below the photosphere) matched to Laplace's equation (modeling the current free corona above the photosphere). The types of fields formed resemble both Kippenhahn-Schlüter and Kuperus-Raadu configurations with feet that drop into supergranule boundaries.


Key words: supergranulation -- convection -- prominences



© ESO 2001