About: Solar prominence magnetic configurations derived numerically from convection

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Attributs	Valeurs
type	work Article
Is Part Of	http://hub.abes.fr/edp/periodical/aa/2001/volume_371/issue_1/w
Subject	supergranulation Planets and planetary systems convection prominences
Title	Solar prominence magnetic configurations derived numerically from convection
Date	2001-01-01(xsd:dateTime)
has manifestation of work	http://hub.abes.fr/edp/periodical/aa/2001/volume_371/issue_1/aah2648/m/print http://hub.abes.fr/edp/periodical/aa/2001/volume_371/issue_1/aah2648/m/web
related by	http://hub.abes.fr/edp/periodical/aa/2001/volume_371/issue_1/aah2648/authorship/1
Author	McKaig, I.
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.
article type	research-article
publisher identifier	aah2648
Date Copyrighted	2001-01-01(xsd:dateTime)
Rights	© ESO, 2001
Rights Holder	ESO
is part of this journal	Astronomy & Astrophysics
is primary topic of	http://hub.abes.fr/edp/periodical/aa/2001/volume_371/issue_1/aah2648/w/record

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