ROLE OF HELICITY IN THE FORMATION OF INTERMEDIATE FILAMENTS

Citation
Dh. Mackay et al., ROLE OF HELICITY IN THE FORMATION OF INTERMEDIATE FILAMENTS, Solar physics, 180(1-2), 1998, pp. 299-312
Citations number
27
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00380938
Volume
180
Issue
1-2
Year of publication
1998
Pages
299 - 312
Database
ISI
SICI code
0038-0938(1998)180:1-2<299:ROHITF>2.0.ZU;2-C
Abstract
In the last few years new observations have shown that solar filaments and filament channels have a surprising hemispheric pattern. To expla in this pattern, a new theory for filament channel and filament format ion is put forward. The theory describes the formation of a specific t ype of filament, namely the 'intermediate filament' which forms either between active regions or at the boundary of an active region. It des cribes the formation in terms of the emergence of a sheared activity c omplex. The complex then interacts with remnant flux and, after conver gence and flux cancellation, the filament forms in the channel. A key feature of the model is the net magnetic helicity of the complex. With the correct sign a filament channel can form, but with the opposite s ign no filament channel forms after convergence. It is shown how the h emispheric pattern of helicity in emerging flux regions produces the o bserved hemispheric pattern for filaments.