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Filament Channels: Essential Ingredients for Filament Formation

Published online by Cambridge University Press:  12 April 2016

V. Gaizauskas
V. Gaizauskas*
Affiliation:
Herzberg Institute of Astrophysics, National Research Council of Canada, 100 Sussex Drive, Ottawa, K1A 0R6, Canada

Abstract

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Channels share with their filaments in a hemispheric dependance for the orientation of their axial magnetic fields. This property has significant implications for models of filaments. In support of new model-building exercises, this review examines known signatures of channels, presents evidence that emerging flux plays a key role in creating a new filament channel, and compares channels which form in the belts of active latitudes with those formed closer to the poles.

Type
Birth and Death of Filaments
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 257 - 264
Copyright
Copyright © Astronomical Society of the Pacific 1998

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