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Coronal Condensation in Funnel Prominences as Return Flows of the Chromosphere-Corona Mass Cycle View all abstracts by submitter

Wei Liu   Submitted: 2014-04-03 19:04

We present SDO/AIA observations of a potentially novel type of prominence, called "funnel prominence", that forms out of coronal condensation at magnetic dips. They can drain a large amount of mass (up to 1015 g/day) and may play an important role as return flows of the recently recognized chromosphere-corona mass cycle. We compare funnel prominences with large-scale polar crown prominences, cloud prominences or coronal spiders, as well as coronal rain.

Authors: Wei Liu, Thomas E. Berger, B. C. Low
Projects: SDO-AIA

Publication Status: Published 01/2014, IAU Sympos., Vol. 300, pp. 441, DOI: 10.1017/S1743921313011460
Last Modified: 2014-04-07 10:55
Go to main E-Print page  A Chain of Winking (Oscillating) Filaments Triggered by an Invisible Extreme-Ultraviolet Wave  Nonlinear Force-Free Field Extrapolation of a Coronal Magnetic Flux Rope Supporting a Large-Scale Filament from Photospheric Vector Magnetogram  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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