Are giant tornadoes the legs of solar prominences?

Wedemeyer, Sven, Scullion, Eamon, Rouppe van der Voort, Luc, Bosnjak, Antonija and Antolin, Patrick (2013) Are giant tornadoes the legs of solar prominences? The Astrophysical Journal, 774 (2). p. 123. ISSN 0004-637X

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Official URL: http://dx.doi.org/10.1088/0004-637X/774/2/123

Abstract

Observations in the 171 Å channel of the Atmospheric Imaging Assembly of the space-borne Solar Dynamics Observatory show tornado-like features in the atmosphere of the Sun. These giant tornadoes appear as dark, elongated, and apparently rotating structures in front of a brighter background. This phenomenon is thought to be produced by rotating magnetic field structures that extend throughout the atmosphere. We characterize giant tornadoes through a statistical analysis of properties such as spatial distribution, lifetimes, and sizes. A total number of 201 giant tornadoes are detected in a period of 25 days, suggesting that, on average, about 30 events are present across the whole Sun at a time close to solar maximum. Most tornadoes appear in groups and seem to form the legs of prominences, thus serving as plasma sources/sinks. Additional Hα observations with the Swedish 1 m Solar Telescope imply that giant tornadoes rotate as a structure, although they clearly exhibit a thread-like structure. We observe tornado groups that grow prior to the eruption of the connected prominence. The rotation of the tornadoes may progressively twist the magnetic structure of the prominence until it becomes unstable and erupts. Finally, we investigate the potential relation of giant tornadoes to other phenomena, which may also be produced by rotating magnetic field structures. A comparison to cyclones, magnetic tornadoes, and spicules implies that such events are more abundant and short-lived the smaller they are. This comparison might help to construct a power law for the effective atmospheric heating contribution as a function of spatial scale.

Item Type: Article
Uncontrolled Keywords: Sun: atmosphere, Sun: filaments, prominences
Subjects: F500 Astronomy
Department: Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering
Depositing User: Paul Burns
Date Deposited: 11 Dec 2018 12:11
Last Modified: 10 Oct 2019 16:16
URI: http://nrl.northumbria.ac.uk/id/eprint/37181

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