Is Magnetic Topology Important for Heating the Solar Atmosphere?

Magnetic fields permeate the entire solar atmosphere weaving an extremely complex pattern on both local and global scales. In order to understand the nature of this tangled web of magnetic fields, its magnetic skeleton, which forms the boundaries between topologically distinct flux domains, may be d...

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Veröffentlicht in:	arXiv.org 2015-05
Hauptverfasser:	Parnell, C E, Stevenson, J E H, Threlfall, J, Edwards, S J
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Boundaries Cycle time Domains Energy dissipation Heating Magnetic fields Physics - Solar and Stellar Astrophysics Separators Solar atmosphere Solar cycle Solar flares Solar magnetic field Solar wind Topology
Online-Zugang:	Volltext
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