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A theoretical model for the magnetic helicity of solar active regions

✍ Scribed by Piyali Chatterjee; Arnab Rai Choudhuri; Kristof Petrovay; Dibyendu Nandy


Book ID
108065995
Publisher
Elsevier Science
Year
2008
Tongue
English
Weight
284 KB
Volume
41
Category
Article
ISSN
0273-1177

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A note on the evolution of magnetic heli
✍ Wang Jingxiu πŸ“‚ Article πŸ“… 1996 πŸ› Springer 🌐 English βš– 301 KB

The evolution of magnetic helicity in a rapidly growing active region is governed mainly by the advection of magnetic fields into the photosphere. Dissipation at the photosphere makes only a minor contribution to helicity evolution. Current helicity dissipation in the three-dimensional domain around