The Structure and Evolution of a Sigmoidal Active Region
Open Access
- 1 August 2002
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 574 (2), 1021-1038
- https://doi.org/10.1086/341090
Abstract
No abstract availableThis publication has 50 references indexed in Scilit:
- Are Magnetic Dips Necessary for Prominence Formation?The Astrophysical Journal, 2001
- The Effects of Rotation on the Evolution of Rising Omega Loops in a Stratified Model Convection ZoneThe Astrophysical Journal, 2001
- The onset and association of CMEs with sigmoidal active regionsGeophysical Research Letters, 2000
- Whole Sun Month at solar minimum: An introductionJournal of Geophysical Research, 1999
- Synoptic Sun during the first Whole Sun Month Campaign: August 10 to September 8, 1996Journal of Geophysical Research, 1999
- X‐ray coronal changes during Halo CMEsGeophysical Research Letters, 1998
- Reconnection and Helicity in a Solar FlareThe Astrophysical Journal, 1996
- Evidence for Helically Kinked Magnetic Flux Ropes in Solar EruptionsThe Astrophysical Journal, 1996
- On the spontaneous formation of electric current sheets above a flexible solar photosphereThe Astrophysical Journal, 1991
- The topological properties of magnetic helicityJournal of Fluid Mechanics, 1984