Formation and Large-Scale Patterns of Filament Channels and Filaments
- 21 October 2014
- book chapter
- Published by Springer Nature
- p. 355-380
Abstract
No abstract availableKeywords
This publication has 87 references indexed in Scilit:
- THE EMERGENCE OF A TWISTED FLUX TUBE INTO THE SOLAR ATMOSPHERE: SUNSPOT ROTATIONS AND THE FORMATION OF A CORONAL FLUX ROPEThe Astrophysical Journal, 2009
- On the Formation of Filament ChannelsThe Astrophysical Journal, 2007
- Dynamic and Topological Features of Photospheric and Coronal Activities Produced by Flux Emergence in the SunThe Astrophysical Journal, 2006
- 3D simulations identifying the effects of varying the twist and field strength of an emerging flux tubeAstronomy & Astrophysics, 2006
- Magnetic Reconnection Models of Prominence FormationThe Astrophysical Journal, 2005
- A Simple Dynamical Model for Filament Formation in the Solar CoronaThe Astrophysical Journal, 2005
- Are Magnetic Dips Necessary for Prominence Formation?The Astrophysical Journal, 2001
- Magnetostatic structures of the solar corona. 2: The magnetic topology of quiescent prominencesThe Astrophysical Journal, 1995
- Magnetic fields in quiescent prominencesThe Astrophysical Journal, 1990
- Solar magnetic fields derived from hydrogen alpha filtergramsReviews of Geophysics, 1972