The Trigger Mechanism of Solar Flares in a Coronal Arcade with Reversed Magnetic Shear
- 20 July 2004
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 610 (1) , 537-549
Abstract
No abstract availableKeywords
This publication has 35 references indexed in Scilit:
- Kink unstable coronal loops: current sheets, current saturation and magnetic reconnectionSolar Physics, 2003
- Coronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. I. Boundary Motion–driven EvolutionThe Astrophysical Journal, 2003
- Localization, the clue to fast magnetic reconnectionPhysics of Plasmas, 2001
- An Emerging Flux Trigger Mechanism for Coronal Mass EjectionsThe Astrophysical Journal, 2000
- Simulations of Three‐Dimensional Reconnection in the Solar CoronaThe Astrophysical Journal, 2000
- Helicity Redistribution during Relaxation of Astrophysical PlasmasPhysical Review Letters, 2000
- Photospheric Magnetic Field Evolution and Eruptive FlaresThe Astrophysical Journal, 1995
- Magnetic arcade evolution and instabilitySolar Physics, 1989
- The topological properties of magnetic helicityJournal of Fluid Mechanics, 1984
- Finite-Resistivity Instabilities of a Sheet PinchPhysics of Fluids, 1963