OBSERVING FLUX ROPE FORMATION DURING THE IMPULSIVE PHASE OF A SOLAR ERUPTION
Authors:
- X. ChengXCX. Cheng
- J. ZhangJZJ. Zhang
- Y. LiuYLY. Liu
- M. D. DingMDM. D. Ding
- 15 April 2011
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 732 (2) , L25
Abstract
No abstract availableAll Related Versions
This publication has 49 references indexed in Scilit:
- FORMATION OF TORUS-UNSTABLE FLUX ROPES AND ELECTRIC CURRENTS IN ERUPTING SIGMOIDSThe Astrophysical Journal, 2009
- EVIDENCE FOR A PRE-ERUPTIVE TWISTED FLUX ROPE USING THE THEMIS VECTOR MAGNETOGRAPHThe Astrophysical Journal, 2009
- Role of projection effects on solar coronal mass ejection properties: 1. A study of CMEs associated with limb activityJournal of Geophysical Research, 2004
- Coronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. I. Boundary Motion–driven EvolutionThe Astrophysical Journal, 2003
- Flare Plasma Cooling from 30 MK down to 1 MK modeled from Yohkoh, GOES, and TRACE observations during the Bastille Day Event (14 July 2000)Solar Physics, 2001
- A Twisted Flux Rope Model for Coronal Mass Ejections and Two-Ribbon FlaresThe Astrophysical Journal, 2000
- Sigmoidal morphology and eruptive solar activityGeophysical Research Letters, 1999
- A Model for Solar Coronal Mass EjectionsThe Astrophysical Journal, 1999
- Theory of prominence eruption and propagation: Interplanetary consequencesJournal of Geophysical Research, 1996
- A magnetic cloud and a coronal mass ejectionGeophysical Research Letters, 1982