On the Origin, 3D Structure and Dynamic Evolution of CMEs Near Solar Minimum
- 2 October 2009
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 259 (1-2) , 143-161
Abstract
No abstract availableKeywords
This publication has 47 references indexed in Scilit:
- The Current Sheet Associated with the 2003 November 4 Coronal Mass Ejection: Density, Temperature, Thickness, and Line WidthThe Astrophysical Journal, 2008
- Spatial Relationship between Solar Flares and Coronal Mass EjectionsThe Astrophysical Journal, 2008
- On the three-dimensional configuration of coronal mass ejectionsAstronomy & Astrophysics, 2004
- 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
- Magnetic Geometry and Dynamics of the Fast Coronal Mass Ejection of 1997 September 9The Astrophysical Journal, 2000
- Coronal Mass Ejections1999
- A Model for Solar Coronal Mass EjectionsThe Astrophysical Journal, 1999
- Evidence of an Erupting Magnetic Flux Rope: LASCO Coronal Mass Ejection of 1997 April 13The Astrophysical Journal, 1997
- The Large Angle Spectroscopic Coronagraph (LASCO)Solar Physics, 1995