Initiation and propagation of coronal mass ejections

Abstract

This paper reviews recent progress in the research on the initiation and propagation of CMEs. In the initiation part, several trigger mechanisms are discussed; In the propagation part, the observations and modelings of EIT waves/dimmings, as the EUV counterparts of CMEs, are described.

8 pages, 1 figure, an invited review, to appear in J. Astrophys. Astron

References in corpus (3)

• A Model for Solar Coronal Mass Ejections
• Confined and ejective eruptions of kink-unstable flux ropes
• Self-Consistent MHD Modeling of a Coronal Mass Ejection, Coronal Dimming, and a Giant Cusp-Shaped Arcade Formation

Cited by in corpus (11)

• The Relation between EIT Waves and Coronal Mass Ejections
• Statistical Analysis of Filament Features Based on the Hα Solar Images from 1988 to 2013 by Computer Automated Detection Method
• Study the build-up, initiation and acceleration of 2008 April 26 coronal mass ejection observed by STEREO
• Development of an Advanced Automated Method for Solar Filament Recognition and Its Scientific Application to a Solar Cycle of MLSO Hα Data
• Solar Filament Recognition Based on Deep Learning
• The dependence of the EIT wave velocity on the magnetic field strength
• Can We Determine the Filament Chirality by the Filament Footpoint Location or the Barb-bearing?
• Solar Cycle Dependence of ICME Composition
• EIT waves and coronal magnetic field diagnostics
• Composition Comparison between ICMEs from Active Regions and Quiet-Sun Regions
• Graph Learning with Multiplicative Aggregation for Solar Filament Fragment Association Modeling in Full-disk H$\alpha$ Images