Topical Issue in Solar Physics: Flux-rope Structure of Coronal Mass Ejections Preface
arXiv:1304.0085 · doi:10.1007/s11207-013-0280-1
Abstract
This Topical Issue of Solar Physics, devoted to the study of flux-rope structure in coronal mass ejections (CMEs), is based on two Coordinated Data Analysis Workshops (CDAWs) held in 2010 (20 - 23 September in Dan Diego, California, USA) and 2011 (September 5-9 in Alcala, Spain). The primary purpose of the CDAWs was to address the question: Do all CMEs have flux rope structure? There are 18 papers om this topical issue, including this preface.
4 pages
References in corpus (4)
- Interplanetary shocks lacking type II radio bursts
- Magnetic Field Configuration Models and Reconstruction Methods for Interplanetary Coronal Mass Ejections
- The Solar Connection of Enhanced Heavy Ion Charge States in the Interplanetary Medium: Implications for the Flux-rope Structure of CMEs
- Near-Sun Flux Rope Structure of CMEs
Cited by in corpus (4)
- Estimation of Reconnection Flux using Post-eruption Arcades and Its Relevance to 1-au Magnetic Clouds
- Coronal Flux Ropes and their Interplanetary Counterparts
- Simulating Solar Coronal Mass Ejections constrained by Observations of their Speed and Poloidal flux
- Comparison of counterstreaming suprathermal electron signatures of ICMEs with and without magnetic cloud: are all ICMEs flux ropes?