ICMEs in the inner heliosphere: Origin, evolution and propagation effects

2006 | journal article. A publication with affiliation to the University of Göttingen.

Jump to: Cite & Linked | Documents & Media | Details | Version history

Cite this publication

​ICMEs in the inner heliosphere: Origin, evolution and propagation effects​
Forsyth, R. J.; Bothmer, V.; Cid, M. C.; Crooker, N. U.; Horbury, T. S.; Kecskemety, K. & Klecker, B. et al.​ (2006) 
Space Science Reviews123(1-3) pp. 383​-416​.​ DOI: https://doi.org/10.1007/s11214-006-9022-0 

Documents & Media

License

GRO License GRO License

Details

Authors
Forsyth, R. J.; Bothmer, Volker; Cid, Maria C.; Crooker, N. U.; Horbury, T. S.; Kecskemety, K.; Klecker, B.; Linker, J. A.; Odstrcil, Dusan; Reiner, M. J.; Richardson, I. G.; Rodriguez-Pacheco, J.; Schmidt, J. M.; Wimmer-Schweingruber, R. F.
Abstract
This report assesses the current status of research relating the origin at the Sun, the evolution through the inner heliosphere and the effects on the inner heliosphere of the interplanetary counterparts of coronal mass ejections (ICMEs). The signatures of ICMEs measured by in-situ spacecraft are determined both by the physical processes associated with their origin in the low corona, as observed by space-borne coronagraphs, and by the physical processes occurring as the ICMEs propagate out through the inner heliosphere, interacting with the ambient solar wind. The solar and in-situ observations are discussed as are efforts to model the evolution of ICMEs from the Sun out to 1 AU.
Issue Date
2006
Status
published
Publisher
Springer
Journal
Space Science Reviews 
ISSN
1572-9672; 0038-6308

Reference

Citations


Social Media