Strong coronal channelling and interplanetary evolution of a solar storm up to Earth and Mars

The severe geomagnetic effects of solar storms or coronal mass ejections (CMEs) are to a large degree determined by their propagation direction with respect to Earth. There is a lack of understanding of the processes that determine their non-radial propagation. Here we present a synthesis of data fr...

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Detalhes bibliográficos
Publicado no:Nat Commun
Main Authors: Möstl, Christian, Rollett, Tanja, Frahm, Rudy A., Liu, Ying D., Long, David M., Colaninno, Robin C., Reiss, Martin A., Temmer, Manuela, Farrugia, Charles J., Posner, Arik, Dumbović, Mateja, Janvier, Miho, Démoulin, Pascal, Boakes, Peter, Devos, Andy, Kraaikamp, Emil, Mays, Mona L., Vršnak, Bojan
Formato: Artigo
Idioma:Inglês
Publicado em: Nature Pub. Group 2015
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Article
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC4455070/
https://ncbi.nlm.nih.gov/pubmed/26011032
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms8135
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