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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Detalles Bibliográficos
Autores principales: 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: Online Artículo Texto
Lenguaje:English
Publicado: Nature Pub. Group 2015
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4455070/
https://www.ncbi.nlm.nih.gov/pubmed/26011032
http://dx.doi.org/10.1038/ncomms8135

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