Coronal mass ejections and their sheath regions in interplanetary space

Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a shock wave develops ahead of the ICME. The turbulent region between the shock and the ICME is called the sheath regi...

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Detalles Bibliográficos
Autores principales: Kilpua, Emilia, Koskinen, Hannu E. J., Pulkkinen, Tuija I.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 2017
Materias:
Review Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6956910/
https://www.ncbi.nlm.nih.gov/pubmed/31997985
http://dx.doi.org/10.1007/s41116-017-0009-6

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6956910/
https://www.ncbi.nlm.nih.gov/pubmed/31997985
http://dx.doi.org/10.1007/s41116-017-0009-6

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