Forward Modeling of Coronal Mass Ejection Flux Ropes in the Inner Heliosphere with 3DCORE

Forecasting the geomagnetic effects of solar storms, known as coronal mass ejections (CMEs), is currently severely limited by our inability to predict the magnetic field configuration in the CME magnetic core and by observational effects of a single spacecraft trajectory through its 3‐D structure. C...

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Detalles Bibliográficos
Autores principales: Möstl, C., Amerstorfer, T., Palmerio, E., Isavnin, A., Farrugia, C. J., Lowder, C., Winslow, R. M., Donnerer, J. M., Kilpua, E. K. J., Boakes, P. D.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2018
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5947730/
https://www.ncbi.nlm.nih.gov/pubmed/29780287
http://dx.doi.org/10.1002/2017SW001735

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5947730/
https://www.ncbi.nlm.nih.gov/pubmed/29780287
http://dx.doi.org/10.1002/2017SW001735

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