Flare differentially rotates sunspot on Sun's surface

Sunspots are concentrations of magnetic field visible on the solar surface (photosphere). It was considered implausible that solar flares, as resulted from magnetic reconnection in the tenuous corona, would cause a direct perturbation of the dense photosphere involving bulk motion. Here we report th...

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Detalles Bibliográficos
Autores principales: Liu, Chang, Xu, Yan, Cao, Wenda, Deng, Na, Lee, Jeongwoo, Hudson, Hugh S., Gary, Dale E., Wang, Jiasheng, Jing, Ju, Wang, Haimin
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2016
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5062561/
https://www.ncbi.nlm.nih.gov/pubmed/27721463
http://dx.doi.org/10.1038/ncomms13104

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5062561/
https://www.ncbi.nlm.nih.gov/pubmed/27721463
http://dx.doi.org/10.1038/ncomms13104

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