Observing Kelvin–Helmholtz instability in solar blowout jet

Kelvin–Helmholtz instability (KHI) is a basic physical process in fluids and magnetized plasmas, with applications successfully modelling e.g. exponentially growing instabilities observed at magnetospheric and heliospheric boundaries, in the solar or Earth’s atmosphere and within astrophysical jets....

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Detalles Bibliográficos
Autores principales: Li, Xiaohong, Zhang, Jun, Yang, Shuhong, Hou, Yijun, Erdélyi, Robert
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5970241/
https://www.ncbi.nlm.nih.gov/pubmed/29802364
http://dx.doi.org/10.1038/s41598-018-26581-4

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5970241/
https://www.ncbi.nlm.nih.gov/pubmed/29802364
http://dx.doi.org/10.1038/s41598-018-26581-4

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