Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona

Solar flares often involve the acceleration of particles to relativistic energies and the generation of high-intensity bursts of radio emission. In some cases, the radio bursts can show periodic or quasiperiodic intensity pulsations. However, precisely how these pulsations are generated is still sub...

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Detalles Bibliográficos
Autores principales: Carley, Eoin P., Hayes, Laura A., Murray, Sophie A., Morosan, Diana E., Shelley, Warren, Vilmer, Nicole, Gallagher, Peter T.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2019
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6533292/
https://www.ncbi.nlm.nih.gov/pubmed/31123312
http://dx.doi.org/10.1038/s41467-019-10204-1

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6533292/
https://www.ncbi.nlm.nih.gov/pubmed/31123312
http://dx.doi.org/10.1038/s41467-019-10204-1

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