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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...
| Autores principales: | , , , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2019
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| Materias: | |
| 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 |