The Effect of the Parametric Decay Instability on the Morphology of Coronal Type III Radio Bursts
The nonlinear evolution of Alfvén waves in the solar corona leads to the generation of Alfvénic turbulence. This description of the Alfvén waves involves parametric instabilities where the parent wave decays into slow mode waves giving rise to density fluctuations. These density fluctuations, in tur...
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| Hoofdauteurs: | , , , , , , |
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| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
IOP Publishing
2023-01-01
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| Reeks: | The Astrophysical Journal Letters |
| Onderwerpen: | |
| Online toegang: | https://doi.org/10.3847/2041-8213/ad137e |
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