SIMULATIONS of the KELVIN-HELMHOLTZ INSTABILITY DRIVEN by CORONAL MASS EJECTIONS in the TURBULENT CORONA
Recent high-resolution Atmospheric Imaging Assembly/Solar Dynamics Observatory images show evidence of the development of the Kelvin-Helmholtz (KH) instability, as coronal mass ejections (CMEs) expand in the ambient corona. A large-scale magnetic field mostly tangential to the interface is inferred,...
Guardado en:
| Autores principales: | Gómez, D.O., Deluca, E.E., Mininni, P.D. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v818_n2_p_Gomez |
| Aporte de: |
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