Hopf bifurcations in coronal loops. II. Nonlinear evolution of instabilities

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In a previous paper, we have modeled the coupling between corona and chromosphere and derived a non-linear set of equations, where the global stability properties of the coronal plasma can be studied. The linear stability analysis indicates that the static equilibrium is stable unless the heating ra...

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Detalles Bibliográficos
Autores principales: Gómez, D., Sicardi Schifino, A., Ferro Fontán, C.
Formato: JOUR
Materias:
Hydromagnetics
Sun: chromosphere
Sun: corona
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v352_n1_p326_Gomez
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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