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

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...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Gomez, Daniel Osvaldo, Sicardi Schifino, Aníbal Carlos, Ferro Fontán, Constantino
Publicado: 1990
Materias:
Hydromagnetics
Sun: chromosphere
Sun: corona
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v352_n1_p326_Gomez
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

Ejemplares similares

Ejemplares similares