Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles

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Aims. We study the modes and stability of non-isothermal coronal loop models with different intensity values of the equilibrium magnetic field. Methods. We use an energy principle obtained via non-equilibrium thermodynamic arguments. The principle is expressed in terms of Hermitian operators and all...

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Detalles Bibliográficos
Autores principales: Costa, A., González, R.
Formato: JOUR
Materias:
Standards
Sun: corona
Waves
Continuous spectrum
Corona
Solar coronal loops
Thermodynamic irreversible energy principles
Magnetic fields
Mathematical models
Mathematical operators
Spectrum analysis
System stability
Thermodynamics
Solar radiation
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v458_n3_p953_Costa
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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