Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles: II. Modes in twisted non-isothermal magnetic field configurations

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

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Detalles Bibliográficos
Autores principales: Costa, A., González, R.
Formato: Artículo publishedVersion
Publicado: 2008
Materias:
Sun: corona
Sun: magnetic fields
Sun: oscillations
Absorption
Energy efficiency
Equations of motion
Magnetic field measurement
Magnetic fields
Magnetic materials
Mathematical operators
Mechanisms
Solar energy
Thermodynamic stability
Thermodynamics
Coronal loops
Coupled systems
Critical values
Eigen-frequencies
Eigen-modes
Energy equation
Energy principles
Equation of motion
Equilibrium parameters
Helicity
Hermitian operators
Intensity values
Irreversible energy
Long wavelengths
Magnetic energies
Magnetic field configurations
Magnetic field strengths
Mode analysis
Non-equilibrium
Non-isothermal
Resonant absorption
Solar coronal loops
Stabilizing effects
System stability
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v489_n2_p755_Costa
http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00046361_v489_n2_p755_Costa_oai
Aporte de:
Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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