Exploring the Kipenhahn-Schlüter model

We explored the generalised Kippenhan-Schluter model non-isothermal stationary states for solar prominences where we made some improvements. The most important is to use recent observed values of radiative losses to build the piecewise heat balance equation. We explicity found several stationary sta...

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Detalles Bibliográficos
Autores principales: Vigh, C.D., Gonzalez, R., Rial, D.
Formato: CONF
Materias:
Numerical models
Plasma devices
Plasma flow
Plasma jets
Heat balance equations
Magnetic shear
Nonisothermal
Observed values
Radiative loss
Solar prominences
Stationary state
System of equations
Magnetoplasma
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17426588_v1031_n1_p_Vigh
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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