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
Publicado: 2018
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:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v1031_n1_p_Vigh
http://hdl.handle.net/20.500.12110/paper_17426588_v1031_n1_p_Vigh
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_17426588_v1031_n1_p_Vigh
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spelling paper:paper_17426588_v1031_n1_p_Vigh2023-06-08T16:27:09Z Exploring the Kipenhahn-Schlüter model 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 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 states without and with magnetic shear solutions for the system of equations in the beta plasma range between 0 and 1,6. Finally, we computed magnetic streamlines field for the different shears. Joining all these elements we obtained a catalogue to study the stability of the prominence candidates. © 2018 Institute of Physics Publishing. All rights reserved. 2018 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v1031_n1_p_Vigh http://hdl.handle.net/20.500.12110/paper_17426588_v1031_n1_p_Vigh
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic 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
spellingShingle 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
Exploring the Kipenhahn-Schlüter model
topic_facet 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
description 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 states without and with magnetic shear solutions for the system of equations in the beta plasma range between 0 and 1,6. Finally, we computed magnetic streamlines field for the different shears. Joining all these elements we obtained a catalogue to study the stability of the prominence candidates. © 2018 Institute of Physics Publishing. All rights reserved.
title Exploring the Kipenhahn-Schlüter model
title_short Exploring the Kipenhahn-Schlüter model
title_full Exploring the Kipenhahn-Schlüter model
title_fullStr Exploring the Kipenhahn-Schlüter model
title_full_unstemmed Exploring the Kipenhahn-Schlüter model
title_sort exploring the kipenhahn-schlüter model
publishDate 2018
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v1031_n1_p_Vigh
http://hdl.handle.net/20.500.12110/paper_17426588_v1031_n1_p_Vigh
_version_ 1768543202440118272

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