Abstract:
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.
Registro:
Documento: |
Conferencia
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Título: | Exploring the Kipenhahn-Schlüter model |
Autor: | Vigh, C.D.; Gonzalez, R.; Rial, D. |
Filiación: | Instituto de Ciencias, Universidad Nacional de General Sarmiento, Los Polvorines, Buenos Aires, Argentina Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales, Departamento de Física, Buenos Aires, Argentina CONICET-Universidad de Buenos Aires, Instituto de Física Del Plasma (INFIP), Buenos Aires, Argentina Instituto de Desarrollo Humano, Universidad Nacional de General Sarmiento, Los Polvorines, Buenos Aires, Argentina Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales, Departamento de Matematica, Buenos Aires, Argentina
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Palabras clave: | 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 |
Año: | 2018
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Volumen: | 1031
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Número: | 1
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DOI: |
http://dx.doi.org/10.1088/1742-6596/1031/1/012012 |
Título revista: | 12th International Conference on Numerical Modeling of Space Plasma Flows, ASTRONUM 2017
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Título revista abreviado: | J. Phys. Conf. Ser.
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ISSN: | 17426588
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v1031_n1_p_Vigh |
Referencias:
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Citas:
---------- APA ----------
Vigh, C.D., Gonzalez, R. & Rial, D.
(2018)
. Exploring the Kipenhahn-Schlüter model. 12th International Conference on Numerical Modeling of Space Plasma Flows, ASTRONUM 2017, 1031(1).
http://dx.doi.org/10.1088/1742-6596/1031/1/012012---------- CHICAGO ----------
Vigh, C.D., Gonzalez, R., Rial, D.
"Exploring the Kipenhahn-Schlüter model"
. 12th International Conference on Numerical Modeling of Space Plasma Flows, ASTRONUM 2017 1031, no. 1
(2018).
http://dx.doi.org/10.1088/1742-6596/1031/1/012012---------- MLA ----------
Vigh, C.D., Gonzalez, R., Rial, D.
"Exploring the Kipenhahn-Schlüter model"
. 12th International Conference on Numerical Modeling of Space Plasma Flows, ASTRONUM 2017, vol. 1031, no. 1, 2018.
http://dx.doi.org/10.1088/1742-6596/1031/1/012012---------- VANCOUVER ----------
Vigh, C.D., Gonzalez, R., Rial, D. Exploring the Kipenhahn-Schlüter model. J. Phys. Conf. Ser. 2018;1031(1).
http://dx.doi.org/10.1088/1742-6596/1031/1/012012