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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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_17426588_v1031_n1_p_Vigh |
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todo:paper_17426588_v1031_n1_p_Vigh2023-10-03T16:30:27Z Exploring the Kipenhahn-Schlüter model Vigh, C.D. Gonzalez, R. Rial, D. 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. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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 Vigh, C.D. Gonzalez, R. Rial, D. 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. |
| format |
CONF |
| author |
Vigh, C.D. Gonzalez, R. Rial, D. |
| author_facet |
Vigh, C.D. Gonzalez, R. Rial, D. |
| author_sort |
Vigh, C.D. |
| 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 |
| url |
http://hdl.handle.net/20.500.12110/paper_17426588_v1031_n1_p_Vigh |
| work_keys_str_mv |
AT vighcd exploringthekipenhahnschlutermodel AT gonzalezr exploringthekipenhahnschlutermodel AT riald exploringthekipenhahnschlutermodel |
| _version_ |
1807323966781521920 |