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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Bibliographic Details
Published in:Journal of physics. Conference series 2018-05, Vol.1031 (1), p.12012
Main Authors: Vigh, Carlos D., Gonzalez, Rafael, Rial, Diego
Format: Article
Language:English
Subjects:
Heat balance
Physics
Prominences
Solar prominences
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Summary: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.
ISSN:1742-6588
1742-6596
DOI:10.1088/1742-6596/1031/1/012012