| dc.creator | Gómez, D | |
| dc.creator | Sicardi Schifino, A. | |
| dc.creator | Ferro Fontán, C. | |
| dc.date | 1987 | |
| dc.date | 2022-06-09T14:59:50Z | |
| dc.date.accessioned | 2023-07-15T06:58:27Z | |
| dc.date.available | 2023-07-15T06:58:27Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/137617 | |
| dc.identifier | issn:1669-9521 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7478726 | |
| dc.description | The coronal loops confine a low density (n=10¹⁰ cm⁻³) and hot plasma (T=10⁶ K), whose ends interact with the much denser and hotter photospheric fluid. The linear stability of the dynamical and thermal equilibria of the coronal plasma is analyzed. A formalism based on methods of irreversible thermodynamics was used, which systematically builds up (whenever it is possible) a variational principle for studying the stability. The stability conditions derived in this work are compared with results available in the literature, which were obtained by standard stability methods. | |
| dc.description | Asociación Argentina de Astronomía | |
| dc.format | application/pdf | |
| dc.language | es | |
| dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
| dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
| dc.subject | Astronomía | |
| dc.subject | Galaxias | |
| dc.title | Thermal stability analysis of coronal loops | |
| dc.type | Articulo | |
| dc.type | Comunicacion | |
