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Abstract:

Using methods of non-equilibrium thermodynamics that extend and generalize the MHD energy principle of Bernstein et al. (1958, Proc. Roy. Soc. A, 244, 17) we develop a formalism in order to analyze the stability properties of prominence models considered as dissipative states i.e. states far form thermodynamic equilibrium. As an example, the criterion is applied to the Kippenhahn-Schlüter model (hereafter K-S) considering the addition of dissipative terms in the coupled system of equations: the balance of energy equation and the equation of motion. We show from this application, that periods corresponding to typical oscillations of the chromosphere and photosphere (3 and 5 min respectively), that were reported as observations of the prominence structure, can be explained as internal modes of the prominence itself. This is an alternative explanation to the one that supposes that the source of these perturbations are the cold foot chromospheric and photospheric basis.

Registro:

Documento: Artículo
Título:Stability analysis of quiescent prominences using thermodynamic irreversible energy principles
Autor:Costa, A.; González, R.; Schifino, A.C.S.
Filiación:Inst. Astronomia Y Fis. del Espacio, CONICET, 1428 Buenos Aires, Argentina
Departamento de Física, FCEyN, UBA, Argentina
Departamento de Física, Facultad de Ciencias, Facultad de Ingeniería, UR, Uruguay
Palabras clave:Instabilities; Sun: prominences; Waves; Energy dissipation; Equations of motion; Magnetohydrodynamics; Perturbation techniques; Thermodynamic stability; Thermodynamics; Chromosphere; Photosphere; Quiescent prominences; Thermodynamic irreversible energy principles; Astrophysics
Año:2004
Volumen:427
Número:1
Página de inicio:353
Página de fin:361
DOI: http://dx.doi.org/10.1051/0004-6361:20041260
Título revista:Astronomy and Astrophysics
Título revista abreviado:Astron. Astrophys.
ISSN:00046361
CODEN:AAEJA
PDF:https://bibliotecadigital.exactas.uba.ar/download/paper/paper_00046361_v427_n1_p353_Costa.pdf
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v427_n1_p353_Costa

Referencias:

  • Anzer, U., (1969) Sol. Phys., 8, p. 37
  • Balthasar, H., Wiehr, E., Schleicher, H., Wohl, H., (1993) A&A, 277, p. 635
  • Blanco, S., Bochialini, K., Costa, A., Rovira, M., Vial, J.-C., (1999) Sol. Phys., 186, p. 281
  • Bénard, H., (1900) Revue Gen. Sci. Pur. Appl., 11, p. 1261
  • Bernstein, I.B., Frieman, E.A., Kruskal, M.D., Kulsrud, R.M., (1958) Proc. Roy. Soc. A, 244, p. 17
  • Bocchialini, K., Costa, A., Domenech, G., Rovira, M., Vial, J.-C., (2001) Sol. Phys., 199 (1), p. 133
  • Chiuderi, C., Van Hoven, G., (1979) ApJ, 232, pp. L69
  • Costa, A., Ferro Fontán, C., Gonzalez, R., Sicardi Schifino, A.C., (2001) Physica A, 300, p. 468
  • Galindo Trejo, J., (1987) Sol. Phys., 108 (2), p. 265
  • Galindo Trejo, J., (1989) Rev. Mex. Astron. Astrofis., 17, p. 47
  • Galindo Trejo, J., Schindler, K., (1984) ApJ, 277, p. 422
  • Glansdorff, P., Nicolis, G., Prigogine, I., (1974) Proc. Nat. Acad. Sci., 71, p. 197
  • Glansdorff, P., Prigogine, I., (1971) Structure Stability and Fluctuations, , New York: Wiley Interscience
  • Gouttebroze, P., Vial, J.-C., Bocchialini, K., Lemaire, P., Leibacher, J.W., (1999) Sol. Phys., 184, p. 253
  • Graham, R., (1978) Lect. Notes Phys., 84, p. 83
  • Halberstadt, G., Goedbloed, J.P., (1993) A&A, 280, p. 647
  • Keizer, J., (1976) J. Chem. Phys., 69, p. 2609
  • Kennedy, D.C., Bludman, S.A., (1997) ApJ, 484, p. 329
  • Kippenhahn, R., Schluter, A., (1957) Z. Astrophys., 43, p. 36
  • Lavenda, B.H., (1985) Nonequilibium Statistical Thermodynamics, , Chicehster: Wiley-Interscience
  • Keizer, J., (1987) Statistical Thermodynamics of Nonequilibium Processes, , New York: Springer-Verlag
  • Lavenda, B.H., (1993) Thermodynamics of Irreversible Processes, , New York: Dover
  • Ledoux, P., Walraven, N., Variable stars (1958) Handbuch, Phys., 51, p. 353
  • Lefschetz, S., (1977) Differential Equations: Geometric Theory, , New York: Dover
  • Lerche, I., Low, B.C., (1980) Sol. Phys., 67, p. 229
  • Lerche, I., Low, B.C., (1981) Sol. Phys., 69, pp. L327
  • Low, B.C., Wu, S.T., (1981) ApJ, 248, p. 335
  • Manneville, P., (1987) Dissipative Structures and Weak Turbulence, , 1.2 Chap. 3 (New York: Academic Press)
  • Nagablushana, B.S., (1998) A&A, 333, p. 1043
  • Nicolis, G., Prigogine, I., (1979) Proc. Acad. Sci., 76, p. 6060
  • Oliver, R., (1999) The 9th European Meeting on Solar Physics ESA SSP-448, p. 425
  • Oliver, R., Ballester, J.L., (1996) ApJ, 456, p. 3930
  • Onsager, L., (1931) Phys. Rev., 37, p. 405
  • Onsager, L., Machlup, S., (1953) Phys. Rev., 91, p. 1505
  • Priest, E., (1982) Solar Magneto-hydrodynamcis, , Boston: Publishing Company
  • Prigogine, I., (1967) Thermodynamics of Irreversible Processes, , New York: Wiley Interscience
  • Rayleigh, L., (1916) Phil. Mag., 32, p. 529
  • Régnier, S., Solomon, J., Vial, J.-C., Amari, D., Mickey, T., (1999) The 9th European Meeting on Solar Physics, ESA SSP-448, p. 519
  • Sicardi Schifino, A.C., Costa, A., Ferro Fontán, C., (1991) J. Math. Phys., 32, p. 1350
  • Sicardi Schifino, A.C., Ferro Fontán, C., (1985) Phys. Lett. A, 113, p. 263
  • Sicardi Schifino, A.C., Ferro Fontán, C., (1989) Phys. Lett. A, 134, p. 371
  • Sicardi Schifino, A.C., Ferro Fontán, C., González, R., Costa, A., (2004) Physica A, 334, p. 201
  • Sicardi Schifino, A.C., Gonzalez, R., Ferro Fontán, C., (1989) Phys. Lett. A, 137, p. 44
  • Tasso, H., (1975) Plasma Phys., 17, p. 1131
  • Vial, J.-C., Solar prominence diagnostic (1998) IAU Coll., 167
  • Webb, D., Rust, D., Scmieder, B., ASPCS, 150, p. 175
  • Zweibel, E., (1981) ApJ, 249, p. 731
  • Zweibel, E., (1982) ApJ, 258, pp. L53

Citas:

---------- APA ----------
Costa, A., González, R. & Schifino, A.C.S. (2004) . Stability analysis of quiescent prominences using thermodynamic irreversible energy principles. Astronomy and Astrophysics, 427(1), 353-361.
http://dx.doi.org/10.1051/0004-6361:20041260
---------- CHICAGO ----------
Costa, A., González, R., Schifino, A.C.S. "Stability analysis of quiescent prominences using thermodynamic irreversible energy principles" . Astronomy and Astrophysics 427, no. 1 (2004) : 353-361.
http://dx.doi.org/10.1051/0004-6361:20041260
---------- MLA ----------
Costa, A., González, R., Schifino, A.C.S. "Stability analysis of quiescent prominences using thermodynamic irreversible energy principles" . Astronomy and Astrophysics, vol. 427, no. 1, 2004, pp. 353-361.
http://dx.doi.org/10.1051/0004-6361:20041260
---------- VANCOUVER ----------
Costa, A., González, R., Schifino, A.C.S. Stability analysis of quiescent prominences using thermodynamic irreversible energy principles. Astron. Astrophys. 2004;427(1):353-361.
http://dx.doi.org/10.1051/0004-6361:20041260