Artículo

Estamos trabajando para incorporar este artículo al repositorio
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

We present a complete atomic model for Si I line synthesis. We study how the computed profiles of two blue lines of this atom are influenced by the choice of the atomic parameters and find that, although several cross sections are not known accurately, the line profiles do not depend strongly on them and are therefore useful as diagnostics of the atmospheric structure. We study which transitions need not be included in the model, in order to reduce as much as possible the computing time. We compare the profiles computed for a standard model of the quiet solar atmosphere with the observations and find very good agreement. We confirm that irradiation by UV lines originating in the transition region above sunspot umbrae or plages strongly enhances the continuum between 1300 and 1700 Å, which is due to Si I bound-free transitions. If line fluxes typical of the impulsive phase of flares are assumed, the line profiles are also affected.

Registro:

Documento: Artículo
Título:Blue lines as chromospheric diagnostics: The Si I lines at 3906 and 4103 Å
Autor:Cincunegui, C.; Mauas, P.J.D.
Filiación:Inst. Astronomia Fis. Espacio (IAFE), Casilla de Correo 67, Sucursal 28, Buenos Aires 1428, Argentina
Palabras clave:Atomic processes; Line: formation; Line: profiles; Stars: chromospheres; Sun: chromosphere
Año:2001
Volumen:552
Número:2 PART 1
Página de inicio:877
Página de fin:888
DOI: http://dx.doi.org/10.1086/320566
Título revista:Astrophysical Journal
Título revista abreviado:Astrophys. J.
ISSN:0004637X
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v552_n2PART1_p877_Cincunegui

Referencias:

  • Andretta, V., Doyle, J.G., Byrne, P.B., (1997) A&A, 322, p. 266
  • Asplund, M., (2000) A&A, 359, p. 755
  • Avrett, E.H., (1985) Chromospheric Diagnostics and Modeling, p. 67. , ed. B. W. Lites (Sunspot: NSO)
  • Avrett, E.H., Loeser, R., (1992) ASP Conf. Ser., 26, p. 489. , Cool Stars, Stellar Systems, and the Sun: 7th Cambridge Workshop, ed. M. S. Giampapa & J. A. Bookbinder (San Francisco: ASP)
  • Avrett, E.H., Machado, M.E., Kurucz, R.L., (1986) The Lower Chromosphere of Solar Flares, p. 216. , ed. D. F. Neidig (Sunspot: NSO)
  • Baumüller, D., Gehren, T., (1996) A&A, 307, p. 961
  • Becker, U., (1980) Phys. Lett., 76, p. 125
  • Cauzzi, G., (1995) A&A, 299, p. 611
  • (1996) A&A, 306, p. 625
  • Cram, L.E., Mullan, D.J., (1979) ApJ, 234, p. 579
  • Cunto, W., (1993) A&A, 275, pp. L5
  • Deridder, G., Van Rensbergen, W., (1976) A&AS, 23, p. 147
  • Doyle, J.G., Phillips, K.J.H., (1992) A&A, 257, p. 773
  • Falchi, A., Mauas, P.J.D., (1998) A&A, 336, p. 281
  • (1999) Magnetic Fields and Solar Processes, p. 779. , (Noordwijk: ESA)
  • Freund, R.S., (1990) Phys. Rev. A, 41, p. 3575
  • Ganas, P.S., (1999) A&AS, 138, p. 323
  • Giampapa, M.S., Worden, S.P., Linsky, J.L., (1982) ApJ, 258, p. 740
  • Grevesse, N., (1991) A&A, 242, p. 488
  • Griem, H.R., (1974) Spectral Line Broadening by Plasmas, , New York: Academic Press
  • Hibbert, A., (1979) J. Phys. (Paris), C1 (SUPPL. 2), p. 40
  • Hoffman, W., (1969) Z. Naturforschung, 24, p. 990
  • Houdebine, E.R., Doyle, J.G., (1994) A&A, 289, p. 185
  • Iglesias, C.A., Rogers, F.J., Wilson, B.G., (1992) Rev. Mexicana Astron. Astrofis., 23, p. 9
  • Kupka, F., Piskunov, N.E., Ryabchikova, T.A., Stempels, H.C., Weiss, W.W., (1999) A&AS, 138, p. 119
  • Kurucz, R.L., (1991) Precision Photometry: Astrophysics of the Galaxy, p. 441. , ed. A. G. Davis Philip, A. R. Upgren, & K. A. Janes (Schenectady: L. Davis Press)
  • Lemke, M., Holweger, H., (1987) A&A, 173, p. 375
  • Machado, M.E., Avrett, E.H., Vernazza, J., Noyes, R.W., (1980) ApJ, 242, p. 336
  • Machado, M.E., Hénoux, J.C., (1982) A&A, 108, p. 61
  • Machado, M.E., Mauas, P.J.D., (1986) Rapid Fluctuations in Solar Flares, p. 271. , ed. B. R. Dennis, A. Kiplinger, & L. Orwig (Washington: NASA)
  • Maltby, P., (1986) ApJ, 306, p. 284
  • Mauas, P.J.D., (1993) ApJ, 414, p. 928
  • (2000) ApJ, 539, p. 858
  • Mauas, P.J.D., Avrett, E.H., Loeser, R., (1988) ApJ, 330, p. 1008
  • Mauas, P.J.D., Falchi, A., (1994) A&A, 281, p. 129
  • (1996) A&A, 310, p. 245
  • Mauas, P.J.D., Falchi, A., Pasquini, L., Pallavicini, R., (1997) A&A, 326, p. 249
  • Mauas, P.J.D., Machado, M.E., Avrett, E.H., (1990) ApJ, 360, p. 715
  • Mendoza, C., Zeippen, C.J., (1988) J. Phys. B, 21, p. 259
  • Meyer, J., Beck, R.J., (1970) A&A, 8, p. 93
  • Mihalas, D., (1970) Stellar Atmospheres, , San Francisco: Freeman
  • Morton, D.C., (1991) ApJS, 77, p. 119
  • Mukherjee, P.K., Ohno, K., (1989) Phys. Rev. A, 40, p. 1753
  • Nahar, S.N., (1993) Phys. Scr., 48, p. 297
  • Nahar, S.N., Pradhan, A.K., (1993) Phys. Rev. A, 26, p. 1109
  • Neckel, H., (1999) Sol. Phys., 184, p. 421
  • O'Brien, T.R., Lawler, J.E., (1991) Phys. Rev. A, 44, p. 7134
  • Piskunov, N.E., Kupka, F., Ryabchikova, T.A., Weiss, W.W., Jeffery, C.S., (1995) A&AS, 112, p. 525
  • Ryabchikova, T.A., Piskunov, N.E., Stempels, H.C., Kupka, F., Weiss, W.W., (1999) Phys. Scr., 83, p. 162
  • Saloman, E.B., (1990) Spectrochim. Acta, 45, p. 37
  • Sandlin, G.D., (1986) ApJS, 61, p. 801
  • Savage, B.D., Lawrence, G.M., (1966) ApJ, 146, p. 940
  • Smith, K., Henry, R.J.W., Burke, P.G., (1967) Phys. Rev., 157, p. 51
  • Smith, P.L., (1987) ApJ, 322, p. 573
  • Thatcher, J.D., Robinson, R.D., Rees, D.E., (1991) MNRAS, 250, p. 14
  • Van Regemorter, H., (1962) ApJ, 136, p. 906
  • Vernazza, J.E., Avrett, E.H., Loeser, R., (1973) ApJ, 184, p. 605
  • (1976) ApJS, 30, p. 1. , (VAL76)
  • (1981) ApJS, 45, p. 635
  • Verner, D.A., Barthel, P.D., Tytler, D., (1994) A&AS, 108, p. 287
  • Wiese, W.L., Fuhr, J.R., (1999) NIST Atomic Spectra Database

Citas:

---------- APA ----------
Cincunegui, C. & Mauas, P.J.D. (2001) . Blue lines as chromospheric diagnostics: The Si I lines at 3906 and 4103 Å. Astrophysical Journal, 552(2 PART 1), 877-888.
http://dx.doi.org/10.1086/320566
---------- CHICAGO ----------
Cincunegui, C., Mauas, P.J.D. "Blue lines as chromospheric diagnostics: The Si I lines at 3906 and 4103 Å" . Astrophysical Journal 552, no. 2 PART 1 (2001) : 877-888.
http://dx.doi.org/10.1086/320566
---------- MLA ----------
Cincunegui, C., Mauas, P.J.D. "Blue lines as chromospheric diagnostics: The Si I lines at 3906 and 4103 Å" . Astrophysical Journal, vol. 552, no. 2 PART 1, 2001, pp. 877-888.
http://dx.doi.org/10.1086/320566
---------- VANCOUVER ----------
Cincunegui, C., Mauas, P.J.D. Blue lines as chromospheric diagnostics: The Si I lines at 3906 and 4103 Å. Astrophys. J. 2001;552(2 PART 1):877-888.
http://dx.doi.org/10.1086/320566