Abstract
Center-to-limb measurements of the Ca i λ6573 intercombination line and the Ca ii λ7324 forbidden line are compared with synthetic profiles based on a simple representation of the non-LTE Ca-Ca+ ionization equilibrium. The effects of photoionizations from low lying excited states of neutral calcium are found to reduce the sensitivity of the λ6573 center-to-limb behavior as a thermal structure diagnostic. The synthetic center-to-limb behavior is also sensitive to uncertainties in the nonthermal broadening. Nevertheless, the measured center-to-limb behavior of λ6573 favors a ‘cool’ photospheric model similar to the Vernazza, Avrett, and Loeser model M over hotter models based on the Ca ii K wings. The non-LTE calcium abundance obtained from the disk center equivalent widths of λ6573 and λ7324 using the best fit model is A Ca≅2.1±0.2 × 10-6 (by number relative to hydrogen). Applications of these lines as diagnostics of the Ca-Ca+ ionization equilibrium in other stars are briefly discussed.
Similar content being viewed by others
References
Auer, L. H.: 1976, J. Quant. Spectrosc, Radiat. Transf. 16, 931.
Auer, L. H., Heasley, J. N., and Milkey, R. W.: 1972, Kitt Peak National Observatory Contribution No. 555.
Avrett, E. H.: 1977a, private communication.
Avrett, E. H.: 1977b, in The Solar Output and Its Variation, Colorado Assoc. Univ. Press, Boulder, p. 327.
Ayres, T. R.: 1977a, Astrophys. J. 213, 296.
Ayres, T. R.: 1977b, Astrophys. J. 214, 905.
Ayres, T. R.: 1978a, Solar Phys. 57, 19.
Ayres, T. R.: 1978b, Astrophys. J. (in press).
Brault, J. and Tèsterman, L.: 1972, Kitt Peak Solar Atlas, preliminary edition, Kitt Peak National Observatory, Tucson.
Brault, J. W. and White, O. R.: 1971, Astron. Astrophys. 13, 169.
Brault, J. W., Slaughter, C. D., Pierce, A. K., and Aikens, R. S.: 1971, Solar Phys. 18, 366.
Carter, V. L., Hudson, R. D., and Brieg, E. L.: 1971, Phys. Rev. A4, 821.
Crandall, D. H., Dunn, G. H., Gallagher, A., Hummer, D. G., Kunasz, C. V., Leep, D., and Taylor, P. O.: 1974, Astrophys. J. 191, 789.
Evans, J. C. and Testerman, L.: 1975, Solar Phys. 45, 41.
House, L. L.: 1964, Astrophys. J. Suppl. 8, 307.
Kelm, S. and Schlüter, D.: 1962, Z. Astrophys. 56, 78.
Kneer, F.: 1975, Astrophys. J. 200, 367.
Linsky, J. L. and Ayres, T. R.: 1978, Astrophys. J. 220, 619.
Milkey, R. W.: 1976, in Interpretation of Atmospheric Structure in the Presence of Inhomogeneities, University of Sydney, Sydney, p. 55.
Okuno, Y.: 1971, J. Phys. Soc. Japan 31, 1189.
Ramsey, L. W.: 1977, Astrophys. J. 215, 827.
Schorn, R. A., Young, A. T., and Barker, E. S.: 1975, Solar Phys. 43, 9.
Smith, G.: 1967, Proc. Roy. Soc. London A297, 288.
Travis, L. D. and Matsushima, S.: 1968, Astrophys. J. 154, 689.
Ulmschneider, P.: 1974, Solar Phys. 39, 327.
van Regemorter, H.: 1962, Astrophys. J. 136, 906.
Vernazza, J. E., Avrett, E. H., and Loeser, R.: 1973, Astrophys. J. 184, 605.
Vernazza, J. E., Avrett, E. H., and Loeser, R.: 1976, Astrophys. J. Suppl. 30, 1 (VAL).
Withbroe, G. L.: 1977, Center for Astrophysics, preprint No. 524.
Author information
Authors and Affiliations
Additional information
Visiting Astronomer, Kitt Peak National Observatory.
Operated by the Association of Universities for Research in Astronomy, Inc. under contract with the National Science Foundation.
Rights and permissions
About this article
Cite this article
Ayres, T.R., Testerman, L. The center-to-limb behavior of Ca i λ6573 and [Ca ii] λ7324. Sol Phys 60, 19–29 (1978). https://doi.org/10.1007/BF00152329
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00152329