Abstract
A new investigation of the presence of SiH lines in the solar disk spectrum has been performed. It may be concluded that molecular absorption lines of SiH are present in the disk spectrum with maximum equivalent widths of about 2 mÅ. A value of the oscillator strength of SiH has been derived (f 00 = 0.0008 ± 0.0004).
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Delbouille, L., and Roland, G.: 1969, Phil. Trans. Roy. Soc. London A264, 171.
Delbouille, L., Neven, L., and Roland, G.: 1963, J. Quant. Spectr. Radiative Transfer 3, 189.
De Witt Coleman, C., Bozman, W. R., and Meggers, W. F.: 1960, ‘Table of Wavenumbers, vol. 1 (2000 to 7000 Å)’, Natl. Bur. Std. Monograph 3.
Douglas, A. E.: 1957, Can. J. Phys. 35, 71.
Jackson, C. V.: 1930, Proc. Roy. Soc. A126, 373.
Klynning, L., and Lindgren, B.: 1967, Arkiv Fysik 33, 73.
Minnaert, M. G. J., Mulders, G. F. W., and Houtgast, J.: 1940, Photometric Atlas of the Solar Spectrum, Amsterdam.
Moore, C. E., Minnaert, M. G. J., and Houtgast, J.: 1966, ‘Second Revision of Rowland's Preliminary Table of Solar Spectrum Wavelengths’, Natl. Bur. Std. Monograph 61.
Moore-Sitterly, C. E.: 1966, in Proceedings of the Meeting on Sunspots (Firenze, 1964), Vol. 2, p. 181.
Mulliken, R. S.: 1931, Phys. Rev. 37, 733.
Pearse, R. W. B.: 1931, Publ. Am. Astron. Soc. 7, 12.
Rochester, G. D.: 1936, Z. Phys. 101, 769.
Russell, H. N., and Bowen, I. S.: 1929, Astrophys. J. 69, 196.
Schadee, A.: 1964, Bull. Astron. Inst. Neth. 17, 311.
Schadee, A.: 1967, J. Quant. Spectr. Radiative Transfer 7, 169.
Verma, R. D.: 1965, Can. J. Phys. 43, 2136.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Sauval, A.J. Identification of SiH lines in the solar disk spectrum. Sol Phys 10, 319–329 (1969). https://doi.org/10.1007/BF00145520
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00145520