Abstract
The solar spectrum at 3261 Å has been studied using the spectrograph at the Oslo Solar Observatory. From analysis of this wavelength region and recent results at 5085 Å, a solar cadmium abundance log N Cd = 1.86 ± 0.15 is obtained.
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Byron, F. W., McDermott, M. N., and Novick, R.: 1964, Phys. Rev. 134, A615.
Claas, W. J.: 1949, K. Ned. Akad. Wet. Proc. Sect. Sci. 52, No. 5.
Corliss, C. H. and Bozman, W. R.: 1962, N.B.S. Monograph No. 53.
Gingerich, O. and de Jager, C.: 1968, Solar Phys. 3, 5.
Goldberg, L., Müller, A. E., and Aller, L. H.: 1960, Astrophys. J. Suppl. Ser. 5, 1.
Grevesse, N. and Blanquet, G.: 1969, Solar Phys. 8, 5.
Hauge, Ö. and Engvold, O.: 1968, Astrophys. Letters 2, 235.
Hull, R. J. and Stroke, H. H.: 1963, J. Opt. Soc. Am. 53, 1147.
Lambert, D. L. and Mallia, E. A.: 1968, Solar Phys. 3, 499.
Lambert, D. L., Mallia, E. A., and Warner, B.: 1969, Monthly Notices Roy. Astron. Soc. 142, 71.
M.I.T. Wavelength Tables. A Publication of the Technology Press, M.I.T., 1939.
Moore, C. E., Minnaert, M. G. J., and Houtgast, J.: 1966, N.B.S. Monograph No. 61.
Müller, E. A.: 1968, in Origin and Distribution of the Elements (ed. by L. H. Ahrens), Pergamon Press, Oxford.
Righini, A. and Rigutti, M.: 1966, Ann. Astrophys. 29, 379.
Wallerstein, G.: 1966, Icarus 5, 75.
Warner, B.: 1968, Monthly Notices Roy. Astron. Soc. 140, 53.
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Hauge, Ø. The abundance of cadmium in the solar atmosphere. Sol Phys 10, 315–318 (1969). https://doi.org/10.1007/BF00145519
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DOI: https://doi.org/10.1007/BF00145519