Advertisement

Solar Physics

, Volume 41, Issue 1, pp 43–52 | Cite as

The solar lithium abundance

I: Observations of the solar lithium feature at λ6707.8 Å
  • James W. Brault
  • Edith A. Müller
Article

Abstract

A detailed observational study of the solar photospheric lithium feature has been carried out with emphasis on center-limb observations, continuum location, possible effects of telluric lines, effects of blending by atomic and molecular lines, and decomposition of the solar spectrum around λ6707 Å.

Keywords

Lithium Observational Study Solar Spectrum Molecular Line Continuum Location 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Brault, J. W. and White, O. R.: 1971, Astron. Astrophys. 13, 169.Google Scholar
  2. Brault, J. W., Slaughter, C. D., Pierce, A. K., and Aikens, R. S.: 1971, Solar Phys. 18, 366.Google Scholar
  3. Daehler, M.: 1967, Astrophys. J. 150, 667.Google Scholar
  4. Grevesse, N.: 1968, Solar Phys. 5, 159.Google Scholar
  5. Holweger, H.: 1967, Z. Astrophys. 65, 365.Google Scholar
  6. Mutschlecner, J. P.: 1963, Thesis, University of Michigan.Google Scholar
  7. Peach, J. V.: 1968, Monthly Notices Roy. Astron. Soc. 139, 403.Google Scholar
  8. Swensson, J. W., Benedict, W. S., Delbouille, L., and Roland, G.: 1970, Mem. Soc. Roy. Sci. Liège 5.Google Scholar
  9. Tech, J. L.: 1971, Nat. Bur. Stand. Monograph 119, 170.Google Scholar

Copyright information

© D. Reidel Publishing Company 1975

Authors and Affiliations

  • James W. Brault
    • 1
  • Edith A. Müller
    • 2
  1. 1.Kitt Peak National ObservatoryTucsonU.S.A.
  2. 2.Observatoire de GenèveSwitzerland

Personalised recommendations