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Discussion on New Instrumental Techniques

  • A. Unsöld
  • F. Roddier
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 2)

Abstract

Our experiment has yet been described in a Phys. Rev. Letter.1 — The light to be analyzed excites the optical resonance of the vapor of a metal. The intensity of the light re-emitted by the vapor, proportional to the incident intensity, is measured at right angle to the exciting beam by a photomultiplier. The scattering frequency is shifted by applying a magnetic field and by observing one σ component (through a circular analyzer). The variation of intensity of re-emitted light as a function of the field gives the profile of the exciting light.

Keywords

Solar Spectrum Atomic Beam Solar Rotation Instrumental Technique Exciting Light 
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.

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References

  1. 1.
    Blamont, J. E., Roddier, F.: 1961, Phys. Rev. Letters 7, 437.ADSCrossRefGoogle Scholar
  2. 2.
    Olson, E. C.: 1962, Astrophys. J. 136, 946.ADSCrossRefGoogle Scholar
  3. 3.
    Higgs, L. A.: 1962, Mon. Not. Roy. Astron. Soc. 124, 51.ADSGoogle Scholar
  4. 4.
    Adam, M. G.: 1948, Mon. Not. Roy. Astron. Soc. 108, 446.ADSGoogle Scholar
  5. 5.
    Adam, M. G.: 1959, Mon. Not. Roy. Astron. Soc. 119, 460.ADSGoogle Scholar
  6. 6.
    Hart, A. B. : 1954, Mon. Not. Roy. Astron. Soc. 114, 17.ADSGoogle Scholar
  7. 7.
    de Jager, C.: 1959, Handbuch der Physik 52, 338.Google Scholar
  8. 1.
    Migeotte, M., Neven, L., Swensson, J.: 1956, 1957; The Solar Spectrum from 2.8 to 23.7 Microns) Part I, Photometric Atlas, Part II, Measures and Identifications; Mém. Soc. Roy. Sci. Liège, Special Vol. 1 and 2.Google Scholar
  9. 2.
    Delbouille, L. and Roland, G.: 1963, Photometric Atlas of the Solar Spectrum from λ 7488 to λ 12 016, Mém. Roy. Soc. Sci. Liège, Special Vol. 4.Google Scholar
  10. 3.
    Babcock, H. D. and Moore, C. E.: 1947, ‘The Solar Spectrum 6600 to 13495’, Carnegie Inst. Publ. 579, Washington.Google Scholar
  11. 4.
    Delbouille, L., Neven, L., and Roland, G.: 1963, J. Quant. Spectr. Rad. Transfer 3, 189.ADSCrossRefGoogle Scholar
  12. 5.
    Minnaert, M., Mulders, G., and Houtgast, J.: 1940, Photometric Atlas of the Solar Spectrum from λ 3612 to λ 8771, Utrecht.Google Scholar
  13. 6.
    Bruckner, G.: 1960, Photometric Atlas of the Near Ultraviolet Solar Spectrum 2988 A to 3629 Å, Göttingen.Google Scholar
  14. 7.
    Mohler, O.: Private Communication.Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1965

Authors and Affiliations

  • A. Unsöld
    • 1
  • F. Roddier
    • 2
  1. 1.University of KielKielGermany
  2. 2.Observatoire de MarseilleFrance

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