• DocumentCode
    1863041
  • Title

    Stimulated backscattering from the stratosphere: a useful laser guide star?

  • Author

    Hellwarth, R.W. ; Partanen, J.P. ; Nansheng Tang

  • Author_Institution
    Dept. of Electr. Eng. & Phys., Univ. of Southern California, Los Angeles, CA, USA
  • fYear
    1999
  • fDate
    28-28 May 1999
  • Firstpage
    95
  • Abstract
    Summary form only given. Lasers have been employed to create artificial "laser guide stars" (LGS) by exciting various emissions from the upper atmosphere that are bright enough to correct infrared images. Unfortunately, the atmosphere trembles in such a manner that using adaptive optics techniques to correct distortions in blue starlight requires orders-of-magnitude brighter guide stars than any existing LGS. The authors report studies which indicate that stimulated backscattering of a laser focused into the stratosphere, above the atmospheric turbulence, can create such an enormously brighter guide star. There, the atmospheric excitation with the greatest stimulated gain is the S(6) rotational Raman transition of N/sub 2/. Extrapolation to the stratosphere suggests that a one-quarter joule, 352 nm, pulse focused into the stratosphere by the Keck telescope would surpass the S(6) stimulated backscattering threshold.
  • Keywords
    adaptive optics; artificial guide stars; backscatter; laser beam applications; stratosphere; 0.25 J; 352 nm; N/sub 2/; N/sub 2/ S(6) rotational Raman transition; adaptive optics techniques; atmospheric excitation; atmospheric turbulence; blue starlight; bright laser guide star; stimulated backscattering; stratosphere; Adaptive optics; Backscatter; Extrapolation; Focusing; Infrared imaging; Laser excitation; Laser noise; Laser transitions; Optical distortion; Terrestrial atmosphere;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Lasers and Electro-Optics, 1999. CLEO '99. Summaries of Papers Presented at the Conference on
  • Conference_Location
    Baltimore, MD, USA
  • Print_ISBN
    1-55752-595-1
  • Type

    conf

  • DOI
    10.1109/CLEO.1999.833931
  • Filename
    833931