• DocumentCode
    1094493
  • Title

    A comparison of the Cassegrain and other beam expanders in high-power pulsed dye lasers

  • Author

    Trebino, Rick ; Roller, James P. ; Siegman, Anthony E.

  • Author_Institution
    Standford University, Standford, CA, USA
  • Volume
    18
  • Issue
    8
  • fYear
    1982
  • fDate
    8/1/1982 12:00:00 AM
  • Firstpage
    1208
  • Lastpage
    1213
  • Abstract
    We have constructed and compared high peak power YAG-pumped dye lasers using a variety of beam expansion methods, particularly the Cassegrainian telescope, grazing-incidence, and achromaticprism beam expander designs. We find that the Cassegrainian design offers a modest advantage over the conventional Hänsch or refractive telescope design in larger magnification and hence, narrower linewidth, while retaining several inherent drawbacks in cost, alignment difficulty, and amplified spontaneous emission (ASE) problems. New problems specific to the Cassegrainian design in high-power operation include limited wavelength range of the telescope secondary and a severe diffraction grating damage mechanism during alignment. We conclude that, on the whole, the Hänsch and Cassegrainian designs offer roughly equal performance. By comparison, the grazing-incidence design offers significant advantages in cost, ease of alignment, and linewidth without an etalon, but with reductions in efficiency, power output, and in some cases, wavelength stability. Our final judgment is that for high-power multimode operation, the four-prism achromatic beam expander is generally superior to the other designs. For single-mode operation, however, the prism design is rivaled by several ingenious grazing-incidence variations.
  • Keywords
    Dye lasers; Pulsed lasers; Costs; Diffraction; Laser beams; Laser modes; Optical design; Optical pulses; Optical refraction; Power lasers; Spontaneous emission; Telescopes;
  • fLanguage
    English
  • Journal_Title
    Quantum Electronics, IEEE Journal of
  • Publisher
    ieee
  • ISSN
    0018-9197
  • Type

    jour

  • DOI
    10.1109/JQE.1982.1071685
  • Filename
    1071685