• DocumentCode
    1792888
  • Title

    Numerical simulations on self-focusing and filamentation of multi-terawatt picosecond CO2-laser pulse in air

  • Author

    Zemlyanov, Alexander A. ; Geints, Yuri E.

  • Author_Institution
    Wave Propagation Div., V.E. Zuev Inst. of Atmos. Opt., Tomsk, Russia
  • fYear
    2014
  • fDate
    June 30 2014-July 4 2014
  • Firstpage
    1
  • Lastpage
    1
  • Abstract
    At present, CO2-laser is the only actual source of high-power 10-μm radiation traditionally used in various atmospheric optics applications where the extreme power at joule energy in laser pulse is crucial. The advent of high-pressure CO2:N2O gas mixture lasers involves a significant increase of the output pulse power up to multiterawatt level due to laser pulse shortening down to few picoseconds and even to hundreds of femtoseconds. The mid-IR spectral region is attractive because at the relatively low continual absorption the atmosphere can linearly transfer light power up to several terawatts. Further increase of laser power gives rise to nonlinear losses of propagating radiation, which is mostly due to ionization and optical breakdown of air against the background of Kerr self-focusing and filamentation of a laser beam.
  • Keywords
    carbon compounds; gas lasers; high-speed optical techniques; laser beams; light propagation; numerical analysis; optical Kerr effect; optical losses; CO2; Kerr self-focusing; absorption; atmospheric optics applications; high-power radiation; high-pressure gas mixture lasers; joule energy; laser beam filamentation; laser power; light power; mid-IR spectral region; multiterawatt level; multiterawatt picosecond CO2-laser pulse; nonlinear losses; numerical simulations; optical breakdown; output pulse power; propagating radiation; wavelength 10 mum; Lead;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Laser Optics, 2014 International Conference
  • Conference_Location
    Saint Petersburg
  • Print_ISBN
    978-1-4799-3884-1
  • Type

    conf

  • DOI
    10.1109/LO.2014.6886337
  • Filename
    6886337