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Light self-focusing in the atmosphere: thin window model.

Irina A Vaseva1, Mikhail P Fedoruk1,2, Alexander M Rubenchik3

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Ultra-high power laser beams can clean space debris. For thin atmospheres, these beams primarily cause phase distortion, manageable with adaptive optics, potentially aiding laser material processing.

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Area of Science:

  • Physics
  • Optics
  • Aerospace Engineering

Background:

  • Ultra-high power laser beams, exceeding the self-focusing threshold significantly, are being considered for space debris removal.
  • Atmospheric propagation of these intense beams presents unique phenomena distinct from conventional self-focusing.

Purpose of the Study:

  • To investigate the atmospheric propagation characteristics of ultra-high power laser beams relevant to space applications.
  • To determine the impact of atmospheric thickness on laser beam self-focusing and distortion.

Main Methods:

  • Theoretical analysis of laser beam propagation through a thin atmospheric layer.
  • Modeling the lowest order effects of atmospheric interaction on ultra-high power beams.

Main Results:

  • For atmospheric thicknesses much shorter than the focal length (orbit scale), ultra-high power laser beams primarily induce phase distortion.
  • Self-focusing effects are minimal in this 'thin window' regime, with phase distortion being the dominant outcome.

Conclusions:

  • The 'thin window' model demonstrates that atmospheric self-focusing can be mitigated for ultra-high power laser beams using adaptive optics.
  • This understanding has implications for space debris mitigation strategies and advanced applications like femtosecond laser material processing.