2006
DOI: 10.1016/j.physd.2006.09.023
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Atmospheric propagation of gradient-shaped and spinning femtosecond light pulses

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Cited by 28 publications
(25 citation statements)
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“…Azimuthal modulation instability of vortices was also analyzed in [29,5]. The number of filaments predicted in these studies is different from our prediction, yet was in agreement with the numerical simulations conducted in these studies.…”
Section: Azimuthal Instability Of Collapsing Vortex Solutionssupporting
confidence: 56%
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“…Azimuthal modulation instability of vortices was also analyzed in [29,5]. The number of filaments predicted in these studies is different from our prediction, yet was in agreement with the numerical simulations conducted in these studies.…”
Section: Azimuthal Instability Of Collapsing Vortex Solutionssupporting
confidence: 56%
“…Lemma 7. Let G m (r ) be a solution of (29). Then G m (r ) = r m g m (r ), where g 0 = g m (0) = 0 and g m (r ) is the analytic solution of…”
Section: Substitution Of ψ a M Into The Critical Nls (4) Gives The Fomentioning
confidence: 99%
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“…At the wavelength λ 0 = 355 nm, a "long" supergaussian pulse with t p = 500 fs (FWHM 1 ps), small waist w 0 = 200 µm, 100 critical powers, and suffering 5% random noise both in spatial and temporal amplitudes, develops regular modulations on its steepest boarders, before the most intense filaments reach the ionization threshold [29,30]. Figure 3(a) displays the evolution of the maximum pulse intensity and electron density.…”
Section: A Long Pulse Durations (Uv)mentioning
confidence: 99%