Filamentation of ultrashort laser pulses in the atmosphere offers unique opportunities for long-range transmission of high-power laser radiation and standoff detection. With the critical power of self-focusing scaling as the laser wavelength squared, the quest for longer-wavelength drivers, which would radically increase the peak power and, hence, the laser energy in a single filament, has been ongoing over two decades, during which time the available laser sources limited filamentation experiments in the atmosphere to the near-infrared and visible ranges. Here, we demonstrate filamentation of ultrashort mid-infrared pulses in the atmosphere for the first time. We show that, with the spectrum of a femtosecond laser driver centered at 3.9 μm, right at the edge of the atmospheric transmission window, radiation energies above 20 mJ and peak powers in excess of 200 GW can be transmitted through the atmosphere in a single filament. Our studies reveal unique properties of mid-infrared filaments, where the generation of powerful mid-infrared supercontinuum is accompanied by unusual scenarios of optical harmonic generation, giving rise to remarkably broad radiation spectra, stretching from the visible to the mid-infrared.
Laser-induced filamentation1,2,3 is a thrilling phenomenon of ultrafast optical physics, in which diffraction of a laser beam is suppressed by a combined effect of self-focusing and transverse electron density profile induced by ultrafast photoionization. While filamentation of ultrashort light pulses with peak powers above the self-focusing threshold is a universal phenomenon, observed in gases, liquids, and solids2,3, laser filaments in the atmosphere are of special significance as they offer unique opportunities for long-range signal transmission, delivery of high-power laser beams, and remote sensing of the atmosphere4.
In Fig. 1, we present a survey of representative laser filamentation experiments1,2,3,5,6,7,8,9,10,11,12,13,14,15 in various gases, including the atmospheric air, in a diagram where the wavelength and the peak power of laser pulses are used as coordinates. The single-filamentation regime in the atmospheric air exists in the dark area of this diagram. Loosely defined boundaries of this area are shown by gradient shading. The lower boundary is centered at the critical power of self-focusing16,17, Pcr = C(8πn0n2)−1λ2, where n0 is the field-free refractive index, n2 is the nonlinear refractive index and C is a numerical factor, 3.72 < C < 6.4, defined18 by the beam profile (C ≈ 3.72 and 3.77 for Townesian and Gaussian beams, respectively). The Pcr threshold is the key parameter for laser-induced filamentation, which sets a fundamental limit on the peak power and, hence, the energy of laser pulses in a filament. Below this threshold (purple shaded area in Fig. 1), the nonlinear lens induced by a laser beam is not strong enough to compensate for beam diffraction. In the opposite case, when the peak power of a laser field becomes much higher than Pcr (rose shading in Fig. 1), the beam tends to decay into multiple small-scale filaments2,3, losing its spatial coherence. The parameter space where a laser beam can propagate as a single filament in the atmospheric air is thus bound to the dark shaded area in the diagram of Fig. 1.
Up to now, experiments on laser-induced filamentation in the atmospheric air (white circles in Fig. 1) were limited to the visible and near-infrared ranges (λ < 1030 nm), where sufficiently powerful short-pulse laser sources were available1,2,3,5,6,7,8,9,10,11,12,13. Most of those earlier experiments on laser filamentation in the atmosphere were performed using Ti: sapphire laser systems1,2,3. This class of lasers can deliver ultrashort pulses within a broad range of peak powers, allowing the generation of single and multiple filaments in air (white and rose segments of an ellipse centered at 800 nm in Fig. 1), as well as a variety of filamentation regimes in high-pressure gases (the yellow segment of the ellipse at 800 nm). Because of the λ2 scaling of the critical power of self-focusing Pcr, using a longer-wavelength laser driver is a straightforward strategy for increasing the laser peak power and radiation energy in a single filament. Overall, filamentation experiments in high-pressure atomic and molecular gases performed using laser drivers with different carrier wavelengths1,2,3,5,6,7,8,9,10,11,12,13,14,15 confirm this possibility (Fig. 1). However, building longer-λ alternatives to Ti: sapphire1,2,3 and, since recently, ytterbium9 and Cr: forsterite10 lasers that would be capable of delivering ultrashort laser pulses with peak powers above Pcr for the atmospheric air, i.e., at least a factor of λ2 higher than the peak powers of amplified Ti: sapphire and ytterbium laser pulses used for atmospheric filamentation, is a challenging problem.
Here, we show that cutting-edge laser technologies, based on optical parametric chirped-pulse amplification (OPCPA) in the mid-infrared, offer powerful tools to confront this challenge. In our experiments, a high-peak-power compressed output of a multistage mid-infrared OPCPA system (see the Methods section) is employed to enable the generation of mid-infrared laser filaments in the atmosphere for the first time. In the earlier work, an OPCPA-based approach has been used to generate ultrashort pulses in the mid-infrared at the 10-mJ level of output energy19, enabling laser-induced filamentation in high-pressure gases14,15,20. In experiments presented here, the short-pulse mid-infrared source was upgraded to a much higher level of output energies, making it possible to induce laser filaments in the atmospheric air. The stretched-pulse OPCPA output in this upgraded system has an energy above 50 mJ. Compression of these pulses using a grating compressor yields sub-100-fs mid-infrared pulses with an energy up to 30 mJ.
The 3.9-μm OPCPA output with a peak power exceeding Pcr ≈ 150 GW loosely focused by a CaF2 lens with a focal length ranging from 0.5 to 1.2 m induces a filament in the atmosphere. Filament formation is visualized by a bright spark whose length varies from a few centimeters up to 30 cm (pictured against a ruler in Fig. 2), depending on the peak power of the laser driver and the focal length of the focusing lens. Filamentation of laser pulses is accompanied by a dramatic increase in the bandwidth of the mid-infrared pulse behind the region of filamentation. Typical spectra of such broadband radiation measured in our filamentation experiment in the atmosphere are shown in Figs. 3d, 3e, and 4a. The long-wavelength part of these spectra (Fig. 3d) represents a broadened spectrum of the mid-infrared driver with an extended blue wing and a long-wavelength tail attenuated and eventually limited by the absorption of carbon dioxide in the atmosphere (Fig. 3e). The near-infrared section of the spectrum (Figs. 4a–4c) is dominated by spectrally broadened peaks observed near the frequencies of the third and fifth harmonics of the mid-infrared driver. Finally, the visible part of the spectrum (Figs. 4a–4c) features prominent maxima near the frequencies of the seventh and ninth harmonics of the driving field. A typical far-field beam profile of the filament output, shown in the inset to Fig. 4a, reveals a bright white-light central part surrounded by greenish and reddish outer rings.
To analyze the spatiotemporal field dynamics leading to a filamentation of ultrashort mid-infrared pulses, we use a model based on the field evolution equation2,3 that includes the dispersion of the medium, beam diffraction, optical nonlinearities due to the third-, fifth-, seventh-, and ninth-order susceptibilities of a gas medium, ionization-induced nonlinearities, pulse self-steepening, spatial self-action phenomena, as well as plasma-related loss, refraction, and dispersion. This equation is solved jointly with the equation for the electron density ρ(t) with the photoionization rate calculated using the Popov−Perelomov−Terentyev version of the Keldysh formalism2,3. Numerical simulations, performed on the Chebyshev and Lomonosov supercomputer clusters of Moscow State University, accurately reproduce the key features in the experimental spectra (Figs. 4a–4c) and beam profiles (Figs. 5a, 6a, 6b) of the filament output and provide an accurate estimate for the filament length (Figs. 2, 5a). This numerical analysis reveals a number of striking features in the nonlinear spatiotemporal dynamics of mid-infrared pulses in the filamentation regime that never show up in near-infrared laser filaments.
As can be seen from Fig. 6c, the initial stage of filamentation of a mid-infrared beam, within the range of the propagation coordinate z from 0 to 60 cm, is dominated by self-phase modulation − a universal mechanism of spectral broadening of ultrashort laser pulses regardless of the spectral range. However, already at this initial stage of filamentation, other significant nonlinear processes come into play, most notably, odd-order optical harmonic generation. While third-harmonic generation is not uncommon to laser filamentation of Ti: sapphire laser pulses in the atmosphere2,3, higher order harmonics of a 800-nm driver fall outside the atmospheric transmission window and do not show up in filamentation in the near-infrared. The situation is drastically different in the case of filaments induced by mid-infrared pulses, when a whole group of odd-order harmonics can fall, as in the case of our experiments, within the transmission range of the atmospheric air (Fig. 3e). Moreover, the weakness of dispersion of the atmospheric air in the mid-infrared favors phase matching for the generation of these harmonics. These two factors give rise to a unique scenario of optical harmonic generation in a mid-infrared laser filament. The near-infrared and visible parts of filament output spectra in our experiments feature prominent signals near the frequencies of the third, fifth, seventh, and ninth harmonics of the 3.9-μm driver (Figs. 3e, 4a–4c, 6c), all falling within the atmospheric transparency range. Combined with the mid-infrared supercontinuum, these harmonics give rise to remarkably broad radiation spectra at the output of the filament, spanning the entire visible and near-infrared ranges and covering a considerable part of the mid-infrared up to the edge of the mid-infrared atmospheric transmission window.
Enhancement of harmonic generation by a mid-infrared driver due to improved phase matching, facilitated by the weakness of gas dispersion in the mid-infrared range, has been earlier demonstrated in experiments with a collimated mid-infrared pump beam21. Optical harmonic generation in the filamentation regime, however, is in no way reduced to the collinear geometry of harmonic generation by an ultrashort mid-infrared driver. In the filamentation regime, harmonic generation is further enhanced relative to the regime of a collimated laser driver due to a higher intensity of the driver field, sustained over the entire length of a filament (Fig. 5a). Moreover, the far-field beam profile analysis (the inset in Fig. 4a) reveals a complex beam pattern of the filament output, showing that optical harmonic generation in a mid-infrared filament is nonuniform across the beam and clearly indicating the significance of off-axial harmonic-generation processes.
Numerical simulations presented in Figs. 5a–5e offer important insights into the physics behind filamentation of mid-infrared pulses, revealing, in particular, the significance of the (ωp/ω)2 scaling of the ionization-induced change in the refractive index with the radiation frequency ω (ωp being the plasma frequency). Due to this scaling, mid-infrared beams are much more prone to scattering by transient electron-density profiles in filaments (Figs. 5a–5e, 7a) compared to near-infrared beams. As can be seen from simulations performed for a mid-infrared driver focused by a 75-cm-focal-length CaF2 lens, mimicking our experimental geometry, the significance of these plasma-induced scattering effects tends to increase toward the trailing edge of the pulse. Indeed, in the leading edge of the mid-infrared pulse, where the field intensity is low (τ = −50 fs in Fig. 5b), self-focusing and ionization effects are negligible. The beam dynamics in this section of the pulse is dominated by diffraction. However, as the field intensity increases within the mid-infrared pulse, nonlinear phenomena become significant, with an interplay between self-focusing and ionization-induced defocusing giving rise to well-resolved beam refocusing cycles (Figs. 5c–5e).
It is instructive to describe this beam dynamics in terms of two characteristic beam radii − the full width at half-maximum (FWHM) beam radius, rFWHM, and the root-mean-square (rms) beam radius rrms. Since the field intensity on the beam axis is much higher than the field intensity in the peripheral part of the beam, the FWHM beam radius is well-suited to quantify the size of the filament, with the behavior of rFWHM plotted as a function of the propagation path z helping isolate the filament in the overall beam dynamics and visualizing beam refocusing cycles (white line in Figs. 5d and 5e). Unlike the rFWHM, the rms radius does not discriminate between the central, high-intensity part of the beam and its low-intensity peripheral part, providing an integral measure of the transverse beam size. This parameter is thus sensitive to the dynamics of a strongly diverging outer part of the beam, visualizing the scattering of mid-infrared radiation by the electron-density profile (Fig. 5a).
The central part of the mid-infrared driver pulse and its trailing edge “see” a transient electron-density gradient induced by the leading edge of the pulse, which gives rise to a strong, (ωp/ω)2-factor-enhanced scattering of mid-infrared radiation (Figs. 5d, 5e, 7a). A part of this scattered radiation then undergoes refocusing (Figs. 5d, 5e), forming a filament in the central part of the beam. To relate the time-resolved maps of beam dynamics presented in Figs. 5b–5e to the experimentally measurable beam profiles, it is instructive to examine beam dynamics integrated over the entire pulse. Such a time-integrated map of beam dynamics in a mid-infrared laser filament is presented in Fig. 5a. As can be seen from this map, the filament propagating in the direction of arrow 1 in Fig. 5a translates into a bright white spot at the center of the output beam (shown on the right of Fig. 5a, see also Fig. 7a). The remaining part of the plasma-scattered beam, propagating in the direction of arrow 2 in Fig. 5a, forms the ring structure in the output beam profile.
As can be seen from Figs. 5b–5e, the length of the mid-infrared filament, defined as the length within which the FWHM beam radius does not exceed twice its minimum value, becomes as large as lf ≈ 75 cm on the trailing edge of the pulse (Fig. 5e). In the time-averaged map of beam dynamics (Fig. 5a), filamentation is seen to be sustained well beyond the point of nonlinear focus (z = 65 cm, indicated with an arrow in Fig. 5a), predicted by the standard Marburger formula16,22. The length of the filament estimated from this map, lf ≈ 40 cm, is still substantially larger than the Rayleigh length for the mid-infrared driver in our experimental geometry, lR ≈ 8.5 cm.
An ultrafast buildup of the electron density ρ(t) induced by the driver pulse gives rise to a time-dependent plasma change in the refractive medium of the gas, δnp(τ) ≈ −ρ(τ)/(2ρcr), where τ = t − zn0/c, t is the time in the laboratory frame of reference, n0 is the field-free refractive index, c is the speed of light in vacuum, z is the propagation coordinate, and ρcr is the critical electron density. The refractive index will thus decrease from the leading edge of a driver to its trailing edge (Fig. 7b). As a result, the phase velocity in the trailing edge of the driver, vt(τ) = c[n0 + δnp(τ)]−1, is higher than the phase velocity of its leading edge, vl ≈ v0 = c/n0 giving rise to a Doppler-like blue shift (Fig. 7b). Since the outer sections of the beam are due to a strong scattering of radiation off the electron density profile (Figs. 5a, 7a), these parts of the beam, as can be seen in Fig. 6b, exhibit a much stronger blue shift. As a result, the off-axis optical harmonics are also blue-shifted relative to the harmonics generated along the beam axis. Simulations presented in Figs. 6d–6f show how this blue shift of the off-axial harmonics builds up, increasing toward the output end of the filament.
These insights into the beam dynamics help understand the ring structure of the far-field beam profile observed in our mid-infrared filamentation experiments. In the central part of the beam (direction labeled with arrow 1 in Fig. 5a), generation of a mid-infrared supercontinuum (Fig. 3d) is accompanied by efficient generation of the third, fifth, seventh, and ninth harmonics in a collinear geometry, giving rise to a bright white spot centered on the beam axis at the center of the far-field beam pattern (the inset in Fig. 4a). Since the third harmonic lies in the near-infrared range, it does not contribute to the colors of the rings in the output beam pattern. Within the range of angles 1.3–3.5 mrad (direction 2 in Fig. 5a), the fifth harmonic also falls outside the visible range, with the seventh harmonic, centered at 0.56 μm (Fig. 4b), giving rise to a greenish color of the beam pattern. Finally, at the periphery of the beam (corresponding to direction 3 in Fig. 5a), the intense fifth-harmonic signal, blue-shifted to 0.65 μm (Fig. 4c), is responsible for a reddish color of the outer ring in the output beam profile observed in experiments (the inset in Fig. 4a). The colors of the far-field beam pattern synthesized from the results of numerical simulations (Fig. 5a, right) are fully consistent with experimental beam profiles (the inset in Fig. 4a).
To summarize, filamentation of ultrashort mid-infrared pulses in the atmosphere has been demonstrated for the first time. With the spectrum of a femtosecond laser driver centered at 3.9 μm, right at the edge of the atmospheric transmission window, radiation energies above 20 mJ and peak powers in excess of 200 GW have been transmitted through the atmosphere in a single filament. Our studies reveal unique properties of mid-infrared filaments, where the generation of powerful mid-infrared supercontinuum is accompanied by unusual scenarios of optical harmonic generation, giving rise to remarkably broad radiation spectra, stretching from the visible to the mid-infrared.
In our experiments, high-power ultrashort mid-infrared pulses are delivered by a laser system (Fig. 2) consisting of a solid-state Yb: CaF2 laser, a three-stage optical parametric amplifier (OPA), a grism stretcher, a Nd: YAG pump laser, a three-stage OPCPA system, and a grating compressor for mid-infrared pulses. The 1-kHz, 200-fs, 1–2-mJ, 1030-nm regeneratively amplified output of the Yb: CaF2 laser system is used as a pump for the three-stage OPA, which generates 200-fs 1460-nm pulses at its output. These 1460-nm pulses are then stretched with a grism stretcher and used as a seed signal in a three-stage OPCPA, consisting of three KTA crystals I, II, and III (Fig. 2), pumped by 100-ps Nd: YAG-laser pulses with energies 50, 250, and 700 mJ, respectively. The idler-wave output of the OPCPA system has a central wavelength of 3.9 μm and a pulse width of 90 fs. The stretched-pulse OPCPA output has an energy above 50 mJ. Compression of these pulses using a grating compressor yields mid-infrared pulses with a pulse width of 80 to 200 fs and an energy up to 30 mJ.
Detection and pulse characterization in the mid-infrared
Spectral measurements in the mid-infrared range are performed with a homebuilt scanning monochromator and a thermoelectrically cooled HgCdTe detector (Fig. 2). For the spectral measurements in the visible and near-infrared ranges, standard OceanOptics spectrometers were employed. Temporal envelopes and phases of mid-infrared pulses are characterized using frequency-resolved optical gating (FROG) based on second-harmonic generation (SHG) in a 0.5-mm-thick AgGaS2 crystal. A typical spectrum of the 3.9-μm OPCPA output is shown in Fig. 3a. Its FROG trace and temporal envelope and phase retrieved from this trace are presented in Figs. 3b and 3e.
This research was supported in part by the Russian Foundation for Basic Research (project nos. 14-29-07182, 14-22-02099, 14-22-02105, and 14-02-00784) and the Welch Foundation (Grant No. A-1801). Research into ultrafast nonlinear optics in the mid-infrared has been supported by the Russian Science Foundation (project no. 14-12-00772). A.A.V. acknowledges the support of his research by the Dynasty Foundation. A.B. and S.A. acknowledge support by the Austrian Science Fund (FWF) via NextLite SFB F4903-N23 project. T.F. acknowledges support by FWF in the framework of the Doctoral School W1243.
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