At present there are a number of reports on the development and creation of range-gate vision systems operating in the near-IR range. As radiation sources such systems usually use laser diodes or matrixes and as receiving elements are gated imaginer tubes or highly sensitive CCD matrixes. The principle of operation of such systems is quite simple. The object of observation is illuminated by short laser pulses in the infrared spectral range. In this case, the object is observed in an optical device equipped with a fast shutter opening in time with the sending of light pulses for a certain short time. In the case when the time delay between the moment of a radiation pulse and the moment of opening of the shutter is equal to the time necessary for light to travel the distance to the object and back, the observer will see only the object and the area of the space directly surrounding it. The depth of this space is determined both by the time of the open state of the shutter, and by the duration of the light pulse. This method is sometimes called the range gating method. The method makes it possible to obtain much more contrast images in comparison with conventional laser-illuminated observation systems, especially for the case of a scattering medium (fog, rain, snow, etc.). When the image is formed, the light backscatter from the previous layer of the atmosphere is eliminated by gating the photodetector system. However such systems have common fundamental drawbacks. First, laser sources of the near-IR range have a relatively low output power (in the best systems, diode matrixes arrays of the kilowatt range are used). Secondly, near-IR radiation is substantially scattered on such small inhomogeneous particles present in the atmosphere as droplets of condensate, dust particles, raindrops and snowflakes. This imposes serious limitations on the maximum visibility length in conditions of limited transparency of the atmosphere due to the exponential nature of the dependence of the absorption and scattering processes on the path length. In the literature, even the factor of maximum visibility improvement is used. This factor does not exceed 5 times. These shortcomings will be deprived of range-gate vision system based on a CO 2 laser, for which the radiation peak power of several megawatts is a successfully solved problem. Recently, there have been reports of the beginning of a wide production of photodetector arrays for the mid-IR range, for which pulse gating can be easily organized. In addition, if we use CO 2 lasers tuned on oscillation lines to create vision systems in the mid-IR range, it is not only easy to avoid difficulties associated with the selective absorption of light by the gas components of the atmosphere and water vapor, but also to create systems protected from artificial interference. Such systems will be able to quickly and easily settle from one spectral range to another when trying to jam. For example, a CO 2 laser tunable in the range of 9.2-10.8 μm can provide efficient operation on several dozen generation lines suitable for use in the absence of interaction with absorbing gas components of the atmosphere. Involving the so-called non-traditional transitions of the CO 2 molecule can increase the number of such lines to several hundred.