This invention is a detecting of Roman-Mie dispersion
laser atmosphere signal and
laser radar. It sets up the
radar with the output of double-frequency 532nm and triple-frequency 355nm, launches the 532nm, 15% of the 35nm to the
sky and 85% of the 355nm after
diffusion, and the two optical paths parallel with the
optical path of the receiving
telescope, and simultaneously carry out the pitching motion with the receiving
telescope; the receiving
telescope backward dispersing light, the backward light gets into the telescope, then passes the glare tube, the adjusting field view stop and ocular glass, and the dichroic mirror process, and divides the 407nm, the 386nm and the 532nm
scattered light into three beams, and the 532nm
scattered light is divided into 15% and 85% beams, and the four beams are respectively received by the multiplier
phototube, magnified by the magnifier and collect and process the data. It can detect the level
visibility of the
atmosphere, the
aerosol of the whole
troposphere and the vertical outline of winding cloud light eliminating
system and the water and air mixture ratio from the ground to the lower part of the
troposphere. The detecting error of the level
visibility is 15%, the errors of the
aerosol light eliminating modulus and the vertical outline of the water and air mixture are 20%.