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%.