A theoretical study of atmospheric propagation of laser and return light for stand-off laser induced breakdown spectroscopy purposes

A theoretical study of atmospheric extinction mechanisms of optical radiation (molecular/aerosol scattering and absorption) has been carried out in order to assess their influences on stand-off laser-induced breakdown spectroscopy (LIBS) measurements. The atmospheric extinction of laser radiation at wavelengths commonly used in laser-induced breakdown spectroscopy (1064 nm and 532 nm) and of the laser-induced breakdown spectroscopy plasma emission beyond 250 nm is small compared to the attenuation with range due to the inverse square law. The fundamental problem with light propagation through the atmosphere is that the atmospheric transmittance does not remain constant within the whole spectral interval, and that this variation results in a change in the spectral distribution of the light received by the detector. Knowledge of atmospheric transmittance would allow for compensation of this effect.