Abstract
The analysis of basic spectroscopic factors influencing the simulation of atmospheric radiative transfer in the methane absorption IR bands, which are used in the problems of methane total content retrieval from atmospheric solar spectra measurements, is carried out. The role of uncertainties in the parameters of methane and water vapor absorption lines and differences in extraterrestrial solar spectrum models are considered. The comparison with measured atmospheric spectra is made.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
