Abstract
The line-by-line method of computing emission and spectral transmission is analysed in order to determine the H 2O and O 3 concentrations relative to that of O 2 in the lower stratosphere. The effects of computation parameters are discussed. The method of calculating the relative constituent concentrations from integrated emission line areas is analysed quantitatively. While good accuracy was obtained for the results for the strong H 2O lines, the same cannot be said of the weak O 3 lines.
Sign-in/Register to access full text options 
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 callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
