Abstract
The design, construction, and performance of a combined solar telescope and Michelson interferometer for balloon-borne stratospheric far-IR absorption studies is discussed in terms of the relevant parameters and precautions necessary to obtain high resolution radiometrically calibrated spectra of the stratosphere between 20 and 100 cm(-1). Preliminary data are presented to indicate that the system performed as designed and provided constituent concentration values for H(2)O and O(3) from measurements of strong absorption lines in this spectrum.
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.
