Abstract
Fourier transform spectroscopy in the infrared is a very powerful technique for remote sensing measurements of atmospheric constituents. The use of the sun as a radiation source for absorption measurements allows the combination of high spectral resolution together with high signal-to-noise ratio, hence leading to high sensitivity. The possibility of using such a technique under stratospheric balloons adds the capability of good vertical resolution for the measurement of trace species concentration profiles in the solar occultation mode. A description of such an instrumentation and samples of representative results are given.
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 callMore From: Spectrochimica Acta Part A: Molecular Spectroscopy
Disclaimer: 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.
