Remote sensing the column abundance of atmospheric CH4 from ground-based IR solar spectrum

Details Remote sensing the column abundance of atmospheric CH4 from ground-based IR solar spectrum Remote sensing the column abundance of atmospheric CH4 from ground-based IR solar spectrum

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1874..204w&link_type=abstract

Proc. SPIE Vol. 1874, p. 204-208, Infrared and Millimeter-Wave Engineering, Harold T. Buscher; Ed.

Other

Scientific paper

An IR solar spectrometer (ISS), which basically consists of three components: coelstat, spectrometer and data acquiring unit, was developed. With ISS we measured the solar spectra in the wavelength range of 2915 - 2920 cm(superscript -1) on the ground to derive the abundance of atmospheric CH(subscript 4). In this spectrum range, CH(subscript 4) is the main absorption gas and other gases' absorption can be omitted. The measurement results in the winter of 1991 show that the mixing ratio of CH(subscript 4) is around 1.6 ppm, with the mean measurement error about 10%.

Affiliated with

Also associated with

No associations

Rating

Remote sensing the column abundance of atmospheric CH4 from ground-based IR solar spectrum does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Remote sensing the column abundance of atmospheric CH4 from ground-based IR solar spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Remote sensing the column abundance of atmospheric CH4 from ground-based IR solar spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1232485