Simultaneous detection of FC-11, FC-12 and FC-22, through 8 to 13 micrometers IR solar observations from the ground

Details Simultaneous detection of FC-11, FC-12 and FC-22, through 8 to 13 micrometers IR solar observations from the ground Simultaneous detection of FC-11, FC-12 and FC-22, through 8 to 13 micrometers IR solar observations from the ground

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983georl..10..521z&link_type=abstract

Geophysical Research Letters, Volume 10, Issue 7, p. 521-524

Computer Science

Performance

14

Scientific paper

High-resolution solar observations covering the 8 to 13 μm atmospheric window are now being carried out routinely at the Kitt Peak National Observatory (KPNO), Tucson, Arizona, using a 1 meter-path difference Fourier transform spectrometer. Such observations allow the simultaneous measurement of a large number of trace gases. Preliminary results for the three most important fluorocarbons, FC-11, FC-12 and FC-22 are reported here. These results, in the form of average mixing ratios, show the potential and illustrate the performance of the Kitt Peak interferometer for this application.

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