Determination of total ozone over Mauna Loa using very high resolution infrared solar spectra

Details Determination of total ozone over Mauna Loa using very high resolution infrared solar spectra Determination of total ozone over Mauna Loa using very high resolution infrared solar spectra

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993georl..20.2055d&link_type=abstract

Geophysical Research Letters, Volume 20, Issue 19, p. 2055-2058

Physics

3

Scientific paper

A very high resolution infrared Fourier transform spectrometer has been used to record solar spectra at the Mauna Loa Observatory in Hawaii. Spectra are normally taken one day a week at sunrise. These spectra have been analyzed for ozone and N2O total columns, and the ozone column compared with the value reported by the Mauna Loa Dobson spectrophotometer. Aside from the FTIR reporting about 5% lower values than the Dobson (which may be due to a systematic difference in the treatment of tropospheric ozone), the FTIR and Dobson agree to within 2.7% (RMS) during this period.

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