Total ozone determination by chappuis band absorption at an urban location

Main Article Content

T. F. Eck
R. T. Pinker

Abstract

Total columnar ozone was estimated at College Park, Maryland, from spectral measurements of the direct beam solar radiation in the visible wavelength spanning the Chappuis continuum (550 <A <700 nm). A comparison of total ozone derived by the Chappuis band measurements with Dobson spectrometer measurements of total ozone showed that the Chappuis band method differed from the Dobson method by approximately ±20% on the most stable days. These differences can be attributed to a combination of: large aerosol optical depths; diurnal variation of aerosol optical depth; the deviation from the assumed power law relationship used to estimate the change in aerosol optical depth with wavelength; and uncertainty in the values of ozone absorption coefficients.

Article Details

How to Cite
Eck, T. F., & Pinker, R. T. (1988). Total ozone determination by chappuis band absorption at an urban location. Geofisica Internacional, 27(2), 231–240. https://doi.org/10.22201/igeof.00167169p.1988.27.2.784
Section
Article

References

ACKERMAN, M., 1971. Ultraviolet Solar Radiation Related to Mesospheric Processes, Fiocco (Ed.), Mesospheric Models and Related Experiments, pp.149-159, D. Reidel Publishing Co., Dordrecht-Holland. DOI: https://doi.org/10.1007/978-94-010-3114-1_11

DIERMENDJIAN, D., 1968. Electromagnetic Scattering on Spherical Polydispersions. American Elsevier, 290 pp.

DOBSON, G. M. B., 1968. Forty year's research on atmospheric ozone at Oxford: A history. Appl. Opt., 7, 387-405. DOI: https://doi.org/10.1364/AO.7.000387

FLEIG, A. J., K. F. KLENK, P. K. BHARTIA, D. GORDON and W. H. SCHNEIDER, 1982. User's guide for the Solar Backscattered Ultraviolet (SBUV) instrument first-year ozone-S data set. NASA Ref. Pub. 1095.

GUZZI. R., C. TOMASI and O. VITTORI, 1972. Evidence of particulate extinction in the near infrared spectrum of the sun. J. Atmos. Sci., 29, 517-523. DOI: https://doi.org/10.1175/1520-0469(1972)029<0517:EOPEIT>2.0.CO;2

HEATH, D. F., A. J. KRUEGER, H. A. ROEDER and B. D. HENDERSON, 1975. The solar backscatter ultraviolet and total ozone mapping spectrometer (SBUV / TOMS) for NIMBUS-G. Opt. Eng., 14, 323. DOI: https://doi.org/10.1117/12.7971839

KING, M. D. and D. M. BYRNE, 1976. A method for inferring total ozone content from the spectral variation of total optical depth obtained with a solar radiometer. J. Atmos. Sci., 33, 2242-2251. DOI: https://doi.org/10.1175/1520-0469(1976)033<2242:AMFITO>2.0.CO;2

KING, M. D., D. M. BYRNE, J. A. REAGAN and B. M. HERMAN, 1980. Spectral variation of optical depth at Tucson, Arizona between August 1975 and December 1977. J. Appl. Meteor., 19, 723-732. DOI: https://doi.org/10.1175/1520-0450(1980)019<0723:SVOODA>2.0.CO;2

KLENK, K., P. K. BHARTIA, A. J. FLEG, V. G. KAREESHWAR, R. D. McPETERS and P. M. SMITH, 1982. Total ozone determination from the backscattered Ultraviolet (BUV) experiment. J. Appl Meteor., 21. DOI: https://doi.org/10.1175/1520-0450(1982)021<1672:TODFTB>2.0.CO;2

SHAW, G. E., J. A. REAGAN and B. M. HERMAN, 1973. Investigations of atmospheric extinction using direct solar radiation measurements made with a multiple wavelength radiometer. J. Appl. Meteor., 12, 374-380. DOI: https://doi.org/10.1175/1520-0450(1973)012<0374:IOAEUD>2.0.CO;2

SHAW, G. E., 1979. Atmospheric ozone: determination by Chappuis band absorption. J. Appl. Meteor., 18, 1335-1339. DOI: https://doi.org/10.1175/1520-0450(1979)018<1335:AODBCB>2.0.CO;2

SPINHIRNE, J. D., 1983. El Chichón eruption cloud: Latitudinal variation of the spectral optical thickness for October 1982. Geoph. Res. Lett., 10, 9, 881-884. DOI: https://doi.org/10.1029/GL010i009p00881