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Detailed Reference Information |
Russell, P.B., Livingston, J.M., Pueschel, R.F., Reagan, J.A., Browell, E.V., Toon, G.C., Newman, P.A., Schoeberl, M.R., Lait, L.R., Pfister, L., Gao, Q. and Herman, B.M. (1993). Post-Pinatubo optical depth spectra vs. latitude and vortex structure: Airborne tracking sunphotometer measurements in AASE II. Geophysical Research Letters 20: doi: 10.1029/93GL03006. issn: 0094-8276. |
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In January and March 1992, DC-8-measured stratospheric particle optical depth spectra, &tgr;p(&lgr;), peaked broadly at midvisible or longer wavelength. At mid-to-high northern latitudes outside the vortex, &tgr;p (526 nm) above about 11 km was as large as 0.22 in both January and March, reflecting continued Pinatubo volcanic influence. In both months, in-vortex &tgr;p(&lgr;) above 11 km was smaller than outside-vortex values by a factor of two or more, and in January a strong anticorrelation was observed between &tgr;p(&lgr;) and HF column content (an indicator of vortex penetration). In late January at 18--20 S, near the edge of the southern subtropical jet, &tgr;p (526 nm) above 12 km was only about 0.l07--0.09, with a flatter spectral shape than northern mid- to high-latitude measurements in both January and March. Occasional high-latitude vertical profiles indicate 6--11-km slab optical depths, Δ&tgr;p (526 nm), of 0.05 to 0.1, which should be added to the above-11-km values to yield values above 6 km. ¿ American Geophysical Union 1993 |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Atmospheric Composition and Structure, Middle atmosphere—composition and chemistry |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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