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Detailed Reference Information |
Wand, R.H., Rastogi, P.K., Watkins, B.J. and Loriot, G.B. (1983). Fine Doppler resolution observations of thin turbulence structures in the tropostratosphere at Millstone Hill. Journal of Geophysical Research 88: doi: 10.1029/JC088iC06p03851. issn: 0148-0227. |
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The 440-MHz radar at Millstone Hill (42.6 ¿N,71.5 ¿W) was employed to examine the detailed evolution of turbulence structures in the tropostratosphere with a very fine Doppler resolution of 0.12 Hz, corresponding to 4 cm s-1 radial velocity resolution. The measurement technique involved directing the antenna downwind at a low elevation angle (15¿ or 20¿) and processing the echos from a range where the background wind shear was high. Although no attempt was made to obtain good range resolution, a wide variety of turbulence structures were evident by virtue of their different Doppler shifts in the presence of a high wind shear. Using arguments based on the dominance of 'shear broadening' and the required velocity gradient to create instabilities, maximum layer thicknesses in the vicinity of 20--300 m were inferred. The implication of these observations to bulk transport of passive contaminants in the stratosphere is briefly discussed. |
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BACKGROUND DATA FILES |
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Abstract![](/images/icons/spacer.gif) |
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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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