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contributor authorBalsley, B. B.
contributor authorRiddle, A. C.
date accessioned2017-06-09T14:25:06Z
date available2017-06-09T14:25:06Z
date copyright1984/08/01
date issued1984
identifier issn0022-4928
identifier otherams-18893.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4154948
description abstractMonthly-averaged horizontal and vertical mesospheric wind fields have been measured using the Poker Flat Radar at 65°N latitude during 15 months in 1980?81. The horizontal wind fields are reasonably consistent with previous observations and with some of the current theoretical models that take into account enhanced turbulence and eddy transport observed at mesospheric heights. However, the observed vertical wind field has a quasi-sinusoidal seasonal variation with peak values of 25 cm s?1 both downward near summer solstice and upward near winter solstice and is inconsistent with current models of mean circulation in the meridional plane. Because there are no other comparable vertical wind observations, the possibility of error in the vertical wind measurements was carefully considered and rejected. We conclude that the actual mean circulation is more complex than that implied by current models. Possible complicating factors include nonuniform zonal flow, multicellular meridional structure and an enhanced vertical Stokes drift that would arise from strong eddy activity.
publisherAmerican Meteorological Society
titleMonthly Mean Values of the Mesospheric Wind Field over Poker Flat, Alaska
typeJournal Paper
journal volume41
journal issue15
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1984)041<2368:MMVOTM>2.0.CO;2
journal fristpage2368
journal lastpage2380
treeJournal of the Atmospheric Sciences:;1984:;Volume( 041 ):;issue: 015
contenttypeFulltext


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