The Structure of Winds of the Upper Troposphere at MesoscaleSource: Journal of the Atmospheric Sciences:;1963:;Volume( 020 ):;issue: 002::page 94Author:Mantis, Homer T.
DOI: 10.1175/1520-0469(1963)020<0094:TSOWOT>2.0.CO;2Publisher: American Meteorological Society
Abstract: Spectra of the variance of horizontal velocities derived from the trajectories of superpressure altitude-controlled balloons have been obtained in the frequency range 0.005 to 0.5 cy min?1. With the aid of other constant-altitude balloon data, a spectrum of velocity variance of the upper tropospheric winds is proposed for a range of frequencies termed mesoscale, which is meant to describe scales of motion just smaller than synoptic scale but larger than the motions usually referred to as turbulence. The mesoscale spectra all decreases sharply with frequency at frequencies just above synoptic scale to a frequency of about 0.1 cy min?1, where an irregular increase sets in. The spectra continue to rise to the highest frequencies analyzed, pointing to a second spectral maximum in the turbulent regime. The spectra have been used to estimate the non-representative mesoscale standard deviation of the upper winds of 7 to 17 knots. A horizontal diffusivity by mesoscale motions is estimated to be of the order of 102 cm2 see?1.
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| contributor author | Mantis, Homer T. | |
| date accessioned | 2017-06-09T14:12:59Z | |
| date available | 2017-06-09T14:12:59Z | |
| date copyright | 1963/03/01 | |
| date issued | 1963 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-14889.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4150499 | |
| description abstract | Spectra of the variance of horizontal velocities derived from the trajectories of superpressure altitude-controlled balloons have been obtained in the frequency range 0.005 to 0.5 cy min?1. With the aid of other constant-altitude balloon data, a spectrum of velocity variance of the upper tropospheric winds is proposed for a range of frequencies termed mesoscale, which is meant to describe scales of motion just smaller than synoptic scale but larger than the motions usually referred to as turbulence. The mesoscale spectra all decreases sharply with frequency at frequencies just above synoptic scale to a frequency of about 0.1 cy min?1, where an irregular increase sets in. The spectra continue to rise to the highest frequencies analyzed, pointing to a second spectral maximum in the turbulent regime. The spectra have been used to estimate the non-representative mesoscale standard deviation of the upper winds of 7 to 17 knots. A horizontal diffusivity by mesoscale motions is estimated to be of the order of 102 cm2 see?1. | |
| publisher | American Meteorological Society | |
| title | The Structure of Winds of the Upper Troposphere at Mesoscale | |
| type | Journal Paper | |
| journal volume | 20 | |
| journal issue | 2 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1963)020<0094:TSOWOT>2.0.CO;2 | |
| journal fristpage | 94 | |
| journal lastpage | 106 | |
| tree | Journal of the Atmospheric Sciences:;1963:;Volume( 020 ):;issue: 002 | |
| contenttype | Fulltext |