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dc.contributor.authorPyuzza, Nelson D.
dc.date.accessioned2013-05-27T09:37:55Z
dc.date.available2013-05-27T09:37:55Z
dc.date.issued1982
dc.identifier.citationMaster of Scienceen
dc.identifier.urihttp://erepository.uonbi.ac.ke:8080/xmlui/handle/123456789/26153
dc.description.abstract300 mb. mean wind speeds and directions o were extracted at 5 latitude/longitude grid points In a region between latitudes 300N and 300S around the globe for the months of January, April, July and October. The streamline-isotach charts (The Upper Tropospheric Circulation over the Global Tropics) prepared by Sadler (1975) were used for this purpose. The zonal and meridional wind components were used for the computation of the horizontal velocity divergence~ relative vorticity, their component terms and absolute vorti~ity. The horizontal velocity divergence and relative vorticity were used to decompose the wind vector into the divergent and rotational components by the Liebmann reiaxationprocedure and Version II of-Hawkins and Rosenthal (1965) scheme for boundary values. A number of other dynamical computations were made which include a comparlson of the divergent and rotational wind components, an examination of the computable quantities occurring In the divergence and vorticity equations and a determination of their - Xl - Fourier amplitudes and phase angles In the zonal direction. These computations were also used to verify the validity of the classical scale analysis technique, wherever possible. The results of this study show that: (i) For total wind vector V, the magnitude of the zonal wind component is larger than that of the Deridional wind component. The zonal component is smallest in the equatorial latitudes and increases towards the subtropics. It is largest in the winter hemisphere- The magnitude of the meridional component shows very little variation with latitude. gradients occur in the winter hemisphere. (ii\ Large positive values of velocity divergence general_f occur around the equator and large negafi~e values of divergence occur in the sub-tropical latitudes above the surface position of the sub-tropical ridge line. The largest divergence viiues'occur roughly above the surface position of the Intertropical Convergence Zone (ITC~). Ciii) The relative vorticity field 1S dominated by anticyclonic vorticity e~cept in the regions of mid-oceanic cyclonic troughs. The largest values of relative vorticity and its meridional (.IV,) "I'he magnitudes 0f aaxu and aayv vary very 1·1tt1e with latitude. Each is of the same order of magnitude as the horizontal velocity divergence. (v) The magnitude of av than that of ax. is generally much larger au The largest values of ay occur in the winter hemisphere and its smallest - values occur in the equatorial region. have does not vary much with latitude. (vi) The absolute vorticity is positive in the northern hemisphere and negative in the southern hemisphere except within about 50 latitude from the equator, where the position of zero absolute vorticity isopleth fluctuates around the equator, being confined more into the winter hemisphere than into the summer hemisphere. (vii) The velocity potential field shows several closed zonally oriented-·centres of mass sources and sinks. The major mass sources are generally found in the summer hemisphere corresponding to the surface position of the Inter-tropical Convergence Zone. The major mass sinks are found in the winter hemisphere. (viii) The stream function field is in good agreement with the corresponding streamline analysis pattern, with positions of the major cyclonic and anticyclonic systems nearly coinciding. Cix) The magnitude of the meridional divergent wind component v ls generally larger than that of the zonal divergent wind component u. v is about twice u in the sub-tropical latitudes and nearly equal in the equatorial latitudes. (x) The magnitude of the zonal rotational wind component u~ is small in the equatorial latitudes and very large in the sub-tropical latitudes. (xi) The magnitude of the meridional rotational wind component is smaller than that of the zonal rotational wind component use, and it does not vary much with latitude. (xii) The magnitude of the divergent wind vector varies very little with latitude. It is smaller than that of the:rotational wind vector , by about an order of magnitude. The rotational vector wind is largest in the , sub-tropical latitudes. (xi i i.) The magnitude of absolute by the divergent wind (is comparable to that by the rotational wind (xiv) The magnitude of absolute vorticity advection by the total wind is about three times the magnitude of the product of absolute vorticity and horizontal wind divergence , within 50 of equator; elsewhere they are nearly equal. (xv) The magnitude of the Jacobian term is generally less than both the relative vorticity term Ifs\jJa1nd the Beta termlu\jJBlbY an order of magnitude in the tropical region and by even two orders of magnitude in the sub-tropical latitudes. (xvi) The deformation term !(A~+B~) increases from ,the equatorial latitudes towards the subtropical latitudes. (xvii) The relative vorticity term increases from the equatorial towards the sub-tropical latitudes. (xviii) The Fourier amplitude~~ of relative vorticity S, meridional divergent wind v , zonal rotational wind 'meridinal rotational wind deformation term 1 (A2+B2) and vorticity term - !S~ are large and have peaks in the planetary scale waves (~ave numbers 1 to 4). The amplitudes are generally small for synoptic scale waves (wave numbers 5 to 18). (xix) The large Fourier amplitudes of the horizontal wind divergence V-V, zonal divergent wind Ux and Jacobian term 2J(v~,u~) are spread between wave numbers 1 to 10. There are two peaks; a major peak is between wave numbers 1 to 5 and a Minor peak between wave numbers 7 and 9. (xx) The winter hemisphere Fourier amplitudes are generally larger than the summer hemisphere amplitudes. The amplitudes decrease In magnitude towards the equator from the subtropical latitudes. (xxi) The scale analysis values for the horizontal velocity divergence, relative vorticity and Jacobian term are generally smaller than their corresponding observed values. The difference is much larger for wave numbers less than 5 and not as large for wave numbers 6 to 10. The scale analysis values are comparable to the observed values for wave numbers greater than 10.en
dc.language.isoenen
dc.titleA study of the mean upper tropospheric horizontal motion field in the near-equatorial regionen
dc.typeThesisen


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