| contributor author | McAnelly, Ray L. | |
| contributor author | Nachamkin, Jason E. | |
| contributor author | Cotton, William R. | |
| contributor author | Nicholls, Melville E. | |
| date accessioned | 2017-06-09T16:11:18Z | |
| date available | 2017-06-09T16:11:18Z | |
| date copyright | 1997/06/01 | |
| date issued | 1997 | |
| identifier issn | 0027-0644 | |
| identifier other | ams-62899.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4203841 | |
| description abstract | The development of two small mesoscale convective systems (MCSs) in northeastern Colorado is investigated via dual-Doppler radar analysis. The first system developed from several initially isolated cumulonimbi, which gradually coalesced into a minimal MCS with relatively little stratiform precipitation. The second system developed more rapidly along an axis of convection and generated a more extensive and persistent stratiform echo and MCS cloud shield. In both systems, the volumetric precipitation rate exhibited an early meso-?-scale convective cycle (a maximum and subsequent minimum), followed by reintensification into a modest mature stage. This sequence is similar to that noted previously in the developing stage of larger MCSs by McAnelly and Cotton. They speculated that the early meso-? convective cycle is a characteristic feature of development in many MCSs that is dynamically linked to a rather abrupt transition toward mature stage structure. This study presents kinematic evidence in support of this hypothesis for these cases, as derived from dual-Doppler radar analyses over several-hour periods. Mature stage MCS characteristics such as deepened low- to midlevel convergence and mesoscale descent developed fairly rapidly, about 1 h after the early meso-? convective maximum. The dynamic linkage between the meso-? convective cycle and evolution toward mature structure is examined with a simple analytical model of the linearized atmospheric response to prescribed heating. Heating functions that approximate the temporal and spatial characteristics of the meso-? convective cycle are prescribed. The solutions show that the cycle forces a response within and near the thermally forced region that is consistent with the observed kinematic evolution in the MCSs. The initial response to an intensifying convective ensemble is a self-suppressing mechanism that partially explains the weakening after a meso-? convective maximum. A lagged response then favors reintensification and areal growth of the weakened ensemble. A conceptual model of MCS development is proposed whereby the early meso-? convective cycle and the response to it are hypothesized to act as a generalized forcing?feedback mechanism that helps explain the upscale growth of a convective ensemble into an organized MCS. | |
| publisher | American Meteorological Society | |
| title | Upscale Evolution of MCSs: Doppler Radar Analysis and Analytical Investigation | |
| type | Journal Paper | |
| journal volume | 125 | |
| journal issue | 6 | |
| journal title | Monthly Weather Review | |
| identifier doi | 10.1175/1520-0493(1997)125<1083:UEOMDR>2.0.CO;2 | |
| journal fristpage | 1083 | |
| journal lastpage | 1110 | |
| tree | Monthly Weather Review:;1997:;volume( 125 ):;issue: 006 | |
| contenttype | Fulltext | |