From the synoptic perspective, one of the major players in the initial spin-up of pre-Karl is a surge of southerly winds from northern South America on 8-9 September 2010, leading to the formation of a nearly closed earth-relative circulation. This circulation weakened late on 10 September and remained weak through 13 September, during which time the disturbance lacked vertical organization due to an increase in vertical wind shear and only sporadically produced convective bursts. During 13-14 September, more persistent convection developed as the precursor disturbance became vertically stacked and pre-Karl was classified as a tropical cyclone. From the equatorial wave perspective, both the initial spin-up and subsequent shearing of pre-Karl can be tied to the phases of a convectively coupled Kelvin wave (CCKW). The observed formation of the nearly closed circulation on 9 September is well timed with the passage of the convectively active phase of a CCKW, an event recently found to be associated with a reduction in climatological westerly shear. Similarly, the convectively suppressed phase of a CCKW served to temporarily suppress convection in the vicinity of the pre-Karl disturbance on 10-13 September. After the passage of the convectively suppressed phase of the CCKW, a less unfavorable environment allowed more persistent convection to develop, eventually leading to tropical cyclogenesis.
In order to utilize a gridded dataset that assimilated the PREDICT and GRIP dropsondes and maintained a high spatial resolution, operational ECMWF analyses were employed for the synoptic perspective. ERA-Interim reanalysis data are used in conjunction with filtered outgoing longwave radiation observations to track CCKW features for the equatorial wave perspective. The evolution of the vertical wind shear over pre-Karl and the storm's difficulty maintaining deep convection will be examined from both of these perspectives.
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