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首页> 外文期刊>Journal of the Atmospheric Sciences >The Diurnal Cycle of West Pacific Deep Convection and Its Relation to the Spatial and Temporal Variation of Tropical MCSs
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The Diurnal Cycle of West Pacific Deep Convection and Its Relation to the Spatial and Temporal Variation of Tropical MCSs

机译:西太平洋深对流的日循环及其与热带MCSs时空变化的关系

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摘要

Infrared (IR) and visible satellite data from the Japanese Geostationary Meteorological Satellite (GMS-4) with 5-km spatial and 1-h temporal resolution were used to examine the diurnal cycle of deep convection over a sector of the tropical west Pacific warm pool bounded by 0 deg -20 deg N, 140 deg E-180 deg. Data were analyzed for 45 days of summer from 22 June to 5 August 1994 and for 65 days of winter between 28 November 1994 and 31 January 1995. Deep convective clouds were identified in IR imagery using brightness temperature (T_(BB)) threshold techniques. Based on previous studies, a -65 deg C cloud-top T_(BB) threshold was chosen to isolate pixels containing active, deep convection. Spectral analysis of time series constructed from hourly cold cloud (<= -65 deg C) pixel counts revealed a powerful diurnal cycle of deep convection significant at the 95% confidence level during summer and winter. Composited hourly statistics of fractional areal cloud cover documented a 0500-0600 local standard time (LST) maximum with a 1500-1900 LST minimum of convection for both seasons. Objective analysis techniques were developed to analyze the phase and amplitude of the diurnal cycle of deep convection and its relation to the satellite-observed daily spatial and temporal variation of tropical mesoscale convective systems (MCSs). Results showed that the diurnal cycle of convective rainfall with an early morning maximum was disproportionately dominated by the largest approx 10% of MCSs for each time period. While the number of large MCSs increased only slightly throughout nocturnal hours, the area of cold cloud associated with these systems expanded dramatically. An algorithm called "threshold initiation" showed that all scales of organized, intensifying deep convection existed at all times of day and night. In addition, the early morning peak was largely composed of building convection. Conditional recurrence probabilities of deep convection associated with MCSs were computed at 24- and 48-h intervals. Results for summer and December 1994 revealed that when early morning convection associated with a large MCS occurred at any location, the same region contained convection the next morning nearly half the time. Convection was less likely at the 48-h point. These results are not consistent with diurnal theories based on sea surface heating, afternoon initiation of convection, and nocturnal evolution of mesoscale convective systems. Findings indicate that the diurnal cycle of deep convective cloud is driven by the internal variation of large clusters. MCSs embedded in cloud clusters that exist into or form during the night grow spatially larger and more intense. Some results support direct radiative forcing of clouds and large-scale clear-region radiative destabilization as possible contributors to diurnal convective variability. However, all findings are consistent with the work of Gray and colleagues that emphasizes the role of day-night variations in net tropospheric cooling in clear and longwave cooling in cloudy versus clear regions as an explanation of the observed daily variation of tropical convective rainfall and its significant relationship to organized mesoscale convection.
机译:来自日本对地静止气象卫星(GMS-4)的红外(IR)和可见卫星数据,具有5 km时空分辨率和1 h时空分辨率,用于检查热带西太平洋暖池部分深对流的昼夜周期以0度-20度N,140度E-180度为边界从1994年6月22日至1994年8月5日的夏季45天以及从1994年11月28日至1995年1月31日的冬季65天的数据进行了分析。使用亮度温度(T_(BB))阈值技术在红外图像中识别出了深对流云。根据先前的研究,选择了-65℃的云顶T_(BB)阈值来隔离包含活动深对流的像素。由每小时冷云(<= -65摄氏度)像素计数构成的时间序列的频谱分析显示,深对流的强大昼夜周期在夏季和冬季均达到95%的置信度。分数面云覆盖的每小时综合统计数据记录了两个季节的最大对流时间为0500-0600 LST,最小对流时间为1500-1900 LST。开发了客观分析技术,以分析深对流昼夜周期的相位和幅度,以及与卫星观测的热带中尺度对流系统(MCSs)每日时空变化的关系。结果表明,在每个时间段中,对流降雨的昼夜周期不成比例地由最大的MCS所占比例最大。在夜间,大型MCS的数量仅略有增加,而与这些系统相关的冷云面积却急剧增加。一种称为“阈值起始”的算法表明,白天和黑夜的所有时间都存在着各种规模的有组织的,加剧的深度对流。另外,清晨的高峰很大程度上是由对流造成的。与MCS相关的深对流的条件复发概率以24和48小时间隔计算。 1994年夏季和1994年12月的结果表明,在任何位置发生与大型MCS相关的清晨对流时,第二天早晨同一时间的对流区域几乎占一半。在48小时时,对流的可能性较小。这些结果与基于海面加热,对流的下午启动和中尺度对流系统的夜间演变的昼夜理论不一致。结果表明,深对流云的日循环是由大星团的内部变化驱动的。嵌入存在于夜间或在夜间形成的云集群中的MCS在空间上会变得更大且更密集。一些结果支持云的直接辐射强迫和大规模的净区辐射不稳定,这可能是昼夜对流变化的可能原因。但是,所有发现均与Gray及其同事的工作相一致,后者强调昼夜变化在对流层净降温在多云和晴空地区晴空和长波降温中的作用,解释了热带对流降水及其每日观测值的每日变化。与有组织的中尺度对流有重要关系。

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