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The vertical structure of cloud radiative heating over the Indian subcontinent during summer monsoon

机译:夏季季风在印度次大陆云辐射加热的垂直结构

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Clouds forming during the summer monsoon over the Indian subcontinent affect its evolution through their radiative impact as well as the release of latent heat. While the latter is previously studied to some extent, comparatively little is known about the radiative impact of different cloud types and the vertical structure of their radiative heating/cooling effects. Therefore, the main aim of this study is to partly fill this knowledge gap by investigating and documenting the vertical distributions of the different cloud types associated with the Indian monsoon and their radiative heating/cooling using the active radar and lidar sensors onboard CloudSat and CALIPSO. The intraseasonal evolution of clouds from May to October is also investigated to understand pre-to-post monsoon transitioning of their radiative heating/cooling effects. The vertical structure of cloud radiative heating (CRH) follows the northward migration and retreat of the monsoon from May to October. Throughout this time period, stratiform clouds radiatively warm the middle troposphere and cool the upper troposphere by more than ±0.2 K day?1 (after weighing by cloud fraction), with the largest impacts observed in June, July and August. During these months, the fraction of high thin cloud remains high in the tropical tropopause layer (TTL). Deep convective towers cause considerable radiative warming in the middle and upper troposphere, but strongly cool the base and inside of the TTL. This cooling is stronger during active (?1.23 K day?1) monsoon periods compared to break periods (?0.36 K day?1). The contrasting radiative warming effect of high clouds in the TTL is twice as large during active periods than in break periods. These results highlight the increasing importance of CRH with altitude, especially in the TTL. Stratiform (made up of alto- and nimbostratus clouds) and deep convection clouds radiatively cool the surface by approximately ?100 and ?400 W m?2 respectively while warming the atmosphere radiatively by about 40 to 150 W m?2. While the cooling at the surface induced by deep convection and stratiform clouds is largest during active periods of monsoon, the importance of stratiform clouds further increases during break periods. The contrasting CREs (cloud radiative effects) in the atmosphere and at surface, and during active and break periods, should have direct implications for the monsoonal circulation.
机译:在夏季季风形成的云层在印度次大肿的季风中通过辐射的影响影响其演变以及潜热的释放。虽然先前在某种程度上研究了后者,但对不同云类型的辐射撞击和其辐射加热/冷却效果的垂直结构表示相对较少。因此,本研究的主要目的是通过研究和记录与印度季风和辐射加热/冷却的不同云类型的垂直分布来部分填补这种知识差距,以及使用Cloudsat和Calipso的激光器传感器的辐射加热/冷却。还研究了5月至10月份云的季节性进展,以了解其辐射加热/冷却效果的初期季风过渡。云辐射加热(CRH)的垂直结构沿着5月至10月的北方迁移和季风撤退。在这段时间段内,层状云辐射中间对流层,并冷却上层对流层超过±0.2克(云分数后),在6月,7月和8月观察到最大的影响。在此期间,热带对流层层(TTL)中的高薄云的分数保持高。深层对流塔在中上层和上层辐射相当辐射,但强烈冷却底座和TTL内部。与断裂期相比,这种冷却在活跃(?1.23k日?1)季风期间更强(?0.36 k日?1)。高云在TTL中的对比辐射变暖效果在活动期间的两倍大于中断时期。这些结果突出了CRH与高度的越来越重要,特别是在TTL中。层状(由Alto-and Nimbostratus云组成)和深对流云分别通过大约α100和?400Wm≤2辐射表面,同时将气氛辐射地辐射大约40至150wm≤2。虽然深对流和层状云引起的表面的冷却在季风的活动期间最大,而层状云的重要性在断裂期间进一步增加。大气和表面的对比度Cres(云辐射效应)以及在活性和断裂周期期间应该对季透血管产生直接影响。

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