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Use of large-scale atmospheric energetics for understanding the dynamics of contrasting Indian summer monsoon rainfall in different years

机译:使用大规模的大气能量学,以了解不同年份印度夏季季风降雨对比的动态

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摘要

An attempt has been made to understand the dynamics of contrasting Indian summer monsoon rainfall (ISMR) in different years during 1979-2017, from large-scale atmospheric energetics aspects. Daily values of eddy and zonal available potential energy (APE), their generation, eddy and zonal kinetic energy (KE), conversions of zonal KE and eddy APE to eddy KE, and conversions of zonal APE to zonal KE and eddy APE were computed over the region bounded by 65 degrees E-95 degrees E and 5 degrees N-35 degrees N during the period 1 May to 30 September for 39years (1979-2017), using daily ECMWF reanalyzed atmospheric data at 0.125 degrees x0.125 degrees resolution (3 components of wind and temperature). ISMR was classified into three categories, viz., deficient and below normal, normal and above normal and excess. The daily anomaly of these energetics parameters in each of these years was computed using jackknife method and then the composite of the daily anomalies of these parameters constructed for the years with the above-mentioned three categories of ISMR. The following salient features emerge from this study: Analysis of composite anomaly shows that in case of excess and above normal (below normal and deficient) ISMR, C(A(Z), K-Z) was less (more) than normal. In case of excess and above normal (below normal and deficient) ISMR, C(A(E), K-E) was more (less) than normal. Broadly, C(A(Z), A(E)) was more than normal in the years with deficient and below normal ISMR, whereas it was less than normal for years with excess and above normal ISMR. Broadly, G(A(Z)) was below normal for the years with above normal and excess ISMR, whereas it was above normal for the years with below normal and deficient ISMR. Total kinetic energy and total conversion to eddy kinetic energy was above normal for the years with above normal and excess ISMR.
机译:已经尝试了解1979 - 2017年在不同年份的印度夏季季风降雨(ISMR)对比的动态,从大型大气能量方面。涡流和区域可用势能(APE)的日常值,它们的发电,涡流和Zonal动能(KE),Zonal Ke和Eddy猿的转换,以及Zonal Ape对Zonal Ke和Eddy APE的转化在5月1日至9月30日期间,在9月30日(1979-2017)期间,在5月30日(1979-2017)期间,在5月30日(1979-2017)中界定的区域,使用每日ECMWF重新分析的大气数据0.125度X0.125分辨率( 3个组成的风和温度)。 ismr被分为三类,viz,缺乏,正常,正常,正常和多余。这些年度在这些年份中的每日异常使用jackknife方法计算,然后通过上述三类ISMR构建这些参数的每日异常的组合。从本研究中出现以下显着特征:复合异常的分析表明,在过量且正常(正常且缺陷以下)的情况下,C(A(Z),K-Z)小于正常情况。在过量且高于正常(正常和缺陷以下)的情况下,C(a(e),k-e)比正常更高(少)。广泛而言,C(a(z),a(e))在缺乏且正常的ismr低于正常的年内,多年来少于正常,多年来少于正常ismr。广泛而言,G(A(Z))在正常正常和过量的ismr上的岁月下降低于正常,而在正常和缺乏低于ismr的年份,它在正常的正常情况下。在正常和过量的ISMR以上的多年来,总动能和对涡流能量的总转化率高于正常的正常情况。

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