Validation for a tropical belt version of WRF: sensitivity tests on radiation and cumulus convection parameterizations

对基本气候态和降水日变化的分析是检验模式模拟性能、理解模式误差来源的重要手段。为了评估出对热带气候模拟效果较好的物理参数化方案组合,本文应用WRF带状区域模式,主要比较了四种积云对流参数化方案:NewTiedtke、Kain-Fritsch、newSAS、Tiedtke,和两种辐射参数化方案:RRTMG和CAM,对热带带状区域的气候模拟结果。研究表明:使用NewTiedtke积云对流参数化方案和RRTMG辐射方案的试验,表现出对气温、降水及降水日变化等综合性最好的模拟性能;NewTiedtke积云对流参数化方案能模拟出较好的降水空间分布和降水日变化位相分布特征;与RRTMG辐射方案相比,CAM辐射方案会使温度模拟偏低,特别是陆地上更明显,这种陆地上的冷偏差可能主要来源于Tmin的模拟偏冷。     

青海高原致灾性对流天气时空分布特征

利用2005-2016年青海高原地面观测、灾情和卫星云图等资料,对青海高原致灾性对流天气进行筛选和分类,在此基础上分析了各类致灾性对流天气的时空分布特征及与地形的关系。结果表明:(1)青海高原致灾性对流主要有雷暴、短时强降水、冰雹以及混合类四种,集中分布于高原东部。(2)地形对致灾性对流的落区、频次和强度起关键作用。雷暴多产生于山区,短时强降水和冰雹主要产生在迎风坡、河谷和地势较开阔的低地。其中,青东农区以混合类和冰雹居多,青南牧区以混合类居多,环湖与祁连地区和柴达木盆地以短时强降水居多。(3)近12 a青海高原致灾性对流整体呈波动式减少,2005-2010年(前期)致灾性对流日数和次数较多,2011-2016年(后期)显著减少,但不同类型年际变化特征略有差异。其中,冰雹和雷暴日数前期较大,后期显著减少;混合类和短时强降水日数无明显变化趋势,但前者年际波动幅度较后者大。(4)致灾性对流主要产生于5-9月,各类型均呈现典型的单峰型月分布,混合类和冰雹日数及次数的峰值均在8月,雷暴日数和次数的峰值均在6月,而短时强降水日数和次数的峰值分别在8月、7月。(5)致灾性对流集中产生于13:00至次日01:00,高峰时段(16:00-20:00)以冰雹和混合类居多,而夜间时段以短时强降水居多。     

江淮梅雨期极端对流微物理特征的双偏振雷达观测研究

为研究梅雨期极端对流系统的微物理特征,利用2013—2014年江淮梅雨期间南京溧水S波段双偏振雷达探测资料和地面自动站小时降水资料,统计分析了两类极端对流降水系统的微物理特征及差异。这两类极端对流系统的定义基于地面降水强度和雷达回波顶高,分别为所有对流中降水强度最强的1%（R类:小时降水强度>46.2 mm/h）和对流发展高度最高的1%（H类:20 dBz回波顶高>14.5 km）。结果显示这两类极端对流系统仅有30%的样本重合,显示了二者之间的弱相关性。对于相同的反射率因子Z_H,R类极端对流系统的近地面差分反射率因子Z_DR通常较H类极端对流小约0.2 dB,表明R类极端对流具有较小的平均粒径。结合双偏振雷达反演的粒子大小和相态分布显示,虽然两类极端对流都表现出海洋性对流降水特征,但R类极端对流较H类极端对流的总体雨滴粒径更小而数浓度更高,导致R类极端对流系统的地面降水更强。与R类极端对流系统相比,H类极端对流系统的上升运动更强,将更多的水汽和过冷水输送到0℃层以上,有利于形成更大的冰相粒子（如霰粒子等）,并通过融化形成大雨滴。以上研究表明,梅雨期降水强度和对流发展深度并没有必然的联系,极端降水主要是中等高度的对流引起。      

Main Detrainment Height of Deep Convection Systems over the Tibetan Plateau and Its Southern Slope

Deep convection systems (DCSs) can rapidly lift water vapor and other pollutants from the lower troposphere to the upper troposphere and lower stratosphere. The main detrainment height determines the level to which the air parcel is lifted. We analyzed the main detrainment height over the Tibetan Plateau and its southern slope based on the CloudSat Cloud Profiling Radar 2B_GEOPROF dataset and the Aura Microwave Limb Sounder Level 2 cloud ice product onboard the A-train constellation of Earth-observing satellites. It was found that the DCSs over the Tibetan Plateau and its southern slope have a higher main detrainment height (about 10?16 km) than other regions in the same latitude. The mean main detrainment heights are 12.9 and 13.3 km over the Tibetan Plateau and its southern slope, respectively. The cloud ice water path decreases by 16.8% after excluding the influences of DCSs, and the height with the maximum increase in cloud ice water content is located at 178 hPa (about 13 km). The main detrainment height and outflow horizontal range are higher and larger over the central and eastern Tibetan Plateau, the west of the southern slope, and the southeastern edge of the Tibetan Plateau than that over the northwestern Tibetan Plateau. The main detrainment height and outflow horizontal range are lower and broader at nighttime than during daytime.     

利用FY-2F快速扫描资料分析对流初生阶段的云顶物理量特征

基于FY-2F静止气象卫星提供的2015年5—9月的高分辨率数据,通过温度阈值法识别出深、浅对流后,分析和比较了深、浅对流在对流初生(convective initiation,CI)至发展阶段中云顶高度、云顶快速降温率(cloud top cooling rate,CTC)以及多通道差值等云顶物理量特征的变化异同。结果表明:深、浅对流在CI阶段的云顶物理量特征具有相似变化特征,即云顶高度均在短时间内快速上升,CTC值均先减小后增大;深、浅对流差异表现为深(浅)对流云顶上升高度能(不能)超越水汽层高度;深对流CTC最低值较浅对流CTC最低值更低。基于CI阶段深、浅对流的CTC最低值的差异,通过个例验证,表明利用深、浅对流CTC最低值的差异,可以在识别出CI的基础,判断出CI是否发展成为深对流,从而能提前做出预警。     

2018年一次罕见早春飑线大风过程演变和机理分析

2018年3月4—5日,华南、江南等地发生了一次大范围强对流过程,发生时间早,落区范围广,多地伴有雷暴大风、冰雹、短时强降水等剧烈对流天气,尤其飑线在江西境内造成了严重大风灾害。基于大气环流和雷达回波发展演变特征,将该次过程分为初始、发展和减弱三个阶段：初始阶段西风槽前西南急流造成的低压倒槽为强对流提供大尺度触发条件;发展阶段对流活动位于槽前暖区中,飑线在江西造成极端大风;入夜后,冷锋南下,对流进入减弱阶段。环境场及对流参数诊断表明江西中北部低层高温高湿,中层干冷,温度垂直递减率大,有利于产生雷暴大风。南昌探空长时间序列分析表明温湿要素气候态异常,与历史同期比,低层明显偏暖偏湿,中层偏干,有利于极端对流天气发生。综合多源观测资料和雷达资料分析中小尺度特征,本次江西飑线过程特点及成因包括：（1）受引导气流和前向传播共同作用,飑线移动速度快。（2）自动站分析显示飑锋后雷暴高压强,与锋前暖低压作用造成强密度流,有利于产生大范围直线型大风;（3）通过对比飑线弓状回波南北段回波结构差异表明,飑线后侧中层干后向入流促使降水粒子相变,剧烈降温形成的强下沉运动(下击暴流)是导致极端大风的主要原因,后部层云区下沉气流增强雷暴高压加之动量下传作用对雷暴大风有增幅作用。     

Large-scale convective dynamos in a stratified rotating plane layer

We study the effect of stratification on large-scale dynamo action in convecting fluids in the presence of background rotation. The fluid is confined between two horizontal planes and both boundaries are impermeable, stress-free and perfectly conducting. An asymptotic analysis is performed in the limit of rapid rotation (τ???1 where τ is the Taylor number). We analyse asymptotic magnetic dynamo solutions in rapidly rotating systems generalising the results of Soward [A convection-driven dynamo I. The weak field case. Philos. Trans. R. Soc. Lond. A 1974, 275, 611–651] to include the effects of compressibility. We find that in general the presence of stratification delays the efficiency of large-scale dynamo action in this regime, leading to a reduction of the onset of dynamo action and in the nonlinear regime a diminution of the large-scale magnetic energy for flows with the same kinetic energy.     

A nonlinear stability analysis of convection in a generalized incompressible fluid

Abstract

We establish a nonlinear stability result for convection in a generalized incompressible fluid. Both numerical calculations and an asymptotic analysis are carried out. The linear and nonlinear results are shown to be very close in both cases, implying that the region of possible subcritical instabilities is very small.

During this work I was supported by a research studentship awarded by the Science and Engineering Council of the United Kingdom.     

Two-and three-dimensional linear convection in a rotating annulus

Abstract

An exceptional case to the model-independent theory of Knobloch (1995) is presented, by investigating a rotating cylindrical annulus of height H and side wall radii r _o and r _i, with non-slip, perfectly thermally conducting side walls and thermally insulating stress-free ends. Radial heating permits the possibility of either two- or three-dimensional convective solutions being the preferred mode. An analytical solution is obtained for the two-dimensional case and a numerical solution for the three-dimensional solution, which is also applied to the two-dimensional solution. It is shown that both two- and three-dimensional solutions can be realized depending on the aspect ratio, γ = H/d, where d = r _o-r _i is the thickness of the annulus, the radii ratio λ = r _i/r _o and the rotation rate of the model. For γ = O(1) and λ = 0.4, the preferred convective solution is three-dimensional when the Taylor number, T < 10² and two-dimensional for T > 10². For small aspect ratios, γ ? 1, the preferred mode is two-dimensional for all rotation rates.     

渤海海效应暴雪的三维热力结构特征

采用烟台多普勒天气雷达、天气图等观测资料和中尺度模式(RAMS4.4)进行数值模拟,分析了2008年12月4~6日发生的一次海效应暴雪的时空分布和三维热力结构特征。结果表明:(1)渤海海效应降雪并非传统认为的仅发生在蓬莱以东的山东半岛地区,而是广泛分布于山东半岛、莱州湾、渤海中东部和黄海西部洋面上;降雪源地有暖海面和陆地,即莱州湾、渤海中部至渤海海峡和山东半岛。(2)浅层对流是海效应降雪的重要热力特征,当强冷空气流经渤海时,暖海面通过湍流交换等作用向冷空气底层输送感热和潜热,使得低层增温增湿,产生对流层中上层干冷低层暖湿的对流性不稳定。(3)冷空气的强弱影响渤海暖海面及山东半岛地区的垂直热力结构,导致降雪强度在不同时段存在显著差异。海气温差与热通量成正比,初期冷空气弱,对流层中低层的垂直温差小,海面上空的暖湿层浅薄,不稳定能量弱,产生的降雪量小;中后期冷空气强盛,对流层中低层的垂直温差大,暖湿层较为深厚,不稳定能量增强,导致降雪强度和降雪量大。(4)与单一要素温度和湿度相比,对流层低层相当位温的水平分布对强降雪落区具有更好的指示意义,强降雪发生在高相当位温脊线附近。