风切变对边界层对流影响的大涡模拟研究

利用"西北干旱区陆-气相互作用野外观测实验"加密观测期间在敦煌站的观测资料以及大涡模式,模拟了对流边界层的发展,以及示踪物从混合层向残留层传输的时空变化。模拟的对流边界层的结构及演变特征与实测结果基本一致。进一步通过有风切变和无风切变的敏感性数值试验,研究了风切变对垂直速度、位温和示踪物浓度的水平分布以及示踪物传输高度的影响。研究结果表明,在有风切变的试验中(甚至风切变仅存在于近地层中),对流边界层的增长加强,而且示踪物被传输的高度也较高。与浮力驱动的对流边界层相比,由浮力和风切变共同驱动的边界层中上升气流较弱而下沉气流较强,但前者的上升气流与下沉气流的分布在垂直方向上更为倾斜。由于夹卷作用的增强,浮力和风切变共同驱动的对流边界层较浮力驱动的对流边界层暖。在夹卷层,浮力和风切变共同驱动的边界层对流的上升气流和下沉气流都比浮力驱动的边界层对流中的强,而且垂直速度的概率密度函数分布也较对称,其位温和示踪物浓度的概率密度函数分布也比浮力驱动的边界层中的平直。对湍流动能收支的分析也表明风切变对湍流动能有重要影响,尤其对夹卷层中的湍流动能切变产生项影响较大。示踪物浓度的概率密度函数垂直分布显示,浮力驱动的边界层中示踪物浓度随高度变化较小,而浮力和风切变共同驱动的边界层中示踪物浓度随高度递减,但是示踪物传输的高度比较高。     

高原东南缘大气近地层湍能特征与边界层动力、热力结构相关特征

基于云南省大理2008年3、5、7月GPS加密探空试验时段(14和02时)资料,结合边界层铁塔综合观测资料,采用温度梯度法、逆温强度法和涡动相关法分别计算高原东南缘对流边界层(convective boundary layer,CBL)及稳定边界层(stable boundary layer,SBL)顶高度,通过计算获取感热通量、潜热通量、湍流动能、切变项以及浮力项与大气动力、热力过程垂直相关特征综合分析,可发现湍能方程中浮力项、感热、潜热通量与NCEP再分析资料计算获取的大气视热源相关特征显著,这某种程度反映了高原东南缘近地层大气湍流动量、热量输送对低层大气视热源Q_1的重要贡献。低层视热源Q_1亦表现出与湍能方程分量类似的日变化周期,此特征反映了高原东南缘大气热源变化与下垫面水热过程及其湍流输送日变化密切相关;浮力项与湍能等项对大气低层热源与涡动特征、热力混合结构的形成有重要作用;低层大气视热源、水汽汇均与边界层高度有显著相关,综合分析结果某种程度描述了青藏高原东南缘近地层湍流动量、热量输送状况与低层大气热源,热力混合边界层结构的综合相关物理图像,初步探索了高原东南缘对流活跃区大气湍流运动与大气动力、热力过程相互作用特征。研究表明近地层湍流通量变化某种程度可反映未来局地大气视热源垂直结构变化的"强信号"特征。本文上述研究结论也可启发我们进一步关注近地层湍流通量异常变化特征及其对局地降水过程大气热源结构演变的影响问题。     

一次梅雨锋暴雨的边界层热通量输送与湍流动能收支分析

利用中尺度WRF模式对于2007年7月一次典型的梅雨锋暴雨过程进行了高分辨率数值模拟,对于边界层内的热通量输送和湍流动能的时空变化特征,以及湍流动能各收支项的分布及变化特征进行了分析。结果表明,降水发生时段内边界层热通量和湍流动能的时空分布特征与晴空日变化特征表现出显著不同,潜热通量随高度自下而上呈现"正—负—正"的分布,感热通量以负值为主,负值中心高度与潜热通量由负转正的高度相对应,湍流动能的发展高度与持续时间都有所增加,降水区近地面湍流动能弱于其他区域,但是在468 m以上高度则显著强于其他区域。降水区湍流动能的来源主要是平均风切变所产生的机械湍流,浮力作用与粘性耗散在降水期间消耗湍流动能,湍流输送作用将低层的湍流动能输送至较高的高度,使低层减小而高层增大,临界高度与湍流动能的大值中心高度对应。     

利用毫米波云雷达数据反演层云微物理参数和云内湍流耗散率

利用地基毫米波雷达进行云参数及云内湍流特性的探测和反演。根据云雷达回波的功率谱数据,反演出大气垂直运动速度和云微物理参数,得到云内湍流耗散率ε的大小和分布情况,并进一步研究和分析了云内空气垂直运动与云微物理参数、反射率因子、多普勒速度、速度谱宽变化的关系,更好地了解云的演变情况。对2016年8月8日四川稻城的一次层状云过程的探测和反演表明：1）粒子有效半径随着上升气流的增强而增大,由于碰并聚合的作用,粒子数浓度也呈现相应减小的趋势。2）云内湍流耗散率ε在云底、云顶较大,云内较小,量级在10^-8~10^-2 m²·s^-3,多普勒速度能谱验证了假设雷达探测湍涡的尺度在惯性副区的合理性。3）随着上升气流的增强,云粒子的下沉运动相应减小,速度谱宽相应增大。     

凝结潜热释放和地表热通量对一次飑线过程的影响

针对2013年7月4—5日一次产生大风、短时强降水强对流天气的飑线过程进行数值试验,研究了凝结潜热释放和地表热通量在中尺度对流系统的发生发展过程中的影响。结果表明:(1)凝结潜热释放对飑线系统有重要的作用,对飑线发展维持、移动及成熟阶段的垂直结构都有着一定影响。(2)当飑线系统进入成熟阶段后,小尺度的积云对流中的凝结加热作用于中高层大气,加强了高层辐散低层辐合的配置,而对流系统内垂直上升运动的加强又导致凝结加热作用更强。(3)凝结加热作用极大地促进了飑线的低层入流、高层出流的垂直结构,以及系统前方中层入流和高层出流之间形成的间接垂直反环流,促进高空动能下传的同时,使系统前方对流不稳定性增加,新的对流单体易于触发。(4)潜热释放间接增强了对流内部的冷性下沉气流,进而加强了低层的阵风锋,使得新的对流单体能在飑锋处触发,飑线以新老对流单体交替的方式向前移动。(5)在高低空急流的垂直耦合促进飑线发展的同时,成熟阶段飑线中较强的凝结加热对高低层急流有反馈作用,一定程度上增强了这种垂直耦合。(6)地表感热、潜热通量等边界层非绝热过程在对流系统的触发和发展中起到了较为重要的作用。地表热通量在白天加强了对流边界层的湍流混合作用,由此产生的特征维持到了夜间,形成了适合飑线触发的层结条件。另外,在对流形成之前,与地表潜热通量相关的边界层加湿作用为对流的爆发贮存了丰富的水汽和不稳定能量。     

青藏高原雷暴弱降水云微物理特征的卫星反演分析

选取青藏高原3个雷暴弱降水过程,以极轨卫星反演云微物理特征分析方法为主,结合地面实况和探空资料,探讨了云微物理特征及这类雷暴形成的可能原因.结果表明:(1)这类云的云底温度较低,为0℃左右,离地面1～2 km,属冷云底的对流云.与暖云底(云底温度15～20℃)相比,冷云底导致云中的水成物少,释放潜热少,这可能是该区域强...     

西南涡对流云中夹卷率的模拟研究

本文使用中尺度数值模式WRF(Weather Research and Forecasting Model)模拟了2010年7月8—9日发生在四川盆地的一次西南涡降水天气过程,并计算该过程中零度层以下对流云中的夹卷率。从云内垂直特征看:云内的含水量、垂直风速和浮力都在云底之上随高度递增,而在云顶附近随高度递减;云内的湿静力能则主要随高度递减;夹卷率在云底以上随高度递减,而在云顶附近随高度递增,但是云顶高度越高,在云顶附近的递增趋势越不明显。另外,夹卷率和云内的云水、雨水含量都呈负相关,说明夹卷抑制了对流云的发展以及地面降水。当假设被夹卷的环境空气来自云边界附近时,计算所得的夹卷率值要大于假设夹卷空气远离云边界所得值,但这两种假设中夹卷率的其他特征是类似的。从演变特征看,夹卷率总体上随时间减小,这和这段时间内对流云整体发展增高有关。     

防护林地区近地面层湍流结构及通量特征研究

本文采用在大面积防护林地区近地面边界层中采集的湍流、辐射和廓线梯度资料,计算并分析了湍流结构及通量特征。结果表明:当-0.1<ξ<0.1范围内时,湍流动能,湍流强度随稳定度变化迅速;位温宏观量σ/θ_*服从σ_θ/θ_*=A(-ξ)~(1/3)规律,A=0.60;在湍流混合强烈时,林网内下层出现负潜热通量现象,并且林网上层潜热通量明显大于下层;湍流热通量则相反。本文还对计算湍流热通量和潜热通量的方法的适用性也做了比较,并且分别进行了误差分析。     

不同边界层参数化方案对一次梅雨锋暴雨过程湍流交换特征模拟的影响

利用WRF模式结合不同的边界层参数化方案,对2007年7月3—5日发生在江淮流域的一次梅雨锋暴雨过程进行多组数值模拟试验。结果发现,边界层方案的选取对于降水的落区和强度模拟会产生较显著的影响;在降水率及地面要素的模拟上,各方案在降水中后期的模拟差异明显大于降水发生阶段;不同边界层方案的选取对于降水时段内的水平风场、垂直运动和假相当位温的垂直分布都产生影响,直接影响降水时空分布的模拟;不同方案都模拟出了在降水发生之后不同于晴空日变化的湍流动能垂直分布,经分析发现与局地较强的垂直风切变和近地面强湍流气团被抬升有关,而浮力项起着耗散作用;各方案的湍流交换特征与湍流动能特征基本吻合,相比于其他方案,MYJ方案在降水区域的湍流动能及湍流交换强度明显偏弱,对热通量的输送也偏弱;GBM方案在边界层内的湍流混合偏弱而在边界层以上湍流混合显著偏强,热通量输送在边界层以上的高度上误差明显,影响了对降水区域气象要素的模拟能力,仍需要进一步改进。      

鄱阳湖地区复杂地表条件下一次强降水过程的近地面边界层特征

使用鄱阳湖北部70 m气象塔湍流和梯度观测数据,分析了2011年6月6日夜间一次暴雨过程中近地面边界层特征.结果表明,此次过程是在高空低槽和西南急流的天气背景下,受鄱阳湖复杂地表影响产生的局地性强降水.强降水发生前受东南暖平流影响,近地面边界层中水汽累积,不稳定性增加;强降水过程中,近地层感热、潜热通量迅速增加,同时,近地面层湍流动量通量下传和水平输送增加,鄱阳湖的水汽输送加强降水强度.另外,强降水过程中,近地面湍流动能迅速增大并达到最大值,而平均动能的增大发生在强降水结束后,表明地表作用明显,近地面边界层的湍流场为暴雨提供动力条件.尺度分析表明,强降水前,中尺度动量通量占主要地位,降水过程中湍流动量通量显著加强.     

A cold air outbreak near Spitsbergen in springtime — Boundary-layer modification and cloud development

A moderate cold air outbreak from the Arctic ice over the warm West-Spitsbergen current on 15 and 16 May 1988 during the field experiment ARKTIS '88 is analysed using data from four aircraft and one research vessel.The downstream development of cloud coverage appears to depend sensitively on the moisture content above the inversion. The cloud amount determines the energy balance at the sea surface. Under daytime conditions and little cloud cover, energy is added to the ocean in spite of sensible and latent heat losses.The downstream temperature increase in the boundary layer is controlled by sensible heat flux and by longwave radiation cooling. The entrainment sensible heat flux is the dominating term in the region near the ice edge. The downstream moisture increase is controlled by surface evaporation. Condensation processes play no significant role.On 16 May 1988 cloud streets near the ice edge changed to closed cloud meanders in the downstream direction. The aspect ratio increased from 3 to around 10 over a distance of 200 km. In the cloud street region, the dynamical generation of turbulent kinetic energy due to wind shear at the tilted inversion was larger than the thermal generation.Cloud droplet concentration, mean droplet radius and liquid water content increased linearly with height. The maximum liquid water content was only 0.1 g/kg near the top of a 400 m thick closed cloud and clearly below the adiabatic value. The net longwave radiation flux decreased by 50 W/m² at cloud top and increased by 13 W/m² at cloud base.     

Current problems in the stratocumulus-topped atmospheric boundary layer

Extended sheets of stratocumulus (Sc) in the upper part of the atmospheric boundary layer (ABL) often occur under appropriate meteorological conditions. These cloud decks are important both in climate studies and in weather forecasting. We review the current knowledge of the turbulent structure of the ABL capped by a cloud deck, in the light of recent observations and model studies. The most important physical processes determining this structure are longwave radiative cooling at cloud top, shortwave radiative wanning by absorption in the cloud, surface buoyancy flux, and wind shear in the ABL. As a result, turbulence can cause entrainment against the buoyancy jump at cloud top. In cases where only longwave radiative fluxes and surface buoyancy fluxes are important, the turbulent structure is relatively well understood. When shortwave radiative fluxes and/or wind shear are also important, the resulting turbulent structure may change considerably. A decoupling of the cloud from the sub-cloud layer or of the top of the cloud from the rest of the ABL is then regularly observed. In no cases are the details of the entrainment at cloud top understood well enough to derive a relatively simple formulation that is consistent with observations. Cloud-top entrainment instability may lead to the break-up of a cloud deck (but also to cloud deepening). The role of mesoscale circulations in determining fractional cloudiness is not yet well understood.     

Heat fluxes and roll circulations over the western Gulf Stream during an intense cold-air outbreak

Turbulence and heat fluxes in the marine atmospheric boundary layer (MABL) for the roll vortex regime, observed during the Genesis of Atlantic Lows Experiment (GALE) over the western Gulf Stream, have been studied. The spectral analysis suggests that cloud streets (roll vortices) are vertically organized convection in the MABL having the same roll scale for both the cloud layer and subcloud layer, and that the roll spacing is about three times the MABL depth. The roll circulations contribute significantly to the sensible (temperature) and latent heat (moisture) fluxes with importance increasing upward. Near the MABL top, these fluxes are primarily due to roll vortices which transfer both sensible heat and moisture upward in the lower half of the convective MABL. Near the MABL top, the roll circulations transfer sensible heat downward and moisture upward in the clear thermal-street region, but roll vortices influenced by evaporative cooling can transfer sensible heat upward and moisture downward in the cloud-street region. Near the cloud-top, the upward buoyancy flux due to evaporative cooling is highly related to the roll circulations near the inversion.For the lower half of the MABL, the normalized temperature flux decreases upward more rapidly than the humidity flux, which is mainly because potential temperature () increases slightly upward while humidity (q) decreases slightly upward above the unstable surface layer. The gradient production (associated with the gradient) is a source for the temperature flux in the unstable surface layer but changes to a sink in the mixed layer, while the gradient production (associated with the q gradient) acts as a source for the humidity flux in both the unstable surface and mixed layers. The results suggest that the entrainment at the MABL top might affect the budgets of temperature and humidity fluxes in the lower MABL, but not in the unstable surface layer.Caelum Research Corporation, Silver Spring, MD, 20901, U.S.A.     

A numerical study of the marine stratocumulus cloud layer

A one-dimensional grid-level model including longwave radiative transfer and a level-4 second-order turbulent transfer closure which contains prognostic equations for turbulent quantities, is used to study the physics and dynamics of inversion-capped marine stratocumulus clouds.A set of numerical experiments had been performed to examined the role of sea surface temperature, large-scale vertical velocity, wind speed, and vertical wind shear in the formation and the structure of low-level clouds. For a given sea surface and geostrophic wind speed, stratocumulus clouds can grow higher with smaller large-scale subsidence as less dry air entrains into the cloud. Clouds grow higher with higher sea surface temperature for a given geostrophic wind speed and large-scale subsidence as a result of enhanced moist convection. In high wind speeds, the entire cloud deck is lifted up because of larger surface energy flux. In the budget studies of the turbulent kinetic energy (TKE), the buoyancy term is a major source term when the wind speed and the vertical shear are small across the inversion top. When the wind speed and the vertical wind shear across the inversion top become large, the mixed layer is decoupled into a cloud and a subcloud layer. In the TKE budget studies, the shear generation term becomes an important term in the budgets of the TKE and the variance of vertical velocity.     

Observation of a Self-Limiting,Shear-Induced Turbulent Inversion Layer Above Marine Stratocumulus

High-resolution measurements of thermodynamic, microphysical, and turbulence properties inside a turbulent inversion layer above a marine stratocumulus cloud layer are presented. The measurements are performed with the helicopter-towed measurement payload Airborne Cloud Turbulence Observation System (ACTOS), which allows for sampling with low true air speeds and steep profiles through cloud top. Vertical profiles show that the turbulent inversion layer consists of clear air above the cloud top, with nearly linear profiles of potential temperature, horizontal wind speed, absolute humidity, and concentration of interstitial aerosol. The layer is turbulent, with an energy dissipation rate nearly the same as that in the lower cloud, suggesting that the two are actively coupled, but with significant anisotropic turbulence at the large scales within the turbulent inversion layer. The turbulent inversion layer is traversed six times and the layer thickness is observed to vary between 37 and 85 m, whereas the potential temperature and horizontal wind speed differences at the top and bottom of the layer remain essentially constant. The Richardson number therefore increases with increasing layer thickness, from approximately 0.2 to 0.7, suggesting that the layer develops to the point where shear production of turbulence is sufficiently weak to be balanced by buoyancy suppression. This picture is consistent with prior numerical simulations of the evolution of turbulence in localized stratified shear layers. It is observed that the large eddy scale is suppressed by buoyancy and is on the order of the Ozmidov scale, much less than the thickness of the turbulent inversion layer, such that direct mixing between the cloud top and the free troposphere is inhibited, and the entrainment velocity tends to decrease with increasing turbulent inversion-layer thickness. Qualitatively, the turbulent inversion layer likely grows through nibbling rather than engulfment.     

华北一次暴雨过程中潜热对中尺度系统和降水影响的数值研究

针对2005年7月22日的发生于华北的暴雨中尺度对流系统,在用中尺度ARPS模式数值模拟和分析云场、动力场以及微物理过程释放的潜热垂直分布和作用特征的基础上,通过改变主要微物理过程潜热做敏感性数值试验,研究和分析了潜热对云系发展演变、云系宏观动力场、水汽场、云场和降水的影响,总结出云暖区潜热的影响途径。结果表明,在对流云团中,5000 m以上微物理过程起加热作用,以下起冷却作用。不同物理过程潜热加热的云层高度不同:高层起加热作用的主要为水汽凝结、云冰初生和雪凝华增长、霰撞冻云水过程;中层起加热/冷却作用的主要为水汽凝结、霰/雹融化过程;低层雨水的蒸发过程起冷却作用。微物理过程潜热通过影响云系和降水发展过程、云系动力场,进而影响水汽场、云场和降水。忽略霰/雹融化潜热,相当于增加云系暖区潜热,促进了低层气旋性环流的形成,增强了低层动力场的辐合,使得低层辐合区增多、增强;中低层水汽通量辐合区增多、面积扩大,明显地促进了对流云系的发展,增大了含水量和覆盖范围,云系的降水量显著增加,强降水区覆盖范围扩大。即使减少20%的凝结潜热,云系的发展也受到极大抑制,没有气旋性环流生成,低层辐合区缩小、强度降低,水汽通量辐合区也同样缩小、强度降低,云系对流发展减弱、含水量降低,因此,降水量大为减小,降水范围也显著缩小。此外,微物理过程潜热还影响到此次中尺度对流系统发展演变过程,改变了云系的形态、影响到系统的移动和系统中对流云团的发展强度和分布情况。     

Analysis on the Interaction between Turbulence and Secondary Circulation of the Surface Layer at Jinta Oasis in Summer

The kinetic energy variations of mean flow and turbulence at three levels in the surface layer were calculated by using eddy covariance data from observations at Jinta oasis in 2005 summer.It is found that when the mean horizontal flow was stronger,the turbulent kinetic energy was increased at all levels,as well as the downward mean wind at the middle level.Since the mean vertical flow on the top and bottom were both negligible at that time,there was a secondary circulation with convergence in the upper half and divergence in the lower half of the column.After consideration of energy conversion,it was found that the interaction between turbulence and the secondary circulation caused the intensification of each other.The interaction reflected positive feedback between turbulence and the vertical shear of the mean flow.Turbulent sensible and latent heat flux anomaly were also analyzed.The results show that in both daytime and at night,when the surface layer turbulence was intensified as a result of strengthened mean flow,the sensible heat flux was decreased while the latent heat flux was increased.Both anomalous fluxes contributed to the cold island effect and the moisture island effect of the oasis.     

利用TWP-ICE试验资料对比两种边界层参数化方案

利用高分辨率WRF单气柱模式,选取了两种边界层参数化方案(YSU,MYJ),对TWP-ICE(Tropical Warm Pool International Cloud Experiment)试验期间的个例进行数值模拟,比较了两种方案对边界层结构、云和降水模拟的影响。结果表明:季风活跃期,YSU方案模拟的湍流交换系数较小,湍流混合偏弱,边界层内热通量偏小,使地表热量和水汽不易向上输送,水汽含量在近地表明显偏多,而在边界层及其以上大气层具有显著的干偏差,因此该方案模拟的云中液态水和固态水含量偏低,云量偏少,降水率偏小;MYJ方案对于季风活跃期的边界层结构具有较好的模拟能力,其模拟的云和降水更为准确。季风抑制期,MYJ方案模拟的夜间边界层结构存在较大误差,这是因为该方案模拟的夜间湍流交换系数较大,湍流混合偏强,边界层内热通量偏大,模拟的位温和水汽混合比在边界层内随高度变化较小,而观测廓线在边界层内存在较大梯度。季风抑制期两种方案模拟的云和降水均比观测值偏多,方案之间的差异较小。     

‘Evolution of a Storm-driven Cloudy Boundary Layer in the Arctic’

To investigate the processes of development and maintenance of low-level clouds during major synoptic events, the cloudy boundary layer under stormy conditions during the summertime Arctic has been studied using observations from the Surface Heat Budget of the Arctic Ocean (SHEBA) experiment and large-eddy simulations (LES). On 29 July 1998, a stable Arctic cloudy boundary-layer event was observed after the passage of a synoptic low pressure system. The local dynamic and thermodynamic structure of the boundary layer was determined from aircraft measurements including the analysis of turbulence, cloud microphysics and radiative properties. After the upper cloud layer advected over the existing cloud layer, the turbulent kinetic energy (TKE) budget indicated that the cloud layer below 200 m was maintained predominantly by shear production. Observations of longwave radiation showed that cloud-top cooling at the lower cloud top has been suppressed by radiative effects of the upper cloud layer. Our LES results demonstrate the importance of the combination of shear mixing near the surface and radiative cooling at the cloud top in the storm-driven cloudy boundary layer. Once the low-level cloud reaches a certain height, depending on the amount of cloud-top cooling, the two sources of TKE production begin to separate in space under continuous stormy conditions, suggesting one possible mechanism for the cloud layering. The sensitivity tests suggest that the storm-driven cloudy boundary layer is possibly switched to the shear-driven system due to the advection of upper clouds or to the buoyantly driven system due to the lack of wind shear. A comparison is made of this storm-driven boundary layer with the buoyantly driven boundary layer previously described in the literature.     

层积云覆盖的边界层数值模拟研究(Ⅰ):数值模式的建立

层积云是一种在湍流作用下形成的边界层云,在这种边界层中,层积云顶即边界层顶,云层和非云层耦合在一起,为了加深对这种层积云覆盖的边界层的理解,许多作者已经做了大量的野外观测和数值试验研究,然而在数值模拟研究中存在湍流和云物理模式相互脱节的现象,针对这种缺陷,本文在湍流控制方程组中引入云滴控制方程,发展了一个新的用于研究海区层积云覆盖的边界层的数值模式,所建模式具有如下特点：（1）实现了云物理模式与湍流模式的相互耦合;（2）实现了云滴分档凝结模式和三阶湍流闭合边界层模式相互耦合,利用所建模式对大涡模拟对比试验所采用的个例进行了数值模拟,数值模拟结果表明,该边界层模式能较合理地模拟海区层积云覆盖的边界层微湍流结构和云微物理过程。