共查询到17条相似文献，搜索用时 171 毫秒
1.
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。 相似文献
2.
GOALS模式中大气能量循环的诊断分析与不同版本计算结果的比较研究 总被引：5，自引：1，他引：4
利用大气能量循环框图,对比分析中国科学院大气物理研究所大气科学与地球流体力学数值模拟国家重点实验室(LASG/IAP)全球海-陆-气耦合系统模式(GOALS)两个版本(GOALS-2和GOALS-4),以及观测的全球平均大气能量循环的主要特征,并从能量循环贮蓄和转换项的纬向平均贡献去解释全球积分值改善和转坏的原因,以及诊断分析参数化方案变化后产生的影响.结果表明:模式的两个版本基本上能正确地模拟出全球能量循环的主要特征.旧版本GOALS-2能较好模拟全球积分值,常常是不同符号局地误差的相互抵消结果.新版本GOALS-4中某种局地过程的改善在一些情况下导致了全球积分值的转坏.引入辐射日变化参数化方案可能对能量循环各参数的局地贡献有着明显的影响.如纬向平均有效位能向瞬变涡动有效位能的斜压转换率、瞬变涡动有效位能向瞬变涡动动能的斜压转换率以及定常涡动动能的局地贡献有明显改善.南极地区不合实际的上升运动,是模拟的纬向平均有效位能与纬向平均动能之间的转换项全球积分值为负数的主要原因. 相似文献
3.
利用北京中国科学院大气物理研究所325 m气象观测塔的气象梯度资料和湍流资料,分析了2014年11月29日至12月5日北京两次大风过程中气象要素和湍流输送特征的变化。第一次大风过程的强度和持续时间均高于第二次大风过程。强烈的风速垂直切变主要集中在距地面100 m高度范围内,最强风速垂直切变达到0.31 s~(-1)。大风过程中,阵风系数呈现随高度减小的趋势,越接近地面,阵风系数愈大。阵风强度的变化与阵风系数相似,100 m以下高度时,阵风强度随高度增大而减小。大风过程自上而下改变边界层结构,平均动能、湍流动能和摩擦速度最先从上层(280 m)发生变化且迅速增加。近地层由于风速垂直梯度的显著差异,近地层垂直方向的湍流强度最大。大风时各功率谱在低频区(0.01 s~(-1))达到峰值,大风过后各高度的能量都有所下降。 相似文献
4.
试探大气边界层湍流运动的若干问题 总被引：2，自引：0，他引：2
对湍流运动的几个基本理论问题作了一定程度的探讨，并根据湍流动能方程分析了大气边界层湍流产生和发展的能量机制，以此为判据推导了滴运动的凡主范围和物理含意较为清楚的混合长表达式。 相似文献
5.
研究了数值天气预报模式中次阿格湍流垂直扩散过程的参数化问题。以Ｂｏｕｇｅａｕｌｔ和Ｌａｃａｒｒｅｒｅ（１９８９）的参数化方案为基础，改进了处理湍流混合长的方法，使湍流混合长和热力混合长分别依赖于基本气流的静力稳定度和风场切变。新方案的基本思路是把ＶｏｎＫａｒｍａｎ（１９３０）提出的动力（风场切变）湍流扰动假设与ＢＬ－８９方案提出的热力（静力稳定度）湍流扰动假设结合在一起，强调了大气的热力结构、动力结构和湍流动能对湍流混合过程的共同影响。新方案和ＢＬ－８９方案的二维对比数值试验结果表明，在大气处于静力较稳定而风场切变明显条件下的湍流扰动表现能力方面，新方案比原方案有明显的改进。 相似文献
6.
为评估Monin-Obukhov相似理论和涡度相关系统在高标准农田的适用性,利用南通高标准农田水稻下垫面涡度相关观测数据,分析了大气稳定度、湍流方差相似性、湍流谱特征、湍流强度和湍流动能等。结果表明：该高标准稻田上方大气呈现白天不稳定、夜晚稳定的昼夜变化特征;Monin-Obukhov相似理论在该高标准农田适用,三维风速归一化标准差随大气稳定度的变化符合“1/3”次方规律,温度、比湿、CO2密度归一化标准差随大气稳定度的变化在大气不稳定时符合“1/3”次方规律;在惯性子区,三维风速的湍流能谱符合“-2/3”次方斜率,垂直风速与温度、湿度和CO2密度的协谱符合“-4/3”次方斜率,可见涡度相关系统能够观测该高标准农田的水热和CO2通量;三个方向上的湍流强度均随风速增大而减小,且水平方向湍流强度大于垂直方向;湍流动能随风速呈二次函数增大,呈现昼高夜低的日变化特征,大气中性时达到最大,且以动力湍流贡献为主。研究结果可为揭示华东地区高标准农田生态系统与大气之间的物质和能量交换特征以及机制提供参考。 相似文献
7.
本文利用中国自动站与CMORPH（Climate Prediction Center Morphing technique for the production of global precipitation estimates）融合的逐时降水量0.1°网格数据集资料挑选出一次典型的梅雨锋暴雨个例,运用WRF中小尺度模式进行模拟,对模拟得到的高分辨率结果进行Barnes滤波,最后将滤波结果代入动能和位能方程中,目的是定量地分析各个尺度能量的变化以及它们之间的相互作用对暴雨强度的影响。研究发现:模式模拟的降水过程和强度与实况较为吻合,推导的能量方程适用于这次暴雨过程。三种尺度能量之间的相互作用包含了各种跨尺度能量的相互作用。在整个暴雨过程中,跨尺度之间的斜压能量转换包括位能向动能的能量转换和动能向位能的能量转换。同尺度之间的斜压能量转换总是单向的,且量值较大,动能的强度主要靠位能向动能的能量转换来维持。斜压能量转换的多少影响着暴雨的强弱。大尺度斜压能量转换在中高层比较强,中尺度斜压能量转换在低层较强,尤以β中小尺度系统变化最为显著,β中小尺度系统扰动是影响暴雨强度的关键系统。风切变的大小影响各尺度动能之间的能量转换。温度或位温梯度的大小影响各尺度位能之间的能量转换。位能与动能之间的能量转换主要与各尺度垂直速度和温度的垂直分布有关,暖空气上升冷空气下沉是各个尺度位能向动能转换的主要过程。 相似文献
8.
长江三角洲常熟地区近地层湍流特征的研究 总被引：3，自引：0，他引：3
利用1999年5～9月长江三角洲常熟地区的湍流脉动观测资料,分析了该地区感热、潜热和动量通量的日变化以及湍流强度和湍流谱特征,结果表明该地区各能量的日变化与常见情况相同,白天潜热通量的输送占主导地位,感热通量比潜热小得多,且湍流的日变化与天气的关系非常密切,晴天比阴天要大得多.湍流强度和湍流谱的分析结果表明,在近中性条件下,常熟地区各方向湍流强度接近典型平坦下垫面的值.非中性条件下,垂直方向规一化标准差与稳定度的关系都较好地满足1/3次幂定律,水平方向没有垂直方向上的规律好,特别是稳定条件下,数据点分散性大;各风速分量谱在高频段满足理论上的-2/3次幂定律,纵向和垂直方向速度谱的峰值频率与典型平坦下垫面上的结果一致.总体输送系数CD、CH与稳定度的关系密切,随稳定度增加有减小的趋势. 相似文献
9.
长江三角洲常熟地区近地层湍流特征的研究 总被引：5，自引：1，他引：5
利用1999年5－9月长江三角洲常熟地区的湍流脉动观测资料，分析了该地区感热，潜热和动量通量的日变化以及湍流强度和湍流谱特征，结果表明：该地区各能量的日变化与常见情况相同，白天潜热通量的输送占主导地位，感热通量比潜热小得多，且湍流的日变化与天气的关系非常密切，晴天比阴天要大得多。湍流强度和湍流谱的分析结果表明，在近中性条件下，常熟地区各方向湍流强度接近典型平坦下垫面的值。非中性条件下，垂直方向规一化标准差与稳定度的关系都较好地满足1／3次幂定律，水平方向没有垂直方向上的规律好，特别是稳定条件下，数据点分散性大；各风速分量变在高频段满足理论上的－2／3次幂定律，纵向和垂直方向速度谱的峰值频率与典型平坦下垫面上的结果一致，总体输送系数CD，CH与稳定度的关系密切，随稳定度增加有减小的趋势。 相似文献
10.
本文基于海陆风环流的形成机制,在研究分析海陆风环流形成的物理模型基础上,建立了海陆风环流的数学模型。根据此基础,以大连地区海陆风环流为计算实例,模拟了海陆风形成的压力场、速度场、温度场和湍流动能场的日变化及太阳辐射日变化的过程地面的能量变化及导致的湍流动能的变化,预测出海陆风环流的水平湍流扩散系数和动量、温度和湍流动能的垂直湍流扩散系数,为求解海陆风中的污染物扩散浓度以进行环境污染损失评价提供参考。应用此模型,对大连地区的海陆风环流进行了数值模拟,定性与定量地给出了海陆风场中的速度、压力、温度及湍流动能分布情况和主要参数值。结果表明,海陆风环流的大气压力场局地日变化较小,温度场变化较明显。在中午前后,动量、温度和湍流动能的垂直扩散系数达到了最大值。模拟结果与其他文献模拟结果的对比表明,本文建立的模型模拟与实验的结果相符,但预测精度仍需要进一步检验。 相似文献
11.
The effects of an air-temperature inversion in the atmosphere and a seawater density jump in the ocean on the structure of the atmospheric and oceanic boundary layers are studied by use of a coupled model. The numerical model consists of a closed system of equations for velocities, turbulent kinetic energy, turbulent exchange coefficient, local turbulent length scale, and stratification expressions for both air and sea boundary layers. The effects of the temperature inversion and the density jump are incorporated into the equations of turbulent kinetic energy of the atmosphere and ocean by a parameterization. A series of numerical experiments was conducted to determine the effects of various strengths of the inversion layer and surface heat fluxes in the atmosphere and of the density-jump layer in the ocean on the structure of the interacting boundary layers.The numerical results show that the temperature inversion in the atmosphere and density jump in the ocean have strong influences on turbulent structure [especially on the turbulent exchange coefficient (TEC) and turbulent kinetic energy (TKE)] and on air-sea interaction characteristics. Maxima of TKE and TEC strongly decrease with increasing strength of the inversion layer, and they disappear for strong inversions in the atmosphere. Certain strengths (density differences between the upper and the lower layers) of the density-jump layer in the ocean (2 0.1 g/cm3) produce double maxima in TEC-profiles and TKE-profiles in the ocean. The magnitudes of air-sea interaction characteristics such as geostrophic drag coefficient, and surface drift current increase with increasing strength of the density-jump layer in the ocean. The density-jump layer plays the role of a barrier that limits vertical mixing in the ocean. The numerical results agree well with available observed data and accepted quantitive understanding of the influences of a temperature inversion layer and a density-jump layer on the interacting atmospheric and oceanic boundary layers. 相似文献
12.
The Signature of Sea Spray in the Hexos Turbulent Heat Flux Data 总被引：7，自引：0，他引：7
The role of sea spray intransferring heat and moisture across the air-sea interface has remained elusive. Some studies have reported that sea spray does not affect the turbulent air-sea heat fluxes for 10-m wind speeds up to at least 25 m s-1, while others have reported important spray contributions for wind speeds as low as 12 m s-1. One goal of the HEXOS (Humidity Exchange over the Sea) program was to quantify spray's contribution to the turbulent air-sea heat fluxes, but original analyses of the HEXOS flux data found the spray signal to be too small to be reliably identified amid the scatter in the data. We look at the HEXOS data again in the context of the TOGA-COARE bulk flux algorithm and a sophisticated microphysical spray model. This combination of quality data andstate-of-the-art modelling reveals a distinct spray signature in virtually all HEXOS turbulent heat flux data collected in winds of 15 m s-1 and higher. Spray effects are most evident in the latent heat flux data, where spray contributes roughly 10% of the total turbulent flux in winds of 10 m s-1 and between 10 and 40% in winds of 15–18 m s-1. The spray contribution to the total sensible heat flux is also at least 10% in winds above 15 m s-1. These results lead to a new, unified parameterization for the turbulent air-sea heat fluxes that should be especially useful in high winds because it acknowledges both the interfacial and spray routes by which the sea exchanges heat and moisture with the atmosphere. 相似文献
13.
The influence of an idealized moving wavy surface on the overlying airflow is investigated using direct numerical simulations (DNS). In the present simulations, the bulk Reynolds number is Re = 8000 (; where U0 is the forcing velocity of the flow, h the height of the domain and v the kinematic viscosity) and the phase speed of the imposed waves relative to the friction velocity, i.e., the wave age varies from very slow to fast waves. The wave signal is clearly present in the airflow up to at least 0.15λ (where λ is the wave length) and is present up to higher levels for faster waves. In the kinetic energy budgets, pressure transport is mainly of importance for slow waves. For fast waves, viscous transport and turbulent transport dominate near the surface. Kinetic energy budgets for the wave and turbulent perturbations show a non-negligible transport of turbulent kinetic energy directed from turbulence to the wave perturbation in the airflow. The wave-turbulent energy transport depends on the size, tilt, and phase of the wave-induced part of the turbulent Reynolds stresses.According to the DNS data, slow waves are more efficient in generating isotropic turbulence than fast waves.Despite the differences in wave-shape as well as in Reynolds number between the idealized direct numerical simulations and the atmosphere, there are intriguing similarities in the turbulence structure. Important information about the turbulence above waves in the atmosphere can be obtained from DNS—the data must, however, be interpreted with care. 相似文献
14.
Satellite observations of SSTs have revealed the existence of unstable waves in the equatorial eastern Pacific and Atlantic oceans. These waves have a 20-40-day periodicity with westward phase speeds of 0.4-0.6 m s-1 and wavelengths of 1000-2000 km during boreal summer and fall. They are generally called tropical instability waves (TIWs). This study investigates TIWs simulated by a high-resolution coupled atmosphere-ocean general circulation model (AOGCM). The horizontal resolution of the model is 120 km in... 相似文献
15.
为了深入理解非静力近似下的波-湍相互作用问题,本研究在σ坐标的海洋环境研究和预报模型(MERF)中引入常用的Mellor-Yamada两方程湍混合参数化方案(MY2.5),评估垂向湍混合对小尺度背风波传播过程的影响.瞬时状态场的模拟结果表明,无论是否为非静力近似条件,上述湍参数化方案的引入都会减弱背风波传播的模拟效果.从时间平均场的试验结果来看,垂向湍混合过程会显著减小非静力近似和静力近似之间的差异.此外,能量收支分析的诊断结果表明,MY2.5方案会显著抑制陆坡地形下的背风波传播过程,进而将更多的潮能转化到不可逆的湍混合过程中. 相似文献
16.
G. S. GOLITSYN 《大气科学进展》2009,26(3):585-598
The goal of this paper is to quantitatively formulate some necessary conditions for the
development of intense atmospheric vortices. Specifically, these criteria are discussed for tropical
cyclones (TC) and polar lows (PL) by using bulk formulas for fluxes of momentum, sensible heating,
and latent heating between the ocean and the atmosphere. The velocity scale is used in two forms: (1)
as expressed through the buoyancy flux b and the Coriolis parameter lc for rotating fluids convection,
and (2) as expressed with the cube of velocity times the drag coefficient through the formula for
total kinetic energy dissipation in the atmospheric boundary layer. In the quasistationary case the
dissipation equals the generation of the energy. In both cases the velocity scale can be expressed
through temperature and humidity differences between the ocean and the atmosphere in terms of the
reduced gravity, and both forms produce quite comparable velocity scales. Using parameters b and lc,
we can form scales of the area and, by adding the mass of a unit air column, a scale of the total
kinetic energy as well. These scales nicely explain the much smaller size of a PL, as compared to
a TC, and the total kinetic energy of a TC is of the order 1018-1019 J. It will be shown
that wind of 33 m s-1 is produced when the total enthalpy fluxes between the ocean and the
atmosphere are about 700 W m-2 for a TC and 1700 W m-2 for a PL, in association with
the much larger role of the latent heat in the first case and the stricter geostrophic constraints
and larger static stability in the second case. This replaces the mystical role of 26oC as
a criterion for TC origin.
The buoyancy flux, a product of the reduced gravity and the wind speed, together with the atmospheric
static stability, determines the rate of the penetrating convection. It is known from the observations
that the formation time for a PL reaching an altitude of 5--6 km can be only a few hours, and a day, or
even half a day, for a TC reaching 15--18 km. These two facts allow us to construct curves on the plane
of Ts and ΔT=Ts-Ta to determine possibilities for forming an intense vortex. Here, Ta is the atmospheric temperature at the height z=10 m. A PL should have ΔT>20oC in accordance
with the observations and numerical simulations. The conditions for a TC are not so straightforward but
our diagram shows that the temperature difference of a few degrees, or possibly even a fraction of a
degree, might be sufficient for TC development for a range of static stabilities and development times. 相似文献
17.
Turbulent Dissipation Rate In The Boundary Layer Via Uhf Wind Profiler Doppler Spectral Width Measurements 总被引：2，自引：0，他引：2
B. Campistron S. Bernard B. Bénech F. Ardhuin-Girard J. Dessens E. Dupont B. Carissimo 《Boundary-Layer Meteorology》2002,103(3):361-389
The study is focused on the retrieval and validation of the turbulent kinetic energy dissipation rate from spectral width measurements made by a UHF wind profiler in the convective atmospheric boundary layer. The possibility to deduce , which is one of the most important parameters for boundary-layer study and monitoring, from Doppler radar spectral width measurements has a firm theoretical basis established by numerous earlier works. However, the major drawback of this approach lies in various meteorological and instrumental sources of non-turbulent spectral width broadening which have to be recognised and accounted for. In the first part of the study, the theoretical background of the retrieval is detailed and all possible causes of spectral broadening are listed and evaluated. In the second part, the method is applied to four days of UHF diurnal boundary-layer observations, collected during the TRAC-98 experiment, for which in situ aircraft measurements were available. Comparison between radar-retrieved and in situ aircraft measurements yields a fairly good agreement with a linear correlation coefficient of about 0.9 and a residual bias less than 2 × 10-4 m2 s-3. The analysis of derived from vertical and off-zenith observation leads to the recommendation, that in the boundary layer, where the wind is usually moderate, data collected by off-zenith beams should be used. Indeed, the measurement of the vertical spectral width, less affected by the large-scale broadening factor, can still be altered by the ground clutter removal. 相似文献