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1.
冬季城市边界层风场和温度场结构分析 总被引：15，自引：1，他引：15
本文根据沈阳地区大气环境容量研究中1984年12月所进行的观测,对沈阳城市边界层的流场和温度场结构做了分析。得出了冬季城市边界层的一些特征。当地面风速微弱时,热岛效应显著。边界层低层辐合抬升,在城市下风边缘可能出现反向气流。当风速较强时,城市的摩擦效应占优势,城市上风部分辐合抬升,下风部分辐散下沉。观测分析还表明,城市建筑对气流的阻滞作用可伸展到几百米的高度。夜间微风时,接地逆温层厚度可达200m,城市内边界层从上风边缘起开始发展,厚度可达100m。白天风力微弱时,重烟尘污染可导致城市冷岛,并推迟对流边界层的发展。 相似文献
2.
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3.
This paper analyses the meteorological numerical simulation in Paris during two days (March 10 and 13, 1995) observed during ECLAP (Etude de la Couche Limite en Agglomération Parisienne– the boundary-layer study of the Paris area), a recent measurement campaign over the Paris area, in which both in-situ and remote-sensing devices at urban and rural locations have been deployed in addition to the operational meteorological network. The chosen days are well documented and correspond to different meteorological situations leading to pollution events (regarding wind direction, cloud cover, surface and synoptic inversion strength).Comparisons of three-dimensional mesoscale model results with the ECLAP observation data are presented, focusing on the temperature field and turbulent fluxes along with the urban heat island and the evolution of the mixing height. It is shown that the model correctly reproduces the main characteristics of the temperature field, its diurnal evolution (near the ground and higher up) especially the gradient between Paris and the surrounding countryside. The mixing-height evolutions are in a good agreement with the observations and the model is also able to reproduce the turbulent features of the atmosphere. The small difference observed between the urban and rural mixing-height evolution is also well reproduced. 相似文献
4.
城乡过渡地带低空温度平流和边界层特征的观测分析 总被引：4，自引：0，他引：4
利用兰州河谷盆地城乡过渡区边界层观测资料,分析了该地区的温度平流和边界层特征。分析表明:(1)夜间热岛环流明显,白天则较弱;(2)夜间200m高度以下有较强的冷平流,在250～400m高度有较弱的暖平流,冷暖温度平流对测点上空边界层温度和层结变化有显著影响;(3)由声雷达确定的夜间边界层高度对应于Ri<1.0的高度,在这一高度范围内存在逆位温和强的风切变。本地区下垫面和复杂的地形导致夜间边界层高度随时间周期性地升高和降低,变化周期约3h。 相似文献
5.
R. M. Worthington 《Meteorology and Atmospheric Physics》2014,126(1-2):1-12
Early studies of mountain waves reported various results that have rarely been investigated since. These include: large-amplitude mountain waves above an unstable boundary layer much higher than the mountains; a repeated downwind drift and upwind jump of mountain waves; and larger vertical wind magnitude near sunrise and/or sunset. These are investigated using over 3,000 radiosondes and meso-strato-troposphere (MST) radar. Superadiabatic temperature gradients are found beneath mountain waves, explainable by convection which appears to raise the mountain-wave launching height. Movement of mountain-wave patterns is studied by a new method using height–time vertical wind data. A swaying motion of mountain waves, with period of a few minutes, appears to be equally upwind and downwind, rather than asymmetric at the heights measurable. Also, vertical wind shows no change in mean, variance or extreme values near sunrise and sunset, despite the expected diurnal changes of boundary-layer structure. An explanation for differences between MST radar and other measurements and models of mountain waves is suggested in terms of more than one variety of mountain wave. Type 1 has stable air near the ground; type 2 is above a convective/turbulent boundary layer of significant height as compared to the mountains. 相似文献
6.
An analytical framework is proposed for studying variations in the diurnal wind structure in the planetary boundary layer (PBL) and the evolution of the low-level nocturnal jet. A time-dependent eddy-diffusivity coefficient corresponding to solar input is proposed, and an appropriate coordinate transformation ensures that mixing height varies continuously with ground heat-flux changes. The solution exhibits the receding character of the daytime PBL as evening approaches, thereby dividing the PBL into two regimes — the one just above the ground, representing the nocturnal boundary layer, and the region above it. It is assumed that inertial oscillations (IO) are triggered in the upper layer at about the time of sunset when the reversal in the direction of ground heat flux is felt in the upper layer. Two approaches are adopted to determine the characteristic features of IO and the evolution of the nocturnal low-level jet. The first one is based on the physical principle that release of horizontal momentum due to deviation from the geostrophic wind gives rise to the IO. The solution captures all the characteristic features of the IO, such as phase shift and decreasing amplitude of the IO with increasing height. According to this analysis the IO is triggered at a level as soon as the top of the receding boundary layer leaves that level. The solution is discontinuous with respect to the vertical coordinate. In the second approach we solve an initial-value problem to determine the solution in the upper layer, assuming that at about the time of sunset there is a rapid collapse of the daytime PBL to the steady, nocturnal boundary layer. The assumption is based on the mixing-height profiles prepared from climatological data collected at Delhi. The solution for the nocturnal boundary-layer regime is then obtained as a boundary-value problem. The solutions so obtained are continuous throughout the domain of interest and exhibit the characteristic features of an IO. The analysis leads to the conditions under which a low-level nocturnal jet is produced and provides quantitative estimates of the parameters, such as length of night, latitude, mixing height at sunset and nocturnal mixing height, that are conducive to the generation of a jet. The nocturnal wind profile produced by this approach compares well both with typical atmospheric data observed at Delhi and with output from a mesoscale numerical model. There is still some uncertainty related to the time of initiation of the IO as a function of latitude. 相似文献
7.
A two-dimensional time-dependent Earth-atmosphere model is developed which can be applied to the study of a class of atmospheric boundary-layer flows which owe their origin to horizontal inhomogeneities with respect to surface roughness and temperature. Our main application of the model is to explore the governing physical mechanisms of nocturnal urban atmospheric boundarylayer flow.A case study is presented in which a stable temperature stratification is assumed to exist in the rural upwind area. It is shown through integration of the numerical model that as this air passes over a city, the heat is redistributed due to increased surface friction (and hence increased turbulent mixing). This redistribution of heat results in the formation of an urban heat island.Additional numerical integrations of the model are conducted to examine the dependence of induced perturbations on: (1) the upwind temperature inversion; (2) the geostrophic wind speed; and (3) urbanization. The results show a linear relationship between heat-island intensity and the rural temperature inversion with the heat island increasing in intensity as the upwind inversion becomes stronger; that the heat-island intensity close to the surface is inversely proportional to the geostrophic wind; and that the effects of anthropogenic heat cause an increase in the perturbation temperature with the perturbation extending to higher altitudes. From this study, we conclude that with an upwind temperature inversion, a city of any size should generate a heat island as a result of increased surface roughness. The heat-island intensity should increase with city size because of two factors: larger cities are usually aerodynamically rougher; and larger cities have a larger anthropogenic heat output.Research supported in part by NSF Grant GA-16822. 相似文献
8.
Summertime Mixing Heights At Vienna, Austria, Estimated from Vertical Soundings and by a Numerical Model 总被引：1，自引：1，他引：0
Martin Piringer 《Boundary-Layer Meteorology》1998,89(1):25-45
Mixing heights calculated by the Danish OML meteorological pre-processor are compared to those diagnosed from radio- and tether-sonde vertical potential temperature profiles. All methods give reliable estimates of noon mixing heights deduced from radiosoundings, especially when the boundary layer is fully convective. Differences are larger during convective conditions without a well-defined capping inversion in the radiosonde potential temperature profile or when OML calculates a mechanical mixing height. The OML model is also able to calculate the daily course of the mixing height as expected. The tethersonde-derived mixing heights are especially valuable during the morning rise of the elevated inversion. Modifications to all three methods to improve mixing-height predictions are discussed. 相似文献
9.
夜间城市大气边界层和气溶胶的相互作用 总被引：5，自引：1，他引：5
本文利用能量闭合的二维非线性、非定常模式，结合地面热量平衡方程，研究了夜间城市边界层和气溶胶的相互作用问题。结果表明:气溶胶在夜间对大气低层起保温作用，对大气上层起冷却作用；使大气低层稳定度减小，上层稳定度增加；此外，气溶胶还能够削弱贴地逆温强度。在正常城市气溶胶污染情况下，气溶胶对城市热岛强度影响不大，但可使城市热岛环流稍有增加。夜间城市边界层对气溶胶的反馈作用使大气下层气溶胶浓度减小，上层气溶胶浓度增加。上述部分结论得到了在天津取得的城市热岛观测资料的直接验证。 相似文献
10.
Numerical Study of Winter Urban Boundary Layer Structure over Beijing Area 总被引：1，自引：0，他引：1 
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下载免费PDF全文 1. Introduction The urban canopy layer (UCL) (Roth, 2000) is defined as a layer in the vertical structure of urban boundary layer (UBL) ranging from the surface to the top of buildings. The urban infrastructures within UCL, such as buildings with different heights, the het- erogeneity of urban land cover and the anthropogenic activity, all directly influence the thermal and dynam- ical structures of atmosphere and net radiation budget at the surface, meanwhile, affect the structure of ur- … 相似文献
11.
This study deals with the variability of mixing height during daylight hours in the summer months for weak wind regimes. A two-dimensional model was employed using simulated input variables which are quite representative of conditions found over the midwestern United States in late summer and early fall. With the aid of this model and various analytical techniques, the dependence of the urban mixing height on such factors as horizontal advection, downward heat flux across the stable mixing-layer interface, lapse rate in the stable layer, etc., was delineated and compared with actual mixing height variations observed in St. Louis, Missouri during selected days for August, 1972.The experiment indicated the following: (1) A spatially symmetric surface heating profile over a city is accompanied by a similarly symmetric mixing-height profile in the absence of vertical wind shear; (2) When the same heating assumption is invoked and vertically variable wind profiles are introduced, the model-generated mixing-height contours become increasingly asymmetric with vertical wind shear; (3) The modelled mixing heights are more sensitive to temperature fluctuations than to those of wind over the range of speeds studied (wind speeds 4ms–1); (4) Present operational methods of predicting the time of erosion of an inversion (based upon forecast surface temperature ranges and adiabatic diagram considerations) underestimate breakup time by a factor which is proportional to the amount of available downward heat flux from the stable layer into the mixed layer below. 相似文献
12.
Two fair weather afternoons have been examined, where the urban boundary layer over St. Louis, though exhibiting similar thermal characteristics, had a markedly different kinematic structure. The turbulent nature of the boundary layer was examined through analysis of double theodolite wind profiles at an urban and at a rural site on each day. On 14 July 1975, the winds increased with height above the inversion at both sites and on the following day, the winds decreased above the boundary layer in the same region. While the mean wind speed in the lowest 0.8 km agl was similar on both days, the turbulence characteristics of the urban boundary-layer winds were distinctly different on these two afternoons. This was evidenced by the variance of the wind and is in agreement with simultaneous aircraft measurements reported by Hildebrand and Ackerman (1984). A similar difference in turbulence was not found over the rural site. It is suggested that the enhanced turbulence at the urban site on 14 July is likely associated with the wind profile immediately above the boundary layer, where the downward flux of high momentum air from above the inversion may have resulted in stronger mechanical mixing within the boundary layer. 相似文献
13.
北京冬季城市边界层结构形成机制的初步数值研究 总被引：7，自引：1，他引：6
利用耦合了城市冠层参数化方案的MM5模式对2001年冬季北京地区一次典型的城市边界层过程进行成功模拟的基础上,对北京城市化作用、周边地形以及城市化进程发展对城市边界层结构的影响等问题进行了一系列的数值模拟试验。城市化作用的因子分离试验发现,城市化的总体作用即城市下垫面结构对大气热力及动力的综合影响导致了北京冬季城市边界层结构主要特征的形成。此外,揭示了城市结构的不同影响因子———动力因子、热力因子和热动力因子间的相互作用在北京冬季城市边界层结构形成和演变过程中的不同作用。在夜间,城市结构的动力因子对于城市边界层主要特征如市区悬浮逆温、近地层中小的风速及较强的湍流动能等的形成起着主导作用;在白天,城市结构的热力因子则成为影响市区混合层强度以及湍流运动特征等边界层结构的主导因素;热、动力因子间的相互作用对城市边界层结构的形成和演变也有着重要作用,但其影响特征比较复杂。北京周边地形作用的敏感性试验的结果表明,北京周边的特殊地形条件对城市边界层热力结构特征如悬浮逆温层及城市热岛等的结构及分布特征的形成也有着明显的影响,使其具有特殊的局地化特征,同时,它也是北京地区近地层主要气流特征的强迫源。不同城市化程度的敏感性试验结果揭示,随着北京城市建筑高度和密度的增加,市区风速将减小、湍流动能将加强,夜间城市悬浮逆温层底的高度会有所提高,城市热岛的强度也将加强,并可能在白天出现比较明显的城市热岛效应。 相似文献
14.
J. D. Kalma 《Boundary-Layer Meteorology》1974,6(3-4):351-361
It is shown with simple two-dimensional advective models that artificial heat generation in the Sydney area, on early mornings in July, is largely responsible for the downwind temperature increase over the city. The models predict the height of the mixing layer and also the temperature increase downwind which agrees favourably with observations. The models require the following information: (1) average wind speed, (2) lapse rate difference between the stable upwind atmosphere and the air layer over the city, (3) the upwind surface temperature, (4) the vertical thermal diffusivity upwind, and (5) artificial heat generation. Data on energy use in the Sydney area have been presented elsewhere. A sensitivity analysis has been performed to study the interaction between the input parameters and their role in modifying the city's atmospheric boundary layer. 相似文献
15.
Operation of a monostatic acoustic sounder on the campus of The University of Calgary for the period March to September, 1976, has provided data on the atmospheric boundary layer over Calgary. The formation and dissipation of the nocturnal temperature inversion layer leaves a clear signature in the sounder records. A trend is discerned in which the nocturnal layer tends to form at sunset, whereas convective instability is established some 2–3 hours after sunrise. Comparison of sounder records with an extensive set of radiosonde temperature profiles has shown that the height of the inversion layer can be determined reliably when a single, dark, ground-based return is visible on the sounder charts. On many occasions, however, the sounder detects multiple structures in the atmosphere. In these cases, it is difficult to establish a systematic correspondence of the turbulent structure as observed in the sounder records with the temperature profile as observed by the radiosonde. 相似文献
16.
Summary The effects of atmospheric boundary-layer stability on urban heat island-induced circulation are numerically and theoretically
investigated using a nonlinear numerical model (ARPS) and a two-layer linear analytical model. Numerical model simulations
show that as the boundary layer becomes less stable, a downwind updraft cell induced by the urban heat island strengthens.
It is also shown that as the boundary layer becomes less stable, both the height of the maximum updraft velocity and the vertical
extent of the downwind updraft cell increase. Hence, in the daytime with a nearly neutral or less stable boundary layer the
urban heat island-induced circulation can become strong, even though the urban heat island is weak. It is suggested that these
findings can be a mechanism for urban-induced thunderstorms observed in the late afternoon or evening with a nearly neutral
or less stable boundary layer. The boundary-layer stability affects the spatial distribution of scalar concentration through
its influencing urban heat island-induced circulation. Analytical results from a two-layer model with different boundary-layer
stabilities in the lower and upper layers are in general qualitatively consistent with the numerical simulation results, although
the low-level maximum vertical velocity does not change monotonically with lower-layer stability. 相似文献
17.
In this work, the thermic structure of the atmospheric boundary layer is analyzed by means of direct measurements with radiosonde equipment, remote exploration with a three-monostatic Doppler sodar, and a boundary layer model of order one-and-a-half. Intercomparisons of radiosonde data, sodar data, and model results are made through the study of radiative nocturnal inversion, subsidence inversion, development and height of the mixing layer, and calculus of the temperature structure parameter. The ability of sodar to find the mixing layer height and to detect stable layers is enhanced when these layers are low enough. 相似文献
18.
Radiative destabilization of the nocturnal stable atmospheric boundary layer (NSABL) over homogeneous desert terrain is predicted by an analytical model based on a modified diffusion equation. The model applies late at night under calm, dry conditions when long-wave radiative transfer dominates the NSABL evolution. A three-layer structure for the NSABL is proposed: a shear sub-layer closest to the surface, a radiative sub-layer which contains the inversion top, and a coupling sub-layer which matches the NSABL with the residual layer aloft. A sub-sub-layer called the nocturnal internal boundary layer (NIBL) is nested within the radiative sub-layer and comprises the temperature maximum. The model can explain: (1) maximum cooling in the NIBL, (2) deepening of the NIBL, (3) radiative destabilization of the NSABL, and (4) possible surface warming before sunrise. An example from the Mohave Desert, USA is presented, and the observed temperature profile compares favorably with the model solution. 相似文献
19.
采用对数压力坐标系的大气热力、动力方程组，分析了由于城市的加热和摩擦作用，在大气层结不稳定情况下的热岛环流，给出了表征热岛基本特征的垂直运动，水平运动和温度场的空间结构，从理论上证实了热岛环流在不稳定城市边界层中存在的可能性，并得出了如下主要结论:(1) 垂直运动在市区是上升运动，在郊区是下沉运动，在低层z=150m处有一闭合中心；(2) 流场在市区上空呈一层波动，波谷在上风区，波峰在下风区，波长为城市半宽的4倍；(3) 地面的高温区出现在城市的下风区，且无逆温层出现。 相似文献
20.
Viviane S. Guerra Otávio C. Acevedo Luiz E. Medeiros Pablo E. S. Oliveira Daniel M. Santos 《Boundary-Layer Meteorology》2018,166(3):395-422
The study of the boundary layer can be most difficult when it is in transition and forced by a complex surface, such as an urban area. Here, a novel combination of ground-based remote sensing and in situ instrumentation in central London, UK, is deployed, aiming to capture the full evolution of the urban boundary layer (UBL) from night-time until the fully-developed convective phase. In contrast with the night-time stable boundary layer observed over rural areas, the night-time UBL is weakly convective. Therefore, a new approach for the detection of the morning-transition and rapid-growth phases is introduced, based on the sharp, quasi-linear increase of the mixing height. The urban morning-transition phase varied in duration between 0.5 and 4 h and the growth rate of the mixing layer during the rapid-growth phase had a strong positive relationship with the convective velocity scale, and a weaker, negative relationship with wind speed. Wind shear was found to be higher during the night-time and morning-transition phases than the rapid-growth phase and the shear production of turbulent kinetic energy near the mixing-layer top was around six times larger than surface shear production in summer, and around 1.5 times larger in winter. In summer under low winds, low-level jets dominated the UBL, and shear production was greater than buoyant production during the night-time and the morning-transition phase near the mixing-layer top. Within the rapid-growth phase, buoyant production dominated at the surface, but shear production dominated in the upper half of the UBL. These results imply that regional flows such as low-level jets play an important role alongside surface forcing in determining UBL structure and growth. 相似文献