城市下垫面反照率变化对北京市热岛过程的影响——个例分析   总被引：13，自引：1，他引：13  

江晓燕  张朝林高华　苗世光 《气象学报》2007,65(2):301-307

随着城市的不断发展,城区地表反照率等下垫面物理特征和属性会发生明显的变化,进而会对城市热岛等大气环境形成影响。文中使用中国气象科学研究院开发的新一代数值天气预报模式(GRAPES),针对2004年10月北京一次重空气污染事件中的典型城市热岛过程,分别设计了两种数值试验方案:(1)对照试验,使用模式缺省的城区下垫面反照率参数,取值0.18;(2)敏感性试验,参考同期中国科学院大气物理研究所铁塔280m高度下垫面反照率观测事实,将北京区域城市类型下垫面反照率减小至0.15。通过对比两种试验方案在1km水平分辨率下的24h模拟结果,研究了城市下垫面反照率变化对北京地区城市热岛过程的影响。结果表明:(1)GRAPES模式可成功模拟此次热岛过程中城区和郊区近地面温度的日变化趋势;(2)城市下垫面反照率的变化对城市热岛的发展非常重要,城市反照率下降0.03会使城市热岛强度增强0.8℃左右,结果也更接近实况。这说明随着城市发展引起的地表反照率减小有利于城市热岛强度增加;(3)通过分析地表的长波辐射发现,在城市区域较小反照率情形下,城区的长波辐射始终比郊区大,有利于热岛的形成;同时也有利于城区近地层的风场辐合增加,对此次污染过程的发展是有利的。  相似文献   

估算地表热通量和近地层土壤含水量的变分方法   总被引：1，自引：0，他引：1  

张述文邱崇践  张卫东 《气象学报》2007,65(3):440-449

提出一种反演地表感热通量、潜热通量和近地层土壤含水量的变分方法,该方法把不同高度上的风速、位温以及湿度梯度的观测资料与Monin-Obukhov相似理论计算值的偏差、土壤水分蒸发参数化方案估算的蒸发潜热与由相似理论导出值的偏差在地表能量平衡的约束下融合到一个目标泛函数中,采用最优化算法寻求问题的解。利用2001年6月中国暴雨试验与研究项目在安徽肥西观测资料进行了数值验证,结果表明:该方法估算的通量值与Bowen比法具有很好的相关性且又能克服当Bowen比等于-1时计算通量出现的不稳定;同时能克服用廓线法求解热通量与地表能量平衡条件有较大出入的缺点。对观测误差的敏感性试验也表明变分方法是3类方法中最稳定的。反演的近地层土壤含水量对降水具有很好的响应并与观测的0—15 cm深度上平均土壤湿度的变化趋势具有很好的一致性,其绝对偏差小于0.03 m3/m3。  相似文献   

Roles of Mesoscale Terrain and Latent Heat Release in Typhoon Precipitation： A Numerical Case Study     

李昀英  黄伟  赵焦枝 《大气科学进展》2007,24(1):35-43

The mesoscale orographic effects on typhoon Aere＇s precipitation are simulated using an Advanced Regional Eta-coordinate Model （AREM） version 3.0. In particular, the effects of the latent heat release are studied by two comparable experiments： with and without condensational heating. The results show that the typhoon rainfall is tripled by the southeastern China mesoscale terrain, and the condensational heating is responsible for at least half of the increase. One role of the latent heat release is to warm the atmosphere, leading to a depression of the surface pressure, which then causes a larger pressure difference in the zonal direction. This pressure gradient guides the water vapour to flow into the foothills, which in turn amplifies the water vapour flux divergence amplified, causing the typhoon rainfall to increase eventually. The other role of the latent heat release is to make the convection more organized, resulting in a relatively smaller rain area and stronger precipitation.  相似文献   

A Note on the Role of Meridional Wind Stress Anomalies and Heat Flux in ENSO Simulations     

朱杰顺  孙照渤  周广庆 《大气科学进展》2007,24(4):729-738

Four comparative experiments and some supplementary experiments were conducted to examine the role of meridional wind stress anomalies and heat flux variability in ENSO simulations by using a high-resolution Ocean General Circulation Model （OGCM）. The results indicate that changes in the direction and magnitude of meridional wind stress anomalies have little influence on ENSO simulations until meridional wind stress anomalies are unrealistically enlarged by a factor of 5.0. However, evidence of an impact on ENSO simulations due to heat flux variability was found. The simulated Nino-3 index without the effect of heat flux anomalies tended to be around 1.0° lower than the observed, as well as the control run, during the peak months of ENSO events.  相似文献   

鲁北平原地下咸水浅层地热能开发利用条件研究     

赵季初  纪洪磊  刘欢 《中国地质调查》2020,7(3):13-20

为了解决鲁北平原区农村冬季清洁供暖问题,扩大地下水地源热泵系统的应用规模,以区内广泛发育的咸水体为研究目标,在简述第四纪地层特征的基础上,阐明了第四纪含水砂层与咸水体的分布特征,总结了区内以往开展的4个浅层地热能勘查项目所施工的水文地质勘探孔抽水试验与回灌试验成果。结果表明: 研究区咸水含水层单井涌水量320~475 m³/d,单位涌水量12.76~28.3 m³/(d·m),自然回灌条件下单井回灌量30~56 m³/d,单位回灌量5.85~17.5 m³/(d·m); 单眼开采井可供暖面积为3 481.02 m²,可满足约35户农村住宅的冬季供暖需求; 研究区在进行浅层地热能开发时建议优先选择地下水地源热泵系统,对于供暖/制冷能耗需求较小的农村单户建筑,可选择地埋管地源热泵系统进行分散式供暖/制冷。  相似文献   

胶西北金成矿区He、Ar同位素组成及成矿流体来源研究     

王金辉 《岩石矿物学杂志》2020,39(2):172-182

胶东半岛西北地区是我国重要的金成矿区,主要受三山岛断裂、焦家断裂、招平断裂带控制。为探讨3条主要成矿带成矿流体的来源与区别,对成矿带内典型矿床载金黄铁矿中流体包裹体进行了He、Ar同位素测试。结合前人数据表明三山岛成矿带3He/4He均值为1.95 Ra,焦家成矿带^3He/^4He均值为1.74 Ra,招平成矿带^3He/^4He均值为1.54 Ra,从西往东逐渐降低,说明地幔流体参与成矿自西往东逐渐降低。黄铁矿流体包裹体中放射性成因Ar所占比例范围三山岛成矿带1.17%~87.12%,平均33.04%,焦家成矿带15.57%~90.00%,平均55.75%,招平成矿带7.94%~92.69%,平均44.23%,说明在成矿过程中,地壳成矿流体参与成矿作用焦家成矿带最高,招平成矿带次之,三山岛成矿带最低。结合H、O稳定同位素研究,认为成矿流体主要来源于地壳,并有地幔流体加入,具地壳流体和地幔流体混合特征,上升过程中可能还有少量大气降水的参与。  相似文献   

High-velocity stars from decay of small stellar systems     

L. G. Kiseleva    J. Colin    B. Dauphole  & P. Eggleton 《Monthly notices of the Royal Astronomical Society》1998,301(3):759-766

In this paper we present numerical results on the decay of small stellar systems under different initial conditions (multiplicity 3 ≤  N  ≤ 10, and various mass spectra, initial velocities and initial configurations). The numerical treatment uses the CHAIN1 code (Mikkola &38; Aarseth). Particular attention is paid to the distribution of high-velocity escapers: we define these as stars with velocity above 30 km s⁻¹. These numerical experiments confirm that small N -body systems are dynamically unstable and produce cascades of escapers in the process of their decay. It is shown that the fraction of stars that escape from small dense stellar systems with an escape velocity greater than 30 km s⁻¹ is ∼1 per cent for all systems treated here. This relatively small fraction must be considered in relation to the rate of star formation in the Galaxy in small groups: this could explain some moderately high-velocity stars observed in the Galactic disc and possibly some young stars with relatively high metallicity in the thick disc.  相似文献   

Stream overflow and dwarf nova eruptions     

M. R. Schreiber  & F. V. Hessman 《Monthly notices of the Royal Astronomical Society》1998,301(3):626-630

We consider the effects of accretion stream overflow on the viscous dynamics of accretion discs in dwarf novae. If the stream from the secondary star is geometrically thick enough, some fraction of its material can flow over and under the disc. The mass and specific angular momentum of the stream are then deposited not only at the point of collision with the outer disc, but also at those radii in the inner disc with geometric heights that are large enough to intercept the residual stream, or near the radius where the disc has the same specific angular momentum as the stream. The overflowing stream can alter the behaviour of heating fronts and cooling fronts in the disc. If the mass fraction of the overflowing stream is of order tens of per cent, the deposition of mass in the inner parts of the disc is sufficient to change the character of the eruption light curves significantly.  相似文献   

The destructive effects of binary encounters on red giants in the Galactic Centre     

Melvyn B. Davies  Richard Blackwell  Vernon C. Bailey  & Steinn Sigurdsson 《Monthly notices of the Royal Astronomical Society》1998,301(3):745-753

We consider the destructive effects of encounters between binaries and red giant stars in the Galactic Centre. Such encounters may explain the observed depletion of luminous red giants within the central 0.2 pc of the galaxy. We consider encounters involving 2- and 8-M⊙ red giants, and thus span the range of stellar masses contributing to the most luminous red giants observed in the Galactic Centre. To explore the phase space of encounters thoroughly, we simulate 18 × 10³ encounters using a modified four-body code in which the red giant core and components of the binary are treated as point masses, and where the envelope configuration is assumed to remain static throughout the encounter. We then rerun a small number of encounters with a smoothed particle hydrodynamics (SPH) code to confirm the reliability of conclusions drawn from the four-body runs. We see two possible pathways to red giant destruction. A large fraction of encounters lead to the formation of common-envelope systems, where two compact objects (drawn from the red giant core and the components of the original binary) form a binary within a common gaseous envelope, whilst the third body is ejected. The destruction of the red giant will then follow when the envelope is ejected as the binary hardens. In a smaller number of encounters, the intruding binary passes through the star and ejects the red giant core from the envelope. The red giant envelope will then disperse on short time-scales. We compute the time-scales for both of these processes to occur in the Galactic Centre for a variety of binary populations.  相似文献   

The tilt of the Fundamental Plane of early-type galaxies: wavelength dependence     

M. Scodeggio    G. Gavazzi    E. Belsole    D. Pierini  & A. Boselli 《Monthly notices of the Royal Astronomical Society》1998,301(4):1001-1018

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