北京夏季城市热岛现状及楔形绿地规划对缓解城市热岛的作用

通过遥感技术与地面测定相结合的方法，对北京城市热岛现状作观测研究，得到北京城市地面的温度分布特点。使用北京大学城市边界层模式从气象观点就“楔形绿地”规划对北京城市气候的影响进行研究和评价，模式通过对城市地表复杂性和多样性的特征进行细致描述，建立了一个细致模拟城市特点的城市边界层能量平衡模式，并用此能量平衡模式得到的地面温度作为下边界条件，中尺度气象模式MM5做初始场和侧边界条件，建立一个最小分辨率为500 m的城市边界层模式系统，来研究城市边界层在中尺度背景场作用下的精细结构。通过个例模拟，模式能够较准确地模拟城市边界层的风温场分布情况，可以用来对楔形绿地规划进行模拟试验。通过对规划后的气象场在特定的气象条件下进行模拟，结果显示，建造大型的楔形绿地后，绿地区域及绿地周围约1 km以内的地区温度有所降低，降低的程度由规划前后的地表类型改变的剧烈程度、风速大小及与绿地的距离决定，但是这种规划方案却会因城市的下风方向的风速减小而导致通风不畅。     

中尺度模式中的边界层特征量分析

在中尺度数值天气预报模式MM4中，用level3及E-ε-l两种湍流闭合方法对原总体边界层参数化方案进行改进，使得中尺度模式中可以直接输出有关湍流量，并对地表通量参数化方案进行改进，进而对不同下势需如沙漠，植被上的有关湍流量和边界层特征量进行分析。研究中尺度系统中边界层结构的特征，本文主要从地表通量，湍流交换系数，湍流动能（q^2)，温度脉动方差（θ^2)及风温廓线等几个方面进行研究，结果表明，新方案能更好地反映边界层特征。     

青藏高原地面-对流层系统的能量收支

利用CCM3中的辐射模式CRM，计算了1月和7月地－气系统、地面－对流层系统和地面辐射能收支，研究了青藏高原地面－对流层系统辐射能收支的冬、夏季节特征及其与地面和地－气系统辐射能收支的关系，并与东部平原地区和高原北侧干旱地区比较。文中还讨论了云和高原冬季地面积雪对辐射能收支的影响，比较了大气辐射加热和地面感热通量对夏季高原对流层大气加热的贡献。     

改进的切线性模式对一个边界层模式变分资料同化的改善

大气、海洋中边界层物理过程的强非线性会对切线性模式近似（尤其是当积分时间长时）有较大的影响，从而给相应的4维变分资料同化问题的求解造成困难。本构造了Mellor-Yamada湍流封闭模式（level 2.5)的一个改进的切线性模式，相比通常的切线性模式和简化的切线性模式可以提高对非线性扰动的逼近。利用这个改进的切线性模式的伴随模式分别进行了1到7天的变分资料同化试验，得到了满意的结果。而用通常的伴随模式和简化的伴随模式都无法得到令人满意的结果。     

反扩散格式在二维锋生数值模拟中的应用

把无粘流中能成功捕捉接触间断的反扩散差分格式，用在了准地转二维理想锋生的数值模拟中，并将计算结果与Cullen的计算结果和半地转方程的精确解进行了比较。用反扩散格式模拟的锋面较Cullen的结果更加显，而且更接近半地转方程的精确解。     

Observations Of Nocturnal Drainage Flow In A Shallow Gully

The formation of cold air drainage flows in a shallow gully is studied during CASES-99 (Cooperative Atmosphere-Surface Exchange Study). Fast and slow response wind and temperature measurements were obtained on an instrumented 10-m tower located in the gully and from a network of thermistors and two-dimensional sonic anemometers, situated across the gully. Gully flow formed on clear nights even with significant synoptic flow. Large variations in surface temperature developed within an hour after sunset and in situ cooling was the dominant factor in wind sheltered locations. The depth of the drainage flow and the height of the down-gully wind speed maximum were found to be largest when the external wind speed above the gully flow is less than 2 m s^-1. The shallow drainage current is restricted to a depth of a few metres, and is deepest when the stratification is stronger and the external flow is weaker. During the night the drainage flow breaks down, sometimes on several occasions, due to intermittent turbulence and downward fluxes of heat and momentum. The near surface temperature may increase by 6 ° C in less than 30 min due to the vertical convergence of downward heat flux. The mixing events are related to acceleration of the flow above the gully flow and decreased Richardson number. These warming events also lead to warming of the near surface soil and reduction of the upward soil heat flux. To examine the relative importance of different physical mechanisms that could contribute to the rapid warming, and to characterize the turbulence generated during the intermittent turbulent periods, the sensible heat budget is analyzed and the behaviour of different turbulent parameters is discussed.     

体感温度的研究及业务化应用

体感温度是人们对环境温度的综合反应，与人的生活需求密切相关。本文就其概念、研究意义和方法进行了阐述，并结合乌鲁木齐地区的气候特点，提出了符合本地区的体感温度的经验公式并实现业务化应用。     

紫外线模式预报方法的研究和试验

文章介绍了在T106全球谱模式中应用大气辐射传输模式预报紫外线辐射(UVR)的方法,给出了试验运行的结果.UVR强度的划分考虑了到达地表的UVR通量.参考国内、外紫外线(UV)预报服务的经验,制定了5个日光暴露的级别、相应的紫外线指数(UVI)及防护措施.1999年9月起,国家气象中心已在NOTES网上每月不定期地展示UVR预报的一些结果,2000年9月起,在Cray-C92业务操作系统上实施了连续的试验运行.     

Atmospheric Surface-Layer Processes During the Total Solar Eclipse Of 11 August 1999

The central path of the total solar eclipse (TSE) of 11 August 1999 mostly passedthrough a region of active monsoon in India, with the eclipse ending around localsunset. Measurements in the surface layer (SL) were carried out close to the eclipseaxis at Akola (20°42' N, 77°2' E) in central India. The globalradiation flux reaching the surface vanishes around totality at 1803:24 (LT), followedby a small recovery before again dipping to zero at sunset. The temperatures in the SL, and subsoil at 50-mm depth, show a local minimum with a lag of about 10 min after the second contact, whereas the lag appears to vanish when the temperature series is detrended. The SL exhibits near-neutral, though generally stable, conditions from about 1500 hr itself due to heavy cloud cover followed by the eclipse-induced cooling of the surface. The wind component across the eclipse axis vanishes at totality, the wind vector aligning with the azimuth of the traversing moon shadow. The deceleration of the mean flow can be due to the combined effect of the colder surface and downward heat flux, where the locally altered horizontal temperature gradients may cause, as in this instance, the cessation of the cross flow.The oscillations in temperature and wind that show significant peaks, around 90–100 min as well as the semi-period of the eclipse near 60 min, persist for several hours past the eclipse event. A fresh analysis of the published data on the TSE of 7 March 1970 shows spectral peaks in the temperature nearly coincident with those already reported from the surface pressure records. The oscillations in the SL fields during the two TSE events are very similar implying that the source mechanism is also likely to be the same in both the cases.