一次α中尺度低涡暴雨的数值模拟

用WRF模式对2007年4月21—22日的一次中α低涡暴雨过程进行了高分辨率模拟,结果表明:(1)该低涡的产生与湖北西部的地形条件有一定的联系,低压倒槽系统为其提供了必要的环流背景,反演自FY-2 C卫星的TBB资料较好地反映了该中α低涡的整个活动过程。(2)对低涡发展最强阶段的动力和热力结构分析表明,低涡右侧为较强的上升运动,而其左侧则为下沉运动,在中低层冷空气上部有南侧暖湿空气上爬造成的次级上升运动;低涡左侧存在较明显的湿斜压锋区,后部则有明显的干冷气切入;南风风量对总体水汽输送的贡献要大于西风风量。(3)WRF模式中NOAH和热扩散陆面方案的对比分析表明,NOAH方案更加有利于低涡中心的发展,因此能够产生较热扩散方案更强的中心区降水,但是这种增强作用主要分布在低涡区附近,其他地区差别不大。     

气象探空数据动态比对中误差计算方法研究

在高空动态数据比对中,需要同时考虑系统误差与随机误差。采用多个探空仪同球比对施放的方法,从相对系统误差、标准偏差等方面,对被试探空仪进行比对评估,同时采取误差分离方法,计算被试探空仪的随机误差。考虑高空温度在对流层与平流层的不同变化趋势,采取细化分层方式进行计算,以反映大气特性。     

Comparative Studies of Different Mesoscale Convection Parameterization Schemes in the Simulation of Mei-Yu Front Heavy Rain

The mei-yu front heavy rainstorms occurred over Nanjing on 3 5 and 8 9 July 2003 and were simulated in this paper using the Weather Research and Forecasting Model (WRFv3.1) with various mesoscale convection parameterization schemes (MCPSs). The simulations show that the temporal and spatial evolution and distribution of rainstorms can be modeled; however, there was incongruity between the comparative simulations of four different MCPSs and the observed data. These disparities were exhibited in the simulations of both the 24-hour surface rainfall total and the hourly precipitation rate. Further analysis revealed that the discrepancies of vertical velocity and the convective vorticity vector (CVV) between the four simulations were attributed to the deviation of rainfall values. In addition, the simulations show that the mid-scale convection, particularly the mesoscale convection system (MCS) formation, can be well simulated with the proper mesoscale convection parameterization schemes and may be a crucial factor of the mei-yu front heavy rainstorm. These results suggest that, in an effort to enhance simulation and prediction of heavy rainfall and rainstorms, subsequent studies should focus on the development and improvement of MCPS.     

未来极端降水对气候平均变暖敏感性的蒙特卡罗模拟试验

利用Weibull分布拟合逐日降水的原始分布模式,并基于统计降尺度和蒙特卡罗随机模拟方法,对中国东部区域各站逐日极端降水量在未来气候变暖条件下的响应特征进行统计数值试验.结果表明,在全球变暖背景下,区域平均温度的改变即可导致区域极端降水概率分布特征的变动.从两个典型代表区域的预估结果中可见,长江中下游南部平均降水量对平均温度升高有正响应,模拟得到的区域极端降水概率分布曲线有明显的向右平移,导致大量级的极端降水的再现期缩短即概率增大.山东及渤海湾区域平均降水量对平均温度升高有负响应,模拟得到的区域极端降水概率密度分布尺度参数变小更明显,即方差增大,表现为左右两侧概率密度增加,同样导致大量级的极端降水再现期缩短即概率增大.本文仅考察了气候均值改变条件下,未来区域气候极端值的概率预估的可行性方案.对于未来气候方差的变化并未作试验,但理论上已经证明,未来气候极端值的概率对于气候方差变化的敏感性可能更大.由于目前尚未整卵出考察方差变化的较为完整的实际观测资料,该问题还有待进一步深入研究.     

降水气候强迫下非均匀地表区域平均径流的一种参数化方案

将任一中尺度区域的平均瞬间径流率考虑为区域平均降水量和地表土壤层水分渗透垦的余项.根据降水量在地理空间上分布的实测资料拟合其空间概率密度函数(PDF),并结合土壤入渗物理过程的数学描述及其经验公式,精确估计出地表土壤渗透率及其空间分布,由此建立区域地表径流率的统计-动力学估计方案.换言之,区域内地表产流率可视为区域平均降水量与区域平均的土壤下渗量之差值,而区域内土壤的平均下渗量又町分为非饱和区和饱和区两部分的下渗量来分别计算.就陆面水分循环的物理过程而言,地表入渗现象是在一定的下垫面特性基础上,由一定的水分供应源而形成的.根据大气降水向地表层输送水分的物理过程,在满足植被表层覆盖需水(截流水)和地表层土壤人渗水基础上,多余的降水量才会形成地表径流.凶此,推求地表产流率的主要关键在于地表土壤层需水量.为此奉文根据土壤水分通量方程推导出水分入渗公式.又从描述土壤水分和降水的空间PDF出发,推导出非均匀土壤含水量及降水气候强迫所形成的次网格尺度区域平均径流率计算公式.利用长江三角洲地区1996年降水量和土壤特性等实测资料建立区域平均地表径流率的估计公式,并对其影响凶素进行敏感性试验.结果表明,该方法与用Mosaic方法计算的区域径流率(或产流率)结果十分接近.由此可见,该文提出的降水气候强迫下非均匀地表区域平均径流的这种统计-动力参数化方案,具有相当的可靠性与可行性.     

综合办公大楼的雷击风险评估方法

根据标准和现行法律法规的规定,雷电风险评估应在新建建筑物的设计之前进行,或在防雷整改工程实施之前完成,其目的是使雷电防护设计建立在科学的基础上,避免盲目性,保证防雷工程安全可靠、技术先进、经济合理.该文通过对某综合办公大楼进行施工前的雷电风险评估,来具体说明评估的方法.     

ANALYSIS OF THE CHARACTERISTICS OF SUSTAINED TORRENTIAL RAINS IN JUNES DURING 1958-2000

Day-to-day precipitation data of Junes during the 43 years of 1958-2000 from stations to the south of Yangtze River are used to divide regions and run statistical analysis of sustained torrential rainfall processes. A preliminary analysis is then made based on it and the results show that June is the month in which torrential rains in the southern half of China take place frequently and sustained torrential rains occur at the same time in South China and the area to the south of Yangtze River. In addition, the analysis gives the basic features of sustained torrential rains of June in China and their interannual variability patterns, with the suggestion that the amount of these events increases significantly after the 1990s. Lastly, the sustained torrential rains occurring in Junes of 1994, 1998 and 2005 in the southern half of China are taken as examples in the research on the basic patterns and formation mechanisms of the evolution of double rain-bands during the rain season in South China and the area to the south of Yangtze River. The analysis shows that the large scale environment field in which sustained torrential rains occur is related to the stable sustaining of the South Asia High and upper level jet streams.     

连云港沿海地区及近海风能资源评估

通过对连云港市30多年气象整编资料及沿海高密度自动气象站、6座测风塔、4座海岛气象站等加密观测资料研究,在充分考虑当地特殊地形特点的基础上,探讨了该地区沿海及近海风能资源的时空分布规律及特点,并重点对风湍流强度的特征及强湍流对风电的影响进行了剖析;研究表明,近海地区风能资源储量相对丰富,风速变化稳定,且风垂直切变较小,具有更为广阔的开发利用前景.     

The influence of magnetic fields on neutrino-dominated accretion disc

We consider the influence of magnetic fields on the model of neutrino-dominated accretion flows (NDAFs) for gamma-ray bursts (GRBs) via the assumption that the accretion rate of the disc is totally caused by the torque of the Lorentz force, i.e. the magnetic braking of large-scale magnetic fields and magnetic viscosity of small-scale magnetic fields. We calculate the structure, composition, luminosity of neutrino emission and the Poynting flux, and the rate of mass loss driven by neutrino heating or launched centrifugally by large-scale magnetic fields, based on the physical condition of the magnetized NDAFs. It is shown that the magnetized disc is favourable to interpret the diverse prompt emissions as well as the X-ray flares observed in the early afterglow of GRBs.     

Old stellar population synthesis： new age and mass estimates for Mayall Ⅱ = G1

Mayall Ⅱ = G1 is one of the most luminous globular clusters （GCs） in M31. Here, we determine its age and mass by comparing multicolor photometry with theoretical stellar population synthesis models. Based on far- and near-ultraviolet GALEX photometry, broad-band UBVRI, and infrared JHKs 2MASS data, we construct the most extensive spectral energy distribution of G 1 to date, spanning the wavelength range from 1538 to 20 000A. A quantitative comparison with a variety of simple stellar population （SSP） models yields a mean age which is consistent with G1 being among the oldest building blocks of M31 and having formed within ～1.7 Gyr after the Big Bang. Irrespective of the SSP model or stellar initial mass function adopted, the resulting mass estimates （of order 10^7M⊙） indicate that GI is one of the most massive GCs in the Local Group. However, we speculate that the cluster＇s exceptionally high mass suggests that it may not be a genuine GC. Our results also suggest that G1 may contain, on average, （1.65±0.63） × 10^2L⊙ far-ultraviolet-bright, hot, extreme horizontal-branch stars, depending on the adopted SSP model. In addition, we demonstrate that extensive multi-passband photometry coupled with SSP analysis enables one to obtain age estimates for old SSPs that have similar accuracies as those from integrated spectroscopy or resolved stellar photometry, provided that some of the free parameters can be constrained independently.