6种数值模式在安徽区域天气预报中的检验

本文检验了从2006年6月到2008年12月,Grapes、MM5、WRF、T213、JMA和Germany共6个模式对安徽区域72 h内降水量、风速和气温的预报。降水量TS评分显示,从小雨到大雨,JMA的参考价值较高,从大雨到大暴雨则是MM5和WRF比较好;Germany和T213的评分均处于中间水平,而Grapes评分最低。冬夏季各模式的预报较好,其他季节预报较差。风速,24 h JMA和T213的预报较好,48、72 h MM5和WRF的参考价值较高。气温,24、48 h MM5和WRF预报较好,而72 h则是MM5和T213好。Grapes对风速和气温的预报相对较差。上述检验结果不仅有助于预报员更好地利用数值模式制作天气预报,而且为数值天气预报的解释应用提供科学依据。     

雨雪冰冻天气多普勒雷达产品特征

2008年1月下旬至2月上旬福建省西部北部出现了历史罕见的雨雪冰冻灾害。利用多普勒雷达反射率、回波顶高、径向速度、垂直风廓线等产品对此次雨雪冰冻天气进行特征分析,通过分析发现:①冰晶和雪的回波强度通常比连续性降水回波弱,在反射率图上,回波表现为边缘毛松,丝缕状纹理结构明显,边缘模糊不清,没有确定的边界;②回波顶高和零度层较低,因为垂直方向大气相对较稳定,不利于对流发展,降水粒子没有发展到高空;③在径向速度图上存在牛眼,说明在低空有急流存在。在低层有环形的零速度线,中高层的零速度线为倒"S"形,表明低层有风切变存在,中高层有冷平流;④风廓线图上高层为西南风,中层为西北风,低层为西南风,近地层为东北风。说明从近地层到高层为"冷-暖-冷-暖"的层结结构,有利于冻雨天气形成。     

重庆10 kV高压输电线路雷击火灾事故分析

针对2007年7月12日重庆华浩冶炼有限公司粉末厂火灾事故,用力学性能分析和剩余磁场测试相结合的方法对该厂火灾发生处的10 kV高压输电线路进行鉴定,并结合雷电天气分析,得出该火灾事故是由雷击10 kV高压输电线路造成。该方法为在没有安装录波器和闪电计数器的情况下,判断输电线路故障是否由于雷击引起提供参考。     

利用手机气象短信平台打造公共服务信息发布中心

手机气象短信因快捷、准确、定时、一对一服务,深受用户欢迎,但也面临着与报业、广电集团等运营商的竞争.气象部门应发挥自己的网络、品牌、用户众多等优势,拓宽服务范围,加强与公共事业部门合作,发布环保、供电、供水等关系群众生活的实时信息,把气象短信平台打造成公共服务信息发布中心.     

基于ADTD系统的雷电流波头陡度频率分布特征

通过对ADTD闪电定位系统2006 2008年在重庆地区监测的729598次闪电进行统计,重点分析雷电流陡度的频率分布特征。结果表明:雷电流波头陡度及其频率随极性不同而差异较大,正闪陡度明显大于负闪陡度,而同陡度负闪频率却显著大于正闪;雷电流幅值与陡度相关系数为+0.613;采用电力行业标准DL/T620推荐波头时间反推得到的雷电流陡度和采用Ciger推荐公式计算得到的雷电流陡度的概率分布特征与统计特征差异较大。在此基础上分析了ADTD系统获取雷电流陡度资料的局限性,为合理选取雷电流陡度参数提供理论依据。     

Evaluating CEOP model performance with the observational data from Tongyu reference site, semi-arid region of China

Using data archived in the Coordinated Enhanced Observing Period (CEOP) project, comparisons between field observations undertaken at Tongyu CEOP reference site in China and model output from year 2003 to 2004 have been implemented, and in particular, the time series and diurnal cycles of precipitation, near-surface temperature, air temperature, and latent and sensible heat fluxes are presented. The results show that the ability of the model simulations on the temperatures, such as air temperature and the surface temperature, is satisfactory compared with the simulations on the land surface heat fluxes and the precipitation at Tongyu site. In addition, the multi-model ensemble exhibits better results over all items in comparison with the observations. The differences of the precipitation at the interannual and the seasonal time scales between the model results and observations indicate that some of the models are able to reproduce the larger amount of precipitation in 2003 than that in 2004, which is consistent with the trend of the observations at Tongyu site even though the mean square errors of models output calculated from daily precipitation during year 2003 and 2004 are even greater than the daily amount of the precipitation. The poor skill in the quantitative simulation of the precipitation indicates that the deficiency of the models in simulating the surface heat fluxes may be closely related to the biases of the precipitation simulations. In terms of the seasonal time series of the precipitation, there is an increase during summer, accompanied by the same increased trend of the latent heat flux and the decreased trend of the sensible heat flux from the insitu observations.     

贵州安顺新场河水库滑坡成因与变形趋势分析

本文以新场河水库滑坡为研究对象,在野外勘查、探明滑坡地质条件和变形特征的基础上,对新场河水库滑坡的成因进行了分析,根据土体压缩特性和固结原理,参照地基变形计算方法,对滑坡稳定性及未来的变形发展趋势进行了评价。研究表明,具备顺层地质条件的库岸斜坡,在库水位升降和降雨联合作用下,即使没有很好的临空滑移条件,斜坡体也会产生蠕滑变形,其变形量的大小与坡体组成物质的压缩性有关。分析研究可为同类水库滑坡防治及安全运行提供借鉴。     

Prompt optical emission and synchrotron self-absorption constraints on emission site of GRBs

We constrain the distance of the gamma-ray burst (GRB) prompt emission site from the explosion centre R , by determining the location of the electron's self-absorption frequency in the GRB prompt optical-to-X/γ-ray spectral energy distribution, assuming that the optical and the γ-ray emissions are among the same synchrotron radiation continuum of a group of hot electrons. All possible spectral regimes are considered in our analysis. The method has only two assumed parameters, namely the bulk Lorentz factor of the emitting source Γ and the magnetic field strength B in the emission region (with a weak dependence). We identify a small sample of four bursts that satisfy the following three criteria: (1) they all have simultaneous optical and γ-ray detections in multiple observational time intervals, (2) they all show temporal correlations between the optical and γ-ray light curves and (3) the optical emission is consistent with belonging to the same spectral component as the γ-ray emission. For all the time intervals of these four bursts, it is inferred that   R ≥ 10¹⁴  (Γ/300)^3/4 ( B /10⁵ G)^1/4  cm. For a small fraction of the sample, the constraint can be pinned down to   R ≈ 10¹⁴–10¹⁵ cm  for  Γ∼ 300  . For a second sample of bursts with prompt optical non-detections, only upper limits on R can be obtained. We find no inconsistency between the R -constraints for this non-detection sample and those for the detection sample.     

Variability of Extended Bipolar Regions

Using NSO/Kitt Peak synoptic charts from 1975 to 2003, we group the main solar magnetic fields into two categories: one for active regions (ARs) and the other for extended bipolar regions (EBRs). Comparing them, we find that there exist three typical characteristics in the variability of EBRs: First, there exists a correlation between ARs and EBRs. The phase of EBR flux has a delay nearly two CRs. Second, we find that the EBR flux has two prominent periods at 1.79 years and 3.21 years. The 1.79-year period seems to only belong to large-scale magnetic features. Lastly, the North – South asymmetry of EBR flux is not very significant on a time scale of one solar cycle. However, during solar maxima, its dominance is found to shift from one hemisphere to the other.