2005年6月华南暴雨期间西太平洋副高西伸过程分析   总被引：7，自引：1，他引：6  

司东  温敏  徐海明  何金海 《热带气象学报》2008,24(2):169-175

利用NCEP/NCARⅡ逐日再分析资料以及我国实测的降水资料,对2005年6月华南暴雨期间西太平洋副高的西伸过程进行了分析.结果表明:副高的东西进退可能与暴雨过程存在某种联系.分析指出副高中心的下沉气流主要是由副高南北两侧雨带中凝结潜热释放效应所致的上升气流在高空下沉而产生的,副高中心垂直运动的出现有利于副高的加强.而副高南北两侧雨带不但可以加强副高,同时又会激发正涡度增长,限制副高在南北方向上的活动,此时西侧印度季风雨带则会在副高西侧激发反气旋性涡度发展,即可诱使副高西伸.因此,华南强降水和印度季风区降水的共同作用使得副高加强西伸.  相似文献   

我国大雾的时空分布特征及其发生的环流形势   总被引：21，自引：6，他引：15  

林建  杨贵名  毛冬艳 《气候与环境研究》2008,13(2):171-181

根据1971～2005年35年来714站大雾资料,统计了我国大雾的时空分布特征和环流形势.结果表明:年平均大雾最多的地区主要集中在四川盆地、重庆、云南南部、湖南和江南东部;雾日有明显的季节和月际变化,春、夏季雾的范围较小,秋、冬季雾的范围较大,内陆雾主要为(秋)冬季正态分布型,东北的雾夏季偏多,沿海雾春、夏季较多.雾通常开始于晚上20时(北京时间,下同)至次日早晨8时(以6～7时为最多),结束于8～12时,持续时间大多在1～10 h,持续3h的雾出现的频数最高.近35年雾日的线性趋势表明:江南、华南的雾日变化不明显,其余大部分地区的雾日都呈递减趋势,不同能见度的雾日在1985年前后基本上都呈相反的变化趋势,并且能见度越低的雾日变化越明显.主要考虑地面天气形势我国大范围大雾发生的环流形势可分为均压型和锋前型两大类型.  相似文献   

应用多普勒天气雷达资料分析强对流天气的垂直廓线特征   总被引：1，自引：1，他引：0  

赵瑞金  史锐  董保华  李岩 《气象科学》2008,28(Z1)

利用石家庄多普勒天气雷达资料,对2004-2007年的22次冰雹和39次短时强降水天气过程中的各要素进行了对比分析.结果表明:在单体对流云和积层混合型对流云中,冰雹回波的强度、高度均强(高)于短时强降水,并且单体对流云型冰雹和短时强降水的回波强度和顶高均强(高)于积层混合型,积层混合型对流云出现短时强降水比例高于冰雹.在回波中层,短时强降水主要为偏东风和偏南风,冰雹主要为偏西风、偏北风;冰雹平均风速大于短时强降水,在3～6 km的高度风速显著增加.强对流天气出现前均呈现低层辐合,高层辐散;都有较强的上升运动,在天气过程出现后冰雹的下沉运动更强;当高层辐散量大于低层辐合量时,对流云发展加强,反之减弱.  相似文献   

"郑汴一体化"进程中生态廊道系统建设探讨     

董斌  苗蕾  李有 《气象与环境科学》2008,31(1):35-38

研究了废水中不同含盐量对生化处理效果以及生物学变化规律的影响.在废水含盐量低于22 g/L时,废水生化处理系统对COD的去除率可稳定在70%左右,污泥活性良好;随着进水盐浓度的增加,含盐量达到22 g/L时,污泥活性开始受到抑制,COD去除率急剧下降到50%左右;当废水含盐量达到31 g/L时,污泥活性明显受到抑制,污泥絮体开始部分解体,COD去除率下降到40%左右.  相似文献   

L波段测风雷达的选址、天线架设及标定     

崔炳俭  陈德生  王全周  李惠芳  董卫红 《气象与环境科学》2008,31(Z1)

介绍了L波段气象测风雷达场地选址时对遮挡角的要求、对天线底座的要求、天线与值班室距离,天线装置系统架设的技术要求,通电前的检查及雷达的标定.  相似文献   

孟津县远程教育终端防雷装置安全性能的调查与思考     

赵祖强  许怀庆  董硕硕 《气象与环境科学》2008,31(Z1)

调查发现,孟津县远程教育终端防雷装置存在安全隐患:96%的终端卫星接收天线与避雷针的距离不合格;所有终端电源防护只有一级,电源也无穿管埋地敷设,有的电源没有经过sPD保护;所有卫星天线基座与避雷针基座只有一处连接,高频头均未采取屏蔽措施;所有机柜均未与等电位接地端子连接;所有终端天馈线与防雷引下线距离均＜1000 m.设计缺陷,施工人员素质低下,管理不到位.是造成上述问题的直接原因.气象部门应以此为诫,加强防雷管理,加强防雷执法,避免类似事件发生.  相似文献   

On the peculiar momentum of baryons after reionization     

Carlos Hernández-Monteagudo  Shirley Ho 《Monthly notices of the Royal Astronomical Society》2009,398(2):790-806

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Galaxy activity in merging binary galaxy clusters     

Ho Seong Hwang †  Myung Gyoon Lee 《Monthly notices of the Royal Astronomical Society》2009,397(4):2111-2122

We present the results of a study of galaxy activity in two merging binary clusters (A168 and A1750) using the Sloan Digital Sky Survey (SDSS) data supplemented with the data in the literature. We have investigated the merger histories of A168 and A1750 by combining the results from a two-body dynamical model and X-ray data. In A168, two subclusters appear to have passed each other and to be coming together from the recent maximum separation. In A1750, two major subclusters appear to have started interaction and to be coming together for the first time. We find an enhanced concentration of the galaxies showing star formation (SF) or active galactic nuclei (AGN) activity in the region between two subclusters in A168, which were possibly triggered by the cluster merger. In A1750, we do not find any galaxies with SF/AGN activity in the region between two subclusters, indicating that two major subclusters are in the early stage of merging.  相似文献   

Non-Gaussian distribution and clustering of hot and cold pixels in the five-year WMAP sky     

Graziano Rossi  Ravi K. Sheth  Changbom Park  Carlos Hernández-Monteagudo 《Monthly notices of the Royal Astronomical Society》2009,399(1):304-316

We present measurements of the clustering of hot and cold patches in the microwave background sky as measured from the Wilkinson Microwave Anisotropy Probe 5-year data. These measurements are compared with theoretical predictions which assume that the cosmological signal obeys Gaussian statistics. We find significant differences from the simplest Gaussian-based prediction. However, the measurements are sensitive to the fact that the noise is spatially inhomogeneous (e.g. because different parts of the sky were observed for different lengths of time). We show how to account for this spatial inhomogeneity when making predictions. Differences from the Gaussian-based expectation remain even after this more careful accounting of the noise. In particular, we note that hot and cold pixels cluster differently within the same temperature thresholds at few-degree scales. While these findings may indicate primordial non-Gaussianity, we discuss other plausible explanations for these discrepancies. In addition, we find some deviations from Gaussianity at sub-degree scales, especially in the W band, whose origin may be associated with extragalactic dust emission.  相似文献   

A Study on the Long-term Spectral Variability of the Black-hole Candidate X-ray Binary Cyg X-1     

Ai-Jun Dong  Jian-Cheng Wang  Li Xue 《Chinese Astronomy and Astrophysics》2009,33(3):265-278

Using the All-Sky Monitor (ASM, 1.5–12–kev) data of Rossi X-ray Timing Explorer (RXTE) from January 1996 to May 2005, we have made a detailed analysis of the correlation between photon-count rate and spectral hardness ratio HR2 (5–12 keV/3–5 keV) of the black-hole candidate X-ray binary Cyg X-1 in 3 energy bands, namely the A-band (1.5–3 keV), B-band (3–5 keV) and Cband (5–12 keV). By the study on the ASM data of 1-day time scale, we find: (1) When Cyg X-1 is in the soft state, the A-band photon-count rate and hardness ratio HR2 exhibit an anticorrelation, but in B-band and C-band there appears the positive correlation. When Cyg X-1 is in hard state, the photon-count rates in the A,B,C bands are all inversely correlated with the hardness ratio HR2; (2) No matter whether Cyg X-1 is in the soft state or the hard state, the hardness ratios HR2 and HR1 are always positively correlated. In addition, we have analyzed the “dwell by dwell” data of the ASM, and obtained the following interesting results: (1) In the period of MJD = 52600–52760 (while Cyg X-1 is in the hard state), the photon-count rates in the A-band and B-band are inversely correlated with HR2, but in the C-band there appears a relatively strong positive correlation; (2) During the hard state, a clear anticorrelation exists between the hardness ratios HR2 and HR1.  相似文献