1971—2020年辽宁龙卷的气候特征及环境条件分析

为了解辽宁龙卷气候特征,基于《中国气象灾害大典》《中国气象灾害年鉴》和其他相关资料,根据“改进藤田分级”龙卷级别分类标准,对1971—2020年辽宁龙卷进行强度分类和时空分布特征统计,并对比我国辽宁与美国龙卷高发区环境背景差异,分析辽宁龙卷典型的环流形势、物理量特征。得到以下主要结论:1971—2020年辽宁地区共记录到97个龙卷日发生龙卷105次,年均为2.1次,年平均龙卷生成密度为1.4×10^-5个·km^-2,约为美国的1/10。EF2及以上级别强龙卷共记录到17次,年均出现0.3次。95%的龙卷出现在5—9月,67%出现在14—19时。EF2及以上级别强龙卷主要分布在辽宁中部以西地区,东南沿海地区多为弱龙卷,辽宁西北部龙卷季明显早于东南部。对流有效位能和中低层风切变随季节呈反相位变化,两者的合适配置是龙卷等强对流天气产生的前提条件。低层风暴相对螺旋度偏小是我国辽宁较美国龙卷高发区龙卷密度明显偏小的主要原因。辽宁87%的龙卷与冷涡相关,分为低层锋生主导的冷涡底部短波槽和冷涡前部型(65%)、中高空干冷气流主导的冷涡后部型(12%)以及强热...     

0421号热带风暴"海马"登陆后的温带变性过程特征探讨

0421号热带风暴“海马”于2004年9月13日12:00在浙江温州市沿海登陆后,迅速减弱为热低压,然后继续北移;并在中高纬高空槽后的冷平流和中低纬低层暖式切变南部的暖平流共同作用下,低压加深及冷、暖锋生,发展为斜压温带锋面气旋.采用相对辐散作为气旋发展的判据,能很好地体现整个变化过程,气旋的移向基本上沿着相对辐散中心长轴方向移动.通过对地面温度场水平结构分析后发现,该气旋经历了3个阶段:暖涡旋基本对称结构、半冷半热非对称结构、冷涡旋基本对称结构.对流层低层气旋中心上空为暖平流区,引导气旋移动,而对流层中层的冷平流中心区一直位于气旋移向的下侧,推动气旋移动.     

A Probable Short Decimetric Type Ⅰ-like Noise Storm: Associated with Type Ⅲ Bursts?

A rare Type I-like noise storm was observed with the solar radio spectrometers (1.0-2.0 GHz and 2.60-3.8 GHz) at National Astronomical Observatories of China (NAOC) on September 23, 1998. We concentrate on checking the Type I-like noise storm occurred in the decay phase of a Type Ⅳ radio burst. This noise storm consists of many Type I bursts and isolated Type Ⅲ or Type Ⅲ pair bursts. It has a bandwidth of ≤0.5 GHz. The duration of each Type I burst is of the order of 100-300 ms. The total duration is greater than 11 minutes. The circular polarization     

沙尘和生物气溶胶的环境和气候效应

沙尘气溶胶对海洋生态系统的影响及其气候与环境效应,以及生物气溶胶对人类健康的影响及其气候效应是近年来大气气溶胶研究的热点问题。沙尘气溶胶和生物气溶胶之间有很强的联系,沙尘可作为空气中微生物的载体,沙尘气溶胶影响海洋生态系统之后又会影响海洋上空生物气溶胶的产生。本文回顾了国内外沙尘气溶胶对太平洋海域生态系统影响的研究进展,以及生物气溶胶的研究历史和气候效应,特别是中国科学院大气物理研究所十多年来的有关工作。     

Variations of levels and composition of PM10 and PM2.5 at an insular site in the Western Mediterranean

The insular suburban site of Castillo de Bellver was selected for the study of the variability of PM levels and composition in the Western Mediterranean Basin (WMB).Mean annual (in 2004) PM₁₀ and PM_2.5 levels at this site were 29 and 20 µg/m³, respectively. These levels may be regarded as relatively low when compared with other suburban insular locations in the Eastern Mediterranean Basin (EMB), but they are higher than those recorded at most of the European suburban sites, especially in Northern and Western Europe. Seasonal variability of PM levels at this site is governed by meteorology rather than local emissions, whereas the daily cycles are clearly defined by the anthropogenic emissions, mainly coming from the urban area of Palma de Mallorca and the harbour area of the same city.Concerning the aerosol composition at this site, the main PM constituent is the mineral matter (29% in PM₁₀ and 16 % in PM_2.5), more than 50% (in PM₁₀) being attributable to African dust. The amount of secondary inorganic aerosols is also very high (27% in PM₁₀ and 34% in PM_2.5), with the predominance of fine ammonium sulphate, and in a less proportion fine ammonium nitrate (in winter) and coarse Ca and Na nitrate (with higher importance in summer). The carbonaceous particles, dominantly fine, account for 17% of PM₁₀ and 25% of PM_2.5. The elemental carbon/organic carbon (EC/OC) ratio reached a mean value of 0.17, similar to those observed at regional background sites in the WMB coast of Spain. The sea spray aerosols (mainly coarse) represented around 10% of PM₁₀, and only 4% in PM_2.5. Finally, the unaccounted fraction increased from 15% to 20% in PM_2.5, being mostly attributed to water.The concentrations of trace elements in PM₁₀ and PM_2.5 were usually in the range to those observed in regional background sites in the Iberian Peninsula, with the exception of the typical tracers of road traffic such as Cu, Sb, Zn, Sn and Ba, which presented concentrations in the range of urban sites of Iberia. Other elements such as Cr, Zr, Hf and Co have been identified as the main tracers of the harbour contributions.     

2002 Kuiper prize lecture: Dust Astronomy

Dust particles, like photons, carry information from remote sites in space and time. From knowledge of the dust particles' birthplace and their bulk properties, we can learn about the remote environment out of which the particles were formed. This approach is called “Dust Astronomy” which is carried out by means of a dust telescope on a Dust Observatory in space. Targets for a dust telescope are the local interstellar medium and nearby star forming regions, as well as comets and asteroids. Dust from interstellar and interplanetary sources is distinguished by accurately sensing their trajectories. Trajectory sensors may use the electric charge signals that are induced when charged grains fly through the detector. Modern in-situ dust impact detectors are capable of providing mass, speed, physical and chemical information of dust grains in space. A Dust Observatory mission is feasible with state-of-the-art technology. It will (1) provide the distinction between interstellar dust and interplanetary dust of cometary and asteroidal origin, (2) determine the elemental composition of impacting dust particles, and (3) monitor the fluxes of various dust components as a function of direction and particle masses.     

多普勒天气雷达资料在沙尘天气监测中的应用

利用3830型多普勒天气雷达回波资料及常规气象资料对2002年3月20日发生在我国西部一直延伸至黑龙江省的沙尘、浮尘天气过程，分析其多普勒天气雷达回波，并用PPI和RHI上探测沙尘的特征、高度、厚度、浓度、移动特点、速度场分布以及垂直风速分布特点等。为多普勒天气雷达监测沙尘提供可靠依据。     

广州城市暴雨内涝时空演变及建设用地扩张的影响

暴雨内涝是城市常见的“城市病”。本研究通过收集20世纪80年代、90年代,以及2000年之后广州市主城区严重暴雨内涝资料,探索改革开放后广州市暴雨内涝时空演变特征,分析城市建设用地扩张对暴雨内涝的影响。结果表明,20世纪80年代至今,广州市主城区暴雨内涝点在时间和空间2个尺度上有显著的变化。早期内涝点主要集中于市中心的越秀区,随着城市化进程的推进逐渐在白云、天河等城市化较快的区域出现。从1990-2010年,广州市城乡建设用地扩张显著,城市不透水面密度与暴雨内涝点核密度呈正相关。其相关性随城市化发展逐渐增强,表明改革开放后广州市城市的快速扩张,对主城区暴雨内涝点的时空演变有较大的影响。因此,城市暴雨内涝的防治应重视城市不透水面格局的优化和调整。     

理想海域中台风引起的潮、流及波的分析 II.海岸及陆架的影响

采用理想的大陆架地形和台风模型计算了不同方向登陆的台风所激发的海洋响应。结果表明,岸边的潮位变化主要是由于台风引起的强迫振动造成的。而对于登陆型台风来说,在远离台风路径的地方,潮位的变化则是由于边缘波效应。对地平直海岸和二维大陆架,自由边缘波的振幅远小于强迫波的振幅。平行海岸移行台风在岸边产生随台风一起移动的强制波,其中当台风沿着与Ｋｅｌｖｉｎ波相同的方向移行时,岸边有陆架波产生,反之则没有陆架波。此外,还讨论了与风暴潮相关的近岸环流。     

降水气候噪声和可预报性问题的初步研究

本文对2002年12月19日至24日华北地区的一次大暴雪伴特强降温天气过程从天气过程特点，大尺度环流形势特征，大暴雪及特强降温的成因进行了分析研究，得出了几个对该类天气的预报有指示意义的着眼点。