2001年春季中国北方沙尘暴的环流动力结构分析   总被引：14，自引：15，他引：14  

王可丽  江灏  吴虹 《高原气象》2002,21(3):303-308

通过对2001年春季中国北方5次沙尘暴的高度场，涡度场，散度场和风场的分析，研究了沙尘暴强盛期的环流动力结构。结果表明，在5次沙尘暴强盛期有相似的环流动力结构特征。在沙尘暴强盛期的高度场上，蒙古国有深厚的低值系统，乌拉尔高压发展，其间的强气压梯度是沙尘暴的动力源；低值系统有正涡度中心支持，外围是负涡度区，其间有强涡度梯度带；低值中心伴随有低层辐合高层辐散的垂直结构，易于发生近地面大风和上升气流，有利于地面起沙上扬，形成沙尘暴，大风区与强涡度梯度带一致，强风带切变形成的涡度输送有利于加强低值系统，进而增强风场。  相似文献   

平凉地区对流风暴地闪活动与环境层结因子相关性分析   总被引：6，自引：1，他引：6  

张翠华  张义军  郄秀书  王怀斌 《高原气象》2002,21(6):632-636

利用1997年和1998年6－8月间在甘肃平凉地区的3站闪电定位系统所取得的地闪资料与当天早晨探空资料进行了初步的统计分析。分析结果，对流风暴中地闪活动与环境层结因子之间有较好的相关性，不稳定度、余额不稳定度5℃处的环境温度、温度层结中（中层）平均相对湿度是影响对流风暴中地闪活动的重要因子，对流风暴的地闪活动可通过这些因子进行预报。  相似文献   

北太平洋阻塞的年际年代际变化及其与SST、遥相关及风暴路径的关系   总被引：2，自引：0，他引：2  

Huang Fei  Zhou Faxiu  Qian Xiaodan 《大气科学进展》2002,19(5):807-820

利用NCEP／NCAR再分析资料，对1948／1949－1999／2000共52个冬季的北太平洋上空中纬度阻塞异常的气修特征进行了统计分析，小波分析和功率谱分析结果表明该区域阻塞发生的频数具有很明显的3－7年的年际振荡和年代际变化特征。同时2－7年带通平均的小波方差谱分析结果表明阻塞的这种年际变化的振幅存在着缓慢下降的趋势，且气候突变在20世纪70年代，这进一步证明了北太平洋上空的阻塞活动具有年代际变化特征。对强阻塞异常的冬季和弱阻塞异常的冬季分别进行合成分析，结果表明，对于阻塞异常强的冬季，北太平洋西向东北方向加强并分裂成两个中心，而SST异常在中纬度太平洋则对应着典型的PDO型，在赤道地区则为类La Nina型的海温分布。而对于阻塞异常弱的冬季则对应截然不同甚至相反的分布特征，即500hPa高度异常场表现为符号相反的PNA型，风暴路径中心在日界线附近呈纬向型分布。同时SST异常在赤道地区则为典型的El Nino型的海温分布。以上结果揭示出北太平洋阻塞活动的年际变化可能主要与热带海温的遥响应相联系，而年代际变化则主要与中纬度局地的PDO型海温及其通过斜压瞬变波的海－气相互作用有关。  相似文献   

中国沙尘暴天气的新特征及成因分析   总被引：65，自引：6，他引：65       下载免费PDF全文

张仁健  韩志伟  王明星  张小曳 《第四纪研究》2002,22(4):374-380

2000～2002年,中国北方地区频频发生沙尘暴天气,给当地和广大下游地区工农业生产、交通运输、空气质量和人民的日常生活都带来了极大危害。沙尘暴天气呈现频次高、发生时间提前、发生期时间长、强度大、影响范围广等新特征。对气候变化和地理环境背景的分析研究表明,近年来中国北方沙尘暴频繁爆发的原因主要是:1)近两年处于反厄尔尼诺(拉尼娜)事件的高峰期,使东亚冬季风频繁,导致大风天气频繁发生;2)在沙尘暴发生季节,中国北方降水明显减少,气温回升迅速且温度偏高于往年,使解冻的地表土层疏松,为沙尘暴的发生提供了丰富的沙源;3)近年来中国北方干旱加剧、土地荒漠化严重,使原本广阔的戈壁沙漠面积更加扩大,有利于沙尘暴天气的发生,这与不合理的土地利用状况有关。  相似文献   

Simultaneous radio and optical observations of the mid-latitude atmospheric response to a major geomagnetic storm of 6–8 April 2000     

E. L. Afraimovich  Ya. F. Ashkaliev  V. M. Aushev  A. B. Beletsky  V. V. Vodyannikov  L. A. Leonovich  O. S. Lesyuta  Yu. V. Lipko  A. V. Mikhalev  A. F. Yakovets 《Journal of Atmospheric and Solar》2002,64(18)

Basic properties of the mid-latitude traveling ionospheric disturbances (TIDs) during the maximum phase of a major magnetic storm of 6–8 April 2000 are shown. Total electron content (TEC) variations were studied by using data from GPS receivers located in Russia and Central Asia. The nightglow response to this storm at mesopause and termospheric altitudes was also measured by optical instruments FENIX located at the observatory of the Institute of Solar-Terrestrial Physics (51.9°N,103.0°E), and MORTI located at the observatory of the Institute of Ionosphere (43.2°N, 77.0°E). Observations of the O (557.7 and 630.0 nm) emissions originating from atmospheric layers centered at altitudes of 90 and 250 km were carried out at Irkutsk and of the O₂(b¹∑_g⁺−X³∑_g⁻) (0-1) emission originating from an atmospheric layer centered at altitude of 94 km was carried out at Almaty. Our radio and optical measurement network observed a storm-induced solitary large-scale wave with duration of 1 h and a wave front width of no less than 5000 km, while it traveled equatorward with a velocity of 200 m/s from 62°N to 38°N geographic latitude. The TEC disturbance, basically displaying an electron content depression in the maximum of the F2 region, reveals a good correlation with growing nightglow emission, the temporal shift between the TEC and emission variation maxima being different for different altitudes. A comparison of the auroral oval parameters with dynamic spectra of TEC variations and optical 630 nm emissions in the frequency range 0.4–4 mHz (250–2500 s periods) showed that as the auroral oval expands into mid-latitudes, also does the region with a developed medium-sale and small-scale TEC structure.  相似文献   

南向行星际磁场事件与磁暴关系的研究   总被引：5，自引：5，他引：5       下载免费PDF全文

刘绍亮  李立文 《地球物理学报》2002,45(3):297-305

利用172-182年IMP-8飞船的太阳风观测资料和相应地磁活动性指数Dst和AE,研究了43个南向行星际磁场事件期间太阳风和磁层的耦合问题. 与这43个事件对应的地磁暴是中等的和强的磁暴(Dst＜-50nT). 结果表明:(1) 在43个事件中有11个(约占25.6髎)紧随激波之后,18个处于激波下游流场中(占42髎),其余14个(占33髎)和激波没有关连. 绝大多数事件都伴有太阳风动压和总磁场强度的增加;(2) 当行星际晨昏向电场强度EI＞-4mV/m时,只引起磁亚暴,对Dst指数没有明显影响. 仅当EI＜-5mV/m时,磁亚暴和磁暴才会同时出现;(3) 太阳风动压的增加会增强能量向环电流的输入,但不是密度和速度单独起作用,而是以PK=ρV2的组合形式影响能量的输入;(4) 虽然行星际磁场(IMF)南向分量BZ对太阳风和磁层的耦合起着关键作用,但IMF的BX和BY分量相对于BZ的大小对太阳风向磁层的能量传输也有一定影响. 当BX、BY相对BZ较大时能量耦合加强.  相似文献   

渭干河流域"2002·7"特大洪水分析   总被引：6，自引：0，他引：6  

黄健  毛炜峄  李燕  王顺德 《冰川冻土》2003,25(2):204-210

渭干河是塔里木河流域第六大源流, 位于天山西部南麓, 渭干河干流起点有新疆最大的流域性控制工程--克孜尔水库. 2002年7月下旬天山中西部山区出现大暴雨(雪)过程, 渭干河流域山区降水持续时间长达30 h以上, 山区降水量50 mm左右, 导致5条支流和渭干河干流出现有水文记录以来的最大洪峰, 流量超过警戒流量和危险流量的2～3.5倍, 暴雨(雪)过程结束之后, 融雪型洪峰长时间居高不下. 洪水过程中, 各支流以及暴雨与融雪等多种洪峰遭遇现象很明显. 克孜尔水库入库洪峰流量达3 660 m3*s-1, 经水库调洪错峰, 出库峰值流量为1 000 m3*s-1, 削峰率72.7%.  相似文献   

浙江桐庐晚奥陶世晚期沉积层序和沉积环境分析   总被引：3，自引：0，他引：3  

范代读  李从先  蔡进功  邓兵  罗璋 《沉积学报》2003,21(2):247-254

文昌组上段顶部是一套潮汐层理非常发育的泥质砂岩或砂质泥岩,存在双向交错层理,层面有雨痕,应为潮坪沉积。潮坪沉积由小型层序构成,小型层序又是由砂、泥质单层组成。砂质单层底部通常为岩性突变面或侵蚀面,砂质纹层较厚,其中可见对称波痕或泥砾;向上砂质纹层变薄,过渡到泥质单层。砂质单层形成于暴风浪时期,泥质单层是风浪衰减后恢复正常的潮汐沉积。因此,小型层序从成因上说是一风暴层序。碎屑成份、砾石成份分析表明沉积物均来自华夏古陆的沉积岩和变质岩基底。物源一致,岩层产状变化不大,反映文昌组沉积环境稳定。岩性、粒度分析表明文昌组是一向上变细、由浅海高能环境向近岸低能环境过渡的沉积层序。文昌组下段为浅海砂岩沉积,上段顶部为潮坪沉积。二者之间是一套夹砾岩透镜体的泥质粉细砂岩,其沉积环境应介于浅海和滨岸之间,为水下岸坡沉积。砾岩层只是大的沉积旋回中出现的事件性水下冲积物。  相似文献   

Water and sediment outbursts from advanced Franz Josef Glacier,New Zealand   总被引：1，自引：0，他引：1  

Timothy R. H. Davies  Chris C. Smart  Jill M. Turnbull 《地球表面变化过程与地形》2003,28(10):1081-1096

The Franz Josef Glacier, Westland, New Zealand, has a history of catastrophic sediment‐laden outburst ?oods associated with extreme rainfall events when the glacier toe is advanced over its own sediments. Consideration of these events and inspection of recent sediment deposits suggest that there are three distinct modes of outburst. The ?rst is associated with fans fed by over?ow along the glacier margin. As the glacier has advanced across its own fore?eld gravels, it is inferred that the primary drainage conduit has developed a reach of negative slope. In high ?ows massive boulders can block the conduit, trapping lesser clasts. The resulting backup of water causes over?ows through marginal moulins, producing the fan type of deposit. The second type of outburst deposits massive imbricated boulders at a greater or lesser distance from the glacier portal. In this case, pressure buildup drives the blockage out of the portal where the boulders deposit. Smaller materials are generally carried away. The third type consists of very shallow ?ows, and produces massive gravel deposits of uncertain provenance. In this condition, the excess pressure in the conduit results in slight uplift of the glacier and widespread discharge of water and sediment below the glacier snout; gravels and smaller sediments are laid down in a massive deposit across the fore?eld. The massive, boulder‐veneered deposit from the December 1995 outburst is interpreted in the light of the above mechanisms as a hyperconcentrated ?ow deposit from hydraulic jacking, overlain by boulders emplaced by a subsequent conduit outburst. A possible association of outbursts with the present advanced position of the glacier is suggested. Copyright © 2003 John Wiley & Sons, Ltd.  相似文献   

Quantifying Storm Tide Risk in Cairns   总被引：6，自引：5，他引：6  

Ken Granger 《Natural Hazards》2003,30(2):165-185

The United Nations International Decade for Natural Disaster Reduction (IDNDR)gave rise to an increasing level of attention to the risks posed by a range of naturalhazards and the development of strategies by which to reduce those risks. It waswidely recognised that in order to evaluate risk treatment strategies it was necessaryto `measure' the level of risk that already existed and the level of risk that would beencountered with the treatment strategy(s) in place.This paper outlines the methodology developed under the AGSO (now GeoscienceAustralia) Cities Project to quantify the risk associated with storm tide inundation. It includes the methodology for `measuring' the level of community exposure to storm tide hazards and the methodology for `measuring' community vulnerability. The Far North Queensland city of Cairns is used as the case study to demonstrate the application of these methods.  相似文献