1998年5月29日皮山县6.2级地震烈度分布特征及损失评估     

王坚  寇大兵 《内陆地震》1999,13(1):50-57

１９９８年５月２９日皮山县发生６．２级地震,震中距皮山县城约３９ｋｍ,震源深度为３２ｋｍ,烈度分布区为北西－南东走向的椭圆形,极震区烈度为Ⅶ度,个别点为Ⅷ度,地震使皮山县县城,９个乡,２个镇,２个农场,墨玉县部分地区遭到不同程度的损失。共计受伤人数为２６人,其中重伤为２人,无家可归者人数为５５６６人,１３９２户,牲畜死亡４４５４头。地震造成的直接经济损失达５４８６．７５万元。  相似文献   

Pc3 pulsations during variable IMF conditions     

U. Villante  S. Lepidi  P. Francia  M. Vellante  A. Meloni  R. P. Lepping  F. Mariani 《Annales Geophysicae》1999,17(4):490-496

Pc3 geomagnetic field fluctuations detected at low latitude (L’Aquila, Italy) during the passage of a high velocity solar wind stream, characterized by variable interplanetary magnetic field conditions, are analyzed. Higher frequency resonant fluctuations and lower frequency phenomena are simultaneously observed; the intermittent appearance and the variable frequency of the longer period modes can be well interpreted in terms of the variable IMF elements; moreover their polarization characteristics are consistent with an origin related to external waves propagating in antisunward direction. A comparison with simultaneous observations performed at Terra Nova Bay (Antarctica) provides additional evidence for a clear relationship between the IMF and Pc3 pulsations also at very high latitudes.  相似文献   

A laboratory study of directional spectra with maximum likelihood method-Ⅰ Developing wind wave     

Zhao Dongliang  Masuda Akir  Wen Shengchang  Guan Changlong 《海洋学报(英文版)》1999,18(1):59-74

measurements by a circular array consisting of 18 wave gauges in a large wave tank, directional spectra of wind-generated waves in deep water are systematically determined by using maximum likelihood method The investigations reveal that the angular spreading of the wave energy is consistent with cos^2s(θ/2) proposed by Longuet-Higgins et al.(1963, Ocean Wave Spectra, 111-136), if the bimodal distributions of wave energy are not taken into account. Bimodality occurring on higher frequency than peak frequency is too rare to affect our whole resalts. Surprisingly, a much broader directional spreading than that of the field, which is interpreted by the strongly nonlinear energy transfer because of the very young waves in laboratory, is found. The parameter s depends on frequency in the same way as observed by Mitsuyasu et al.(1975, Journal of Physical Oceanography, 5, 750-760) and Hasselmann et al.(1980, Journal of Physical Oceanography, 10, 1264-1280) in the field, and the relationship between the four nondimensional parameters s_m, f_o, b₁ and b₂, determining the directional width, and ū₁₀ (corresponding to the inverse of wave age) are given respectively. The observed distributions are found to agree well with the suggestion of Donelan et al.(1985, Philosophical Transaction of Royal Society of London, A315, 509-562) when applied to field waves.  相似文献   

Interdecadal Variations of ENSO Signals and Annual Cycles Revealed by Wavelet Analysis     

Takashi Setoh  Shiro Imawaki  Alexander Ostrovskii  Shin-Ichiro Umatani 《Journal of Oceanography》1999,55(3):385-394

Interdecadal variations of El Niño/Southern Oscillation (ENSO) signals and annual cycles appearing in the sea surface temperature (SST) and zonal wind in the equatorial Pacific during 1950–1997 are studied by wavelet, empirical orthogonal function (EOF) and singular value decomposition (SVD) analyses. The typical timescale of ENSO is estimated to be about 40 months before the late 1970s and 48–52 months after that; the timescale increased by about 10 months. The spatial pattern of the ENSO signal appearing in SST also changed in the 1970s; before that, the area of strong signal spread over the extratropical regions, while it is confined near the equator after that. The center of the strongest signal shifted from the central and eastern equatorial Pacific to the South American coast at that time. These SST fluctuations near the equator are associated with fluctuations of zonal wiond, whose spatial pattern also shifted considerably eastward at that time. In the eastern equatorial Pacific, amplitudes of annual cycles of SST are weak in El Niño years and strong in La Niña years. This relation is not clear, however, in the 1980s and 1990s.  相似文献   

采用卫星高度计资料分析南海风、浪的月平均特征     

齐义泉  施平 《热带海洋学报》1999,18(2):31

在分析1987—1988年两年间Geosat卫星高度计遥感资料的基础上,给出了南海海面月平均风速和月平均有效波高的分布,以及沿南海NE－SW向的风、浪年变化特征;并与船舶报资料作了对比分析,其结果显示该高度计遥感资料与常规资料（船舶报资料）基本一致。  相似文献   

河口湾区生物扰动强度及扰动作用特征研究——以山海关大石河河口湾为例     

王英国  王珍如 《中国海洋大学学报(自然科学版)》1999,(4)

通过野外实际观察和室内模拟分析,依据现代沉积中的底内生物扰动构造三维结构清晰可辨的特征,认为现代河口湾的动物潜穴均可按照规则的几何体求得个体扰动指数,在此基础上,对河口湾地区生物扰动特点作了研究  相似文献   

Dust in the disk winds from young stars as a source of the circumstellar extinction     

L. V. Tambovtseva  V. P. Grinin 《Astronomy Letters》2008,34(4):231-240

We consider the problem of dust grain survival in the disk winds from T Tauri and Herbig Ae stars. For our analysis, we have chosen a disk wind model in which the gas component of the wind is heated through ambipolar diffusion to a temperature of ～10⁴ K. We show that the heating of dust grains through their collisions with gas atoms is inefficient compared to their heating by stellar radiation and, hence, the grains survive even in the hot wind component. As a result, the disk wind can be opaque to the ultraviolet and optical stellar radiation and is capable of absorbing an appreciable fraction of it. Calculations show that the fraction of the wind-absorbed radiation for T Tauri stars can be from 20 to 40% of the total stellar luminosity at an accretion rate ? _a = 10^?8-10^?6 M _⊙yr^?1. This means that the disk winds from T Tauri stars can play the same role as the puffed-up inner rim in current accretion disk models. In Herbig Ae stars, the inner layers of the disk wind (r ≤ 0.5 AU) are dust-free, since the dust in this region sublimates under the effect of stellar radiation. Therefore, the fraction of the radiation absorbed by the disk wind in this case is considerably smaller and can be comparable to the effect from the puffed-up inner rim only at an accretion rate of the order of or higher than 10^?6 M _⊙yr^?1. Since the disk wind is structurally inhomogeneous, its optical depth toward the observer can be variable, which should be reflected in the photometric activity of young stars. For the same reason, moving shadows from gas and dust streams with a spiral-like shape can be observed in high-angular-resolution circumstellar disk images.  相似文献   

基于谱烈度改进算法的研究与应用          下载免费PDF全文

李通    姚新强    郭迅  曹井泉  刘红艳 《世界地震工程》2023,39(1):189-199

本文基于Housner谱烈度公式中存在的不足和问题提出了一种改进算法,首先将相对速度反应谱积分公式上下限范围扩大为0.1～10.1 s,通过统计分析集集地震、汶川地震和芦山地震反应谱积分值和宏观烈度之间的关系,给出8组分档线性公式来计算改进谱烈度值I_s,并采用普通克里金插值法绘制谱烈度分布图。本文提出的改进算法在地震动加速度时程积分与谱烈度之间建立起一组长周期、连续性和精细化的函数关系,经鲁甸地震对比验证,该改进算法得出的谱烈度分布图与宏观烈度图整体变化趋势一致,谱烈度值与宏观烈度吻合率(偏差±1度以内)约为90%,具有一定的科学性和准确性,可为灾后应急救援以及决策部署等提供科学的数据支撑。  相似文献   

海上风电吸力基础在分层土中的沉贯特性研究综述     

李大勇  黄凌昰  张雨坤  吴学震 《海洋工程》2023,41(1):110-127

吸力基础与海洋工程大直径钢桩相比,具有成本低、安装周期短、对环境影响小、不受海况影响及可回收再利用等优点,近年来在海上风电工程中得到推广应用。吸力基础沉贯至海床预定位置,是其发挥承载力和确保服役稳定性的前提。海床地基土体常以分层土形式分布,且各层土体强度、压缩性和渗透性等存在显著差别,导致吸力基础吸力沉贯机理非常复杂。明确吸力基础在分层土中沉贯特性,有助于指导吸力基础在海上风电工程中的推广应用。对目前吸力基础在分层土中沉贯特性研究进行综述和总结,归纳了其沉贯机理研究进展,并对影响吸力基础在分层土中沉贯因素进行了分析;提出了分层土中吸力基础沉贯的研究方向和改进的沉贯方法。  相似文献   

前期风场控制的太湖北部湖湾水动力及对蓝藻水华影响   总被引：7，自引：6，他引：1  

吴挺峰  朱广伟  秦伯强  丁艳青  吴善锋 《湖泊科学》2012,24(3):409-415

为明确前期风场对太湖北部湖湾水动力及蓝藻水华分布的影响,对2008年9月梅梁湾及贡湖湾水文、水质及气象开展了同步观测,结果表明:受前期东北风影响,梅梁湾及贡湖湾表层、中层及底层湖流流向均顺风向自湾内流向湾外,两个湖湾均不存在补偿流.表层湖流对风场变化响应敏感,而中场及底层流场对风场变化响应存在显著滞时.在偏南风作用下,梅梁湾表层湖流能快速形成顺时针环流.在偏西风作用下,贡湖湾表层湖流流向虽未发生偏转,但是湖流流速显著减小并导致流速沿水体垂向呈递增分布.观测期间水动力强度对太湖北部湖区叶绿素a浓度垂向分层及蓝藻水华水平漂移均具有重要影响.在水动力滞缓水域,蓝藻水华易在水表发生漂移堆积.在水动力强度较大水域,强烈的垂向混合作用能使蓝藻沿水深方向混合均匀,降低水华暴发风险.相对于水动力条件,营养盐对叶绿素a浓度空间分布的影响较弱.  相似文献