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A series of solar flare and coronal mass ejection (CME) event occurred in July 2000, particularly the largest flare (X5.7/3B) with CME on 14th of July since 1989, which stimulated a great geomagnetic storm with Dst index reaching -300 nT. A number of data have been obtained from the Chinese Antarctic Zhongshan Station (ZHS, INT Lat. 74.5°, L≈14）, which is located at cusp latitude, and from the ACE satellite. After analyzing these data we have got the results as follows: a lot of solar high energy particles penetrated into the polar ionosphere and ionized it, which significantly increased the cosmic noise absorption (CNA) and blanked the DPS-4 data for more than two days. The magnetic pulsation in Pc 3/5 frequency band on the ground has a high relation with the fluctuation of interplanetary magnetic field (IMF) Bz, which shows the contribution of interplanetary magnetohydrodynamical (MHD) waves to the Pc 3/5 pulsation on the ground. The Pc 3/5 pulsation was intensified much during the great magnetic storm. The H component of the magnetic field at ZHS varied with the southern value of IMF Bz but lagged behind for about 8 10 h. While Dst index responded to the variation of the IMF Bz very quickly, which suggested that the magnetic storm occurred at low latitude firstly and then effected the ionospheric current at high latitude. 相似文献
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土体小应变剪切模量在基坑、隧道等地下工程的计算分析中有着重要作用,越来越受到人们的关注。虽然上海地区地下工程项目的建设规模不断扩大,但关于上海典型黏土层的小应变剪切模量的研究相对较少。分别采用现场波速测试和室内弯曲元试验对上海典型黏土层的初始剪切模量进行了研究。试验结果表明：在减小土样扰动、保持土样应力状态与原位土体等效的基础上,弯曲元试验得到的初始剪切模量与现场波速测试相一致;考虑了土体应力状态和孔隙比的经验公式能够合理地描述上海典型黏土层初始剪切模量的变化规律,并给出了各土层的经验参数。试验结果可为上海地区地下工程计算分析中小应变剪切模量的估算提供参考。 相似文献
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20 0 0年 7月 ,太阳表面发生了一系列的耀斑与日冕物质抛射事件 ,最大耀斑能级达X5 .7/3 B。地球表面发生相应特大磁暴 ,Dst指数最大负偏达 - 3 0 0 n T。中国南极中山站地处极隙区纬度 ,白天位于磁层极隙区 ,夜间位于极盖区 ,以多种高空大气物理观测设备详细记录了该磁暴过程。对有关数据的分析表明 ,高能粒子引起电离层吸收急剧增加 ,测高仪数据两天多信号空白 ,宇宙噪声吸收显著增加 ;地磁 Pc3 /5脉动增加与行星际磁场南向分量密切对应 ,显示行星际磁流体波对激发磁层脉动的贡献 ;磁暴主相期间 ,Pc3 /5脉动大幅度增加 ;极区地磁水平分量随南向行星际磁场变化 ,但滞后近 8小时 ;Dst指数与南向行星际磁场密切相关 ,磁暴受控于高度负偏的南向行星际磁场 相似文献
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软土地区采用灌注桩围护的深基坑变形性状研究 总被引：14，自引：1，他引：13
根据上海软土地区80个钻孔灌注桩围护的深基坑工程案例有关数据,系统地分析了基坑开挖引致的灌注桩变形性状。所有基坑的灌注桩最大侧向位移介于0.1 %～1.0 %倍的开挖深度之间,平均值为开挖深度的0.44 %。钢筋混凝土支撑和钢支撑在控制墙体的变形上没有明显差别,最大侧向位移一般位于开挖面上下5 m的范围内。无量纲化最大侧向位移随着支撑系统刚度的增大而减小,随着墙底以上软土层厚度的增加而增大,但与灌注桩插入比及坑底抗隆起稳定系数之间并无明显的关系。墙顶侧向位移随着首道支撑位置深度的增加而呈现出指数增长的趋势,而灌注桩最大侧向位移与首道支撑的深度位置无明显关系。 相似文献
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从水文地球化学角度研究鄂尔多斯盆地南区白垩系地下水的排泄途径 总被引：4，自引：2，他引：2
主要从水文地球化学的角度,以鄂尔多斯盆地白于山以南地区白垩系地下水的水化学水平分带和地表水基流水化学特征为主要依据,结合地质构造格局及岩相古地理条件,分析研究了该区白垩系地下水的补、径、排条件。认为该区白垩系地下水水化学场存在一个由东、北、西南向中部的水平分带,愈向盆地中部水质愈复杂、TDS愈高。马莲河基流水质的沿途变化规律反映出其接受东西两侧地下水的补给。说明鄂尔多斯盆地南区的东部地区和西南部地区为地下水补给区,而中心地带为地下水排泄区,最终经马莲河排出区外。天环向斜轴部和马莲河谷是南区汇集东西两侧地下水的排泄通道。 相似文献
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鄂尔多斯盆地白垩系含水层系统分析 总被引：18，自引：2，他引：16
从地下水含水层系统的角度对鄂尔多斯盆地白垩系地下水系统进行了划分和分析。由于下白垩系统保安群为一套陆相碎屑岩建造,岩性复杂,由砂岩、粉砂岩和泥岩组成的频繁交替、重复叠置的多层层状结构,决定了鄂尔多斯白垩系自流水盆地是多层结构的地下水系统。这种重复叠置的多层层状地质结构,决定了地下水含水层系统的多层性、承压性及层与层之间的相对封闭性。根据沉积旋回和含水介质的性质,在全盆地范围内把白垩系地下水系统从上向下划分为：罗汉洞含水岩组、环河含水岩组和洛河含水岩组。通过对这3大含水岩组分别进行了分析认为,洛河含水岩组和环河含水岩组分布范围广、,含水层厚度大、天然资源丰富,是盆地区具供水意义的主要含水岩组。罗汉洞含水岩组因分布面积小,含水层厚度差异大、水质变化大,除陇东地区外,大部分地区供水价值较小。 相似文献
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Using the ground observation data at Zhongshan Station of Antarctica during July 13 to 17, 2000, the intense absorption events associated with the activities of the solar active region R9077 are analyzed. It was shown that an intense polar cap absorption event lasted more than 3 days, which was caused by the solar proton event associated with the X5/3B major flare at 1024 UT on July 13. The polar cap event started at about 1040 UT on July 14, and lasted to about 1940 UT on July 17, with a typical day night variation. At the same time, the intense solar activities extremely disturbed the magnetosphere, therefore aurora substorms occurred frequently. The energetic particle precipitation from the magnetosphere caused several absorption spikes superposing on the background of polar cap absorption. One distinct event is the absorption enhancement that started at about 0300 UT on July 15, reached its peak of 26 dB at about 0645 UT and recovered at about 1110 UT on the same day, which was the strongest absorption event observed at Zhongshan Station since the imaging riometer installed in February, 1997. Another outstanding absorption spike with pulsation occurred at about 1753 UT on 14th, its peak reached to 6 dB. 相似文献
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