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61.
大气气溶胶光学厚度的宽带消光遥感方法及其应用 总被引:6,自引:1,他引:6
该文发展了遥感气溶胶光学厚度的一个宽带消光遥感方法 ,它应用地面上太阳直射表探测的宽波段太阳直射信息反演 0 75 μm大气柱光学厚度。这方法的主要误差因子是气溶胶谱的不确定性。数值试验表明 ,气溶胶谱分布的误差所引起光学厚度解的误差一般小于 5 %。 1995年 1— 10月进行的 12 6 7组对比实验表明 ,由本方法探测的气溶胶光学厚度与光度计探测的气溶胶光学厚度的标准差为 10 5 % ,两者平均结果的偏差只有 0 7%。该文还应用这个方法 ,从气象台站辐射观测资料反演得到北京、沈阳等 10个地方 1980— 1994年间晴天气溶胶光学厚度资料 ,并分析其变化规律 相似文献
62.
63.
本文介绍了采用相遇观测系统中全部走时分支曲线双向同时二维反演拟合法。对翁牛特东部地区的三条剖面基底折射资料二维反演,文中展示了各条剖面的理论走时对比图,射线追踪图,二维速度结构分布图,一维速度柱状图以及理论地震图。 相似文献
64.
利用卫星观测的长波磁异常,用等效偶极源方法推导了中国地区的视磁化强度分布.因卫星的高度远大于磁性地壳的厚度,将视磁化强度转换成磁化强度的垂直积分,它代表地壳内磁性物质的区域变化,利用视磁化强度与地表热流相应关系,计算了中国的新疆和东部一些地区居里等温面的深度.新疆地区的居里面深度为35-50km,其分布形态与塔里木盆地和准噶尔盆地的地貌比较相似;中国东部一些地区居里面深度在20-40km之间,与一些作者用航磁等数据得到的居里深度十分接近. 相似文献
65.
Ming Zhao Charles A. Langston rew A. Nyblade Thomas J. Owens 《Geophysical Journal International》1997,129(2):412-420
An Mw 5.9 earthquake occurred in the Lake Rukwa rift, Tanzania, on 1994 August 18, and was well recorded by 20 broad-band seismic stations at distances of 160 to 800 km and 21 broad-band stations at teleseismic distances. The regional and teleseismic waveforms have been used to investigate the source characteristics of the main shock, and also to locate aftershocks that occurred within three weeks of the main shock. Teleseismic body-wave modelling yields the following source parameters for the main shock: source depth of 25 ± 2 km, a normal fault orientation, with a horizontal tension axis striking NE-SW and an almost vertical pressure axis (Nodal Plane I: strike 126°–142°, dip 63°–66°, and rake 280°–290°; Nodal Plane II: strike 273°–289°, dip 28°–31°, and rake 235°–245°), a scalar moment of 4.1 times 1017 N m, and a 2 s impulsive source time function. Four of the largest aftershocks also nucleated at depths of 25 km, as deduced from regional sPmp–Pmp times. The nodal planes are broadly consistent with the orientation of both the Lupa and Ufipa faults, which bound the Rukwa rift to the northeast and southwest, respectively. The rupture radius of the main shock, assuming a circular fault, is estimated to be 4 km with a corresponding stress drop of 6.5 MPa. Published estimates of crustal thickness beneath the Rukwa rift indicate that the foci of the main shock and aftershocks lie at least 10 km above the Moho. The presence of lower-crustal seismicity beneath the Rukwa rift suggests that the pre-rift thermal structure of the rifted crust has not been strongly modified by the rifting, at least to depths of 25 km. 相似文献
66.
The Darwin Rise has been proposed so many times and in so many forms and places that the time has come to make a more comprehensive examination of the region. Lying on the NW Pacific Plate between the Geisha Guyots, the Mid-Pacific Mountains, the equator, and the trenches, the region is roughly bounded by magnetic anomaly M20 (147 Ma). It was subjected to a massive outpouring of lava about 105 to 120 Ma, which created the guyots and seamounts in that region. Guyots are excellent tools for studying events of long ago because they eroded in the same lowstand in the Cretaceous and guyot relief, therefore, is a surrogate for paleo-sealevel. The relief is derived by subtracting the break depth of the summit plateau of a guyot from the regional depth. Guyot relief would necessarily be less in the center than to the periphery if the feature formed on a pre-existing rise, as has been postulated. The existence of a paleo-Darwin Rise would give concentric contours for the region in question. Of the sixty guyots used in this study, thirty-seven of these guyots were surveyed using SASS multibeam in the Marcus-Wake seamount group. Twenty-three guyots were surveyed using random track single-beam sonar surveys. An entirely different scenario is shown. Data revealed a major fracture passing through the area coevally or after the guyots formed. Because the depths to the summit are not the same now, vertical tectonics occurred after subaerial erosion. This means the fracture formed during and after the erosion (roughly 105 Ma) and influenced the normal sequence of events in guyot formation. Depending on how one deciphers trends through the Hess Rise morass, SASS bathymetry shows a continuation of the Surveyor/Mendocino fracture zone swarm inside the M20 region to the NE of these data. The fracture swarm continues to the western Pacific trench system. Based on this information, if the Darwin Rise ever existed, it had to have done so elsewhere. 相似文献
67.
测氡法快速确定油气田边界及深度 总被引:5,自引:0,他引:5
叶树林 《华东地质学院学报》1996,19(2):150-156
本介绍了运用测氡法快速确定大庆××油气田边界,估算其埋藏深度试验,结果表明,该方法具有可行性和实用性。由于所做工作有限,尚属经验性探讨,还必须从理论和实践上进一步地工作,进而充实、完善它。 相似文献
68.
天山地震活动区的深部构造特征 总被引:1,自引:0,他引:1
以地壳介质的P波速度分布和导电性为基础,描述了天山地区几个主要地震活动区域深部构造特征,地震大都发生在地壳内不同速度块体之间的过渡带附近;沿着天山的南缘和毗邻塔里木盆地的西昆仑、阿尔金等山前地带,壳内高导层由北向南、由东向西逐渐加深并增厚,它们与所在地区震源深度的分相相吻合。这种不稳定的地壳结构有长期受力情况下非常容易发生形变甚至破裂而引发地震。 相似文献
69.
The time evolution of stratospheric aerosol layer formed after a volcanic eruption is studied taking into account the aerosol
microphysical processes of growth, coagulation and sedimentation. Using a simple model we could explain the observed evolution
of the Pinatubo volcanic layer which decayed in about 3 years. The experimental data obtained by Nd:YAG backscatter lidar
over Ahmedabad further supports this finding. The data obtained after the El Chichon volcanic eruption also showed that the
El Chichon aerosol layer decayed in about 3 years time. Thus, though the amount of SO2 injected has been higher, in the case of Pinatubo, about two to three times more than El Chichon, it has resulted in the
production of larger aerosol particles due to faster growth and coagulation processes, and subsequently a faster removal rate,
to give more or less a similar background aerosol amount at the stratosphere in about 3 years time. 相似文献
70.
Measurement and research method of metallogenic depths of Jiaojia orefield and Linglong orefield Shandong Province, China 总被引:1,自引:0,他引:1
Guxian Lü 《中国科学D辑(英文版)》1997,40(5):449-455
Taking the contribution of the tectonic force to the total hydrostatic pressure into account, the author puts forward a new
method on the calculation of the depth of petrogenesis and metallogenesis which is summarized as follows: first the tectonic
added hydrostatic pressured Ps is subtracted from the total hydrostatic pressure P, then using their difference Pr, according to the general method the depth of petrogenesis and metallogenesis can be determined in consideration of lateral
constraint.
By the new method the following data on the depths of the metallogenesis are obtained: 2 243.6 m (No. I and No. II veins with
metallogenic epoch of 105 Ma) and 1 632. 38 m (No. III vein with 105 Ma) for Jiaojia orefield, and 3 454.97 m (NE-trending
zone with 213.2 Ma), 1 902.79 III (ENE-trending zone with 100.28 Ma), 1 090.97 m (NE-trending zone with 80.67 Ma) and 720.55
m (NNE-trending zone with 71.86 Ma) for Linglong orefield.
Project supported by the Foundation of the State Planning Commission, China and the Foundation of the State Science and Technology
Commission, China. 相似文献