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41.
宜兴抽水蓄能电站试验洞的反分析研究 总被引:4,自引:2,他引:4
结合江苏宜兴抽水蓄能电站地下厂房试验洞量测资料的分析,研究了成层各向异性岩体中洞室工程问题的反分析方法。采用分层均质模型进行反分析计算。计算区域的各层岩层均被分别视为均质各向同性体,初始地应力假设呈线性分布。有限元分析中,对倾斜成层的岩层、软弱夹层及断层节理等分别划分了单元,据以模拟成层岩体的各向异性特征。为使计算过程简化,对离洞室较远的岩层拟按地质资料对材料特性参数赋值,反分析计算的目标未知数为初始地应力和试验洞相邻围岩的弹性模量。结果表明,与工程实践符合较好。 相似文献
42.
GPS数据处理中IGS基准站的选取 总被引:7,自引:0,他引:7
IGS基准站的选取问题是目前GPS数据处理中讨论的热点问题。文中从基准站选取的几何意义、统计意义和物理意义3个方面分析讨论了IGS基准站的选取问题。并通过对理论及大量算例的分析,提出了IGS基准站选取的一般原则。 相似文献
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WANG Tiefeng Northeast Investigation Design Research Institute China ZHANG Zhi Northeast Investigation Design Research Institute China YI Yue Northeast Investigation. Design Research Institute China 《国际泥沙研究》1997,(3)
I.INTRODUCTIONThePtlmped-storagepoll,erprojectofPushiriverisconsistedofupperreservoir,lobal-erreset'oir.watertransmissionSystemandpotvergeneratingsystem.ThelowerreservoirIviththecatchmentbasinareaof1141kmZisthewatersupplierl-c'hichislocatedonthedownstreamofthePushiriverinthesouthernpactofNortheastChina.Theupperreservoirisabout300-400metershigherthanthelowerresen!oirattheleftsideoftheriverwithcatchmentbasinareaof1.12km2.Thecharacteristicsoftheprojectandreservoirareshottviintablel-l.Ino… 相似文献
46.
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
47.
陈伯舫 《地震地磁观测与研究》1997,18(2):40-44
用通日月均值减去夜均值计算的月均值资料和Sompi谱分析法分析了14个台站的北向分量1年周期变化的振幅向相位,时段为1984-1988年。分析结果显示用P^0n(dnd=1,…,6)复合模式的估算的C值较合理。各台的C值比较一致。 相似文献
48.
11 million years of Oligocene geomagnetic field behaviour 总被引:2,自引:0,他引:2
An 11 million year long record of the Oligocene geomagnetic field has been obtained from pelagic sediments of DSDP Hole 522 An average sample spacing of 4 cm yielded approximately one specimen per 4 to 8 kyr. The rock magnetics are remarkabh consistent across the entire interval. Previous work demonstrated a magnetic mineralogy dominated by magnetically stable magnetite. The natural remanent magnetism (NRM) carries an Oligocene polarity timescale that is in excellent agreement with the Oligocene reversal record as determined from marine magnetic anomalies (MMAs), including many of the so-called 'crypto-chrons'. Normalized NRM intensities from the undisturbed portions of the record yield a time series of variations with features consistent with a number of other palaeointensity time series derived from both sedimentary and lava sequences. These features include consistent, major decreases in palaeointensity (DIPs) at reversal boundaries, and occasional DIPs between reversal boundaries that could correspond to lineated 'tiny wiggles' in the MMA records. The data set suggests that the overall field strength was 40 per cent higher in the first half of the Oligocene when the average reversal frequency was 1.6 Myr-1 than in the second half when the reversal frequency was 4 Myr-1 . There is also a weak dependence of average field strength on length of polarity interval. Finally, in the three cores suited to spectral analysis (of coherent polarity and relative intensity independent of lithological contamination), there is a persistent ca. 30–50ka periodicity in the variations of the relative intensity, suggesting that the geomagnetic field 'pulses' at about this frequency, not only during the Brunhes (as demonstrated by Tauxe & Shackleton 1994), but in the Oligocene as well. 相似文献
49.
Chiyo Morimoto Yo-ichiro Otofuji Masako Miki Hidefumi Tanaka Tetsumaru Itaya 《Geophysical Journal International》1997,128(3):585-593
The geomagnetic field intensity during Archaean times is evaluated from a palaeomagnetic and chronological study of a dolerite dyke intruded into the 3000 Ma Nuuk Gneisses at Nuuk (64.2°N, 51.7°W), west Greenland. Plagioclase from the dolerite dyke yields a mean K-Ar age of 2752 Ma. Palaeomagnetic directions after thermal demagnetization of the dyke and the gneiss reveal a positive baked-contact test, indicating that the high-temperature-component magnetization of the dyke is primary. Thellier experiments on 12 dyke specimens yield a palaeointensity value of 13.5±4.4 μT. The virtual dipole moment at ca. 2.8 Ga is 1.9±0.6 × 1022 Am2 , which is about one-quarter of the present value. The present study and other available data imply that the Earth's magnetic field at 2.7 ∼ 2.8 Ga was characterized by a weak dipole moment and that a fairly strong geomagnetic field similar to the present intensity followed the weak field after ca. 2.6 Ga. 相似文献
50.
We studied the existence of dynamical stochastic relations in the evolution of the am index. A first analysis of the autocorrelation functions showed evidence of several seasonalities. We first used linear (ARMA) models, and it was found that these do not account for the whole internal dynamics of the data series. We then used various non-linear models to provide a better fit to reality. The forecast performances of the non-linear models are not significantly different from those of the linear model. We give a tentative explanation for the failure of the non-linear predictions. Finally, ARCH models were used in order to take into account the fact that the confidence interval for the predicted value depends on past observations. 相似文献