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111.
CK型陨石是一类高度氧化的碳质球粒陨石, 金属/磁铁矿的比值接近零. 与其它类型的碳质球粒陨石(岩石类型: 1-3)不同, 大多数CK型陨石在母体上经历了强烈的热变质过程(550--1270K), 以4-6型为主. 多项证据表明, CK和CV3型陨石具有成因联系. 但是, 两者在岩相结构和化学组成方面仍存在微小差异. 因此, 精细地区分和比较两者的地球化学特征对于验证CK-CV单一母体假说非常重要. Northwest Africa (NWA) 13943是一块新发现的陨石, 经历过较强烈的热变质作用. 利用扫描电子显微镜和电子探针, 确定了NWA 13943的岩石类型. 并运用质谱分析技术, 重点测定了NWA 13943陨石的全岩氧同位素和铬同位素组成. 综合岩石结构、矿物化学成分、氧同位素异常(△17O,△代表同位素分馏值)和铬同位素异常(ε54Cr, ε表示样品中的同位素比值与标样中的同位素比值的相对偏差的104倍),CK和CV型陨石的母体可能形成于原行星盘中两个相似但不同的化学源区.  相似文献   
112.
利用运动学轨道提高GRACE时变重力场解算   总被引:1,自引:1,他引:0       下载免费PDF全文
基于变分方程法,本文利用GARCE高精度K波段星间测速数据KBRR,结合德国格拉茨大学发布的运动学轨道和GFZ发布的简动力学轨道作为两种伪观测值,分别解算了2005-2010年60阶全球时变重力场模型Hust-IGG01与Hust-IGG02.通过与GRACE官方机构发布的模型和其他国际主流权威模型进行对比,发现基于运动学轨道结合KBRR解算的模型Hust-IGGO1优于基于简动力学轨道结合KBRR解算的模型Hust-IGG02:在重力场系数C_(20)时间序列的统计数据上,Hust-IGG01比Hust-IGG02更接近SLR结果,在如C_(60)、C_(70)、C_(80)以及C_(90)等重力场低阶项上的数学统计均更接近CSR RL05;Hust-IGG01的重力场系数误差分布和GFZ RL05在同一水平,而Hust-IGG02的误差估计过于乐观;Hust-IGG02在主要质量变化区域上存在5%~10%信号低估,而Hust-IGG01能完全达到国际主流机构利用GPS观测数据的解算水平,Hust-IGG01与官方机构CSR、JPL和GFZ最新模型在格陵兰岛的冰川消融年际趋势分别是-125.4、-125.4、-127.3、-124.3 Gt·a~(-1),在亚马逊流域的平均等效水高周年振幅分别是17.56、17.40、17.46、17.22 cm,在撒哈拉沙漠的平均等效水高均方差分别是0.87、0.77、1.10、0.87 cm;另外在Hust-IGG01的实际应用上,本文分析了全球32个主要流域质量变化的年际趋势、周年振幅和半周年振幅三种信号模式,统计结果显示Hust-IGG01与CSR RL05结果基本吻合.  相似文献   
113.
The particle trajectory on a weakly nonlinear progressive surface wave obliquely interacting with a uniform current is studied by using an EulerLagrange transformation. The thirdorder asymptotic solution is a periodic bounded function of Lagrangian labels and time, which imply that the entire solution is uniformlyvalid. The explicit parametric solution highlights the trajectory of a water particle and mass transport associated with a particle displacement can now be obtained directly in Lagrangian form. The angular frequency and Lagrangian mean level of the particle motion in Lagrangian form differ from those of the Eulerian. The variations in the water particle orbits resulting from the oblique interaction with a steady uniform current of different magnitudes are also investigated.  相似文献   
114.
港口、海洋工程结构物基础一般处于复合加载状态,其极限承载力通常采用近来引入的极限荷载图进行评价.对位于地基表面的重力式海洋基础,需要考虑基础与地基间的接触特性对极限承载力的影响.以大型通用有限元软件ABAQUS为计算平台,建立了复合加载模式的地基极限承载力数值分析方法;针对饱和黏土地基上的表面基础,利用在ABAQUS平台上开发的接触计算模块,模拟基础与地基间竖向可分离、切向完全粘结的接触作用;进而基于建立的分析方法,进行系统的有限元计算,分析地基的破坏模式随荷载条件的变化,给出地基的极限荷载包络图,并与经典承载力计算公式结果进行对比.研究结果表明,经典承载力计算公式低估了三维荷载条件下的地基极限承载力,有限元计算模型及数值分析方法,可以较好地分析研究地基的失稳机理及承载力特性,并可考虑基础与地基不同的接触条件对破坏模式及组合极限承载力的影响.  相似文献   
115.
Experiments are carried out to study the characteristics of active bubbles entrained by breaking waves as these propagate over an abruptly topographical change or a submerged breakwater. Underwater sounds generated by the entrained air bubbles are detected by a hydrophone connected to a charge amplifier and a data acquisition system. The size distribution of the bubbles is then determined inversely from the received sound frequencies. The sound signals are converted from time domain to time-frequency domain by applying Gabor transform. The number of bubbles with different sizes are counted from the signal peaks in the time-frequency domain. The characteristics of the bubbles are in terms of bubble size spectra, which account for the variation in bubble probability density related to the bubble radius r. The experimental data demonstrate that the bubble probability density function shows a-2.39 power-law scaling with radius for r>0.8 mm, and a-1.11 power law for r<0.8 mm.  相似文献   
116.
1INTRODUCTIONRiversinTaiwanarerelativelysteepercomparedtothoseinothercontinent.Localyocuredsupercriticalflowarefairlycommonin...  相似文献   
117.
Experiments are carried out to study the characteristics of active bubbles entrained by breaking waves as these propagate over an abruptly topographical change or a submerged breakwater. Underwater sounds generated by the entrained air bubbles are detected by a hydrophone connected to a charge amplifier and a data acquisition system. The size distribution of the bubbles is then determined inversely from the received sound frequencies. The sound signals are converted from time domain to time-frequency domain by applying Gabor transform. The number of bubbles with different sizes are counted from the signal peaks in the time-frequency domain. The characteristics of the bubbles are in terms of bubble size spectra, which account for the variation in bubble probability density related to the bubble radius r. The experimental data demonstrate that the bubble probability density function shows a - 2.39 power-law sealing with radius for r 〉 0. 8 mm, and a- 1.11 power law for r 〈0.8 mm.  相似文献   
118.
119.
On April 20, 2013, a magnitude M s 7.0 earthquake occurred in Lushan, Sichuan Province, China, and caused heavy casualties and economic losses. Based on the local broadband waveforms in Sichuan and adjacent provinces regional networks and teleseismic broadband records from IRIS stations, the focal mechanism and the focal depth are determined by the CAP (Cut And Paste) and its upgraded methods, CAPtele and CAPjoint, respectively. The results show that the focal mechanisms and depth from different methods are steady, and the best double couple solution derived from the joint inversion is 210°, 44°, and 91° for strike, dip, and rake angles respectively for one nodal plane and 29°, 46°, and 89° for another with 16 km focal depth and M w 6.66 moment magnitude. In order to verify the reliability of the results, a number of tests are performed based on local seismograms with different velocity models. They indicate that there is about 10 degree’s fluctuation in focal mechanisms and about 2 km variation in focal depth with a complex velocity structure. Furthermore, inverted by re-sampling the teleseismic waveforms on the basis of epicentral distance, the solutions are consistent with each other, which manifests that the teleseismic records are effective for constraining source parameters of the Lushan earthquake.  相似文献   
120.
Many previous studies have demonstrated that the boreal winters of super El Nino events are usually accompanied by severely suppressed Madden-Julian oscillation(MJO) activity over the western Pacific due to strong descending motion associated with a weakened Walker Circulation. However, the boreal winter of the 2015/16 super El Nino event is concurrent with enhanced MJO activity over the western Pacific despite its sea surface temperature anomaly(SSTA)magnitude over the Nino 3.4 region being comparable to the SSTA magnitudes of the two former super El Nino events(i.e.,1982/83 and 1997/98). This study suggests that the MJO enhanced over western Pacific during the 2015/16 super El Nino event is mainly related to its distinctive SSTA structure and associated background thermodynamic conditions. In comparison with the previous super El Nino events, the warming SSTA center of the 2015/16 super El Nino is located further westward, and a strong cold SSTA is not detected in the western Pacific. Accordingly, the low-level moisture and air temperature(as well as the moist static energy, MSE) tend to increase in the central-western Pacific. In contrast, the low-level moisture and MSE show negative anomalies over the western Pacific during the previous super El Nino events.As the MJO-related horizontal wind anomalies contribute to the further westward warm SST-induced positive moisture and MSE anomalies over the western tropical Pacific in the boreal winter of 2015/16, stronger moisture convergence and MSE advection are generated over the western Pacific and lead to the enhancement of MJO convection.  相似文献   
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