Non-Newtonian topographic relaxation on Europa

Models of topographic support on Europa by lateral shell thickness variations have previously assumed a Newtonian ice viscosity. Here I show that using a more realistic stress-dependent viscosity gives relaxation times which can be significantly different. Topography of wavelength 100 km cannot be supported by lateral shell thickness variations for ∼50 Myr, unless the shell thickness is <10 km or the ice grain size >10 mm. Shorter wavelength topography would require even thinner shells, but may be supported elastically. Global-scale variations in shell thickness, however, can be supported for geological timescales if the shell thickness is O(10 km).     

中国西北地区云的分布及其变化趋势

利用1983年7月—2001年9月ISCCP D2云的月平均资料,针对西北地区15种不同类型云的分布特征进行了分析,给出了中、低云量之和以及高云量在3个气候子区的多年变化趋势,初步探讨了其形成机制。结果表明:水层云、冰层云、水雨层云、冰雨层云和深对流云的光学厚度和云水路径值最大;水层云主要出现在天山山区、北疆地区和陕西南部,冰层云主要出现在北疆地区,水雨层云、冰雨层云和深对流云以及水高层云、冰高层云、卷层云的云量高值区在天山—昆仑山—祁连山一带以及陕南和/或陇南地区,因此上述地区也是有利于人工增水作业的地区。近20年中,高云量在3个气候区都呈明显下降趋势,中、低云量之和则呈上升趋势。西北地区云与地气系统之间可能存在这样一个过程:地面气温的升高,促使地面蒸发加剧,从而导致中、低云量增多而使降水增多,同时高云云量减少。     

考虑基桩嵌岩段侧阻的岩溶区顶板安全厚度计算

为考虑岩溶区基桩嵌岩段侧阻力的影响,提出了一组确定岩溶区桩端顶板安全厚度的计算方法。考虑顶板的整体承载效应,结合弹性力学及第一强度理论,得到了顶板抗弯安全厚度计算式;考虑嵌岩段桩侧摩阻力对桩顶荷载的分担作用,结合格里菲斯判据及摩尔判据,获得了顶板抗冲切和剪切的安全厚度计算公式,进而运用ABAQUS建立了岩溶顶板与基桩整体分析计算模型,有限元计算结果与理论计算值吻合良好。结合工程实例重点分析了顶板厚跨比对抗弯安全厚度的影响,顶板岩层厚度对抗冲切、剪切安全厚度的影响以及嵌岩段侧摩阻力系数?对顶板安全厚度计算的影响。     

桩顶加筋灰土垫层理论分析与工程设计探讨

目前,加筋垫层的工程实践超前于其理论研究,桩顶加筋灰土垫层设计方法受到普遍关注。以郑－西客运专线深厚湿陷性黄土地基处理为工程背景,建立了桩顶加筋灰土垫层理论模型,分析了桩顶垫层荷载特征,提出了灰土垫层设计极限状态理论。考虑不同桩径、不同桩间距、不同路基高度和不同格栅强度情况,对灰土垫层厚度等进行了参数影响性分析。建议高速客运专线路基桩顶垫层设计中宜采用双层、双向土工格栅结构形式,并优先选用延伸率小的筋材。     

声波测井薄层厚度计算公式的研究与应用

以解决工程实践难题为目的,首次提出了根据换能器与薄层所处位置不同,分别利用其不同求薄层厚度公式之观点。研究了声波测井薄层厚度定量计算公式,详细介绍了公式在高背景上检出Vp低值薄层,在低背景上检出Vp高值薄层的应用情况。并就薄层纵波速度的获取以及如何选用合适计算公式等问题作了一些探讨。同时,通过实例证明了这些措施对提高薄层厚度定量计算精度的重要性。     

Pn arrivals and lateral variations of Moho geometry beneath the Kaapvaal craton

Pn arrivals from mining-induced earthquakes on the edge of the Witwatersrand basin show that the P wavespeeds in the uppermost mantle are almost constant throughout most of the Kaapvaal craton. The presence of only small wavespeed variations allows the use of a simple method of estimating crustal thicknesses below the stations of the Kaapvaal broad-band network using Pn times that has been compared with results from receiver functions. One thousand three hundred thirty-seven Pn arrivals were used to derive crustal thicknesses at 46 stations on the Kaapvaal craton. The average crustal thicknesses for 19 centrally located stations on each of the northern and southern regions of the craton that yielded well-constrained thicknesses were 50.52±0.88 km and 38.07±0.85 km, respectively. In contrast, the corresponding average thicknesses determined from receiver functions were 43.58±0.57 km and 37.58±0.70 km, respectively. The systematically lower values for receiver functions in the northern part of the Kaapvaal craton that was affected by the Bushveld magmatism at 2.05 Ga, suggest that the receiver functions do not enable the petrological crust mantle boundary to be reliably resolved due to variations in composition and metamorphic grade in a mafic lower crust. The Pn times also suggest pervasive azimuthal anisotropy with maximum wavespeeds of about 8.40 km/s at azimuths of about 15° and 217° in the northern and southern regions of the craton, respectively, and minimum wavespeeds of about 8.25 km/s.     

新疆巴楚和塔什库尔干地震台下方地壳结构研究

Using the teleseismic waveform data recorded by the seismic station Bachu( hereafter referred to as station BCH) i n the Tarim Basin and the seismic station Taxkorgan(h ereafter referred to as station TAG) i n the west Kunlun Mountains for years,we applied the receiver function H-κ stacking method to study the crustal structure beneath stations BCH and TAG. The results showed that there are obvious differences in the crustal thickness beneath stations BCH and TAG,and the regional crustal thickness and terrain have a very good corresponding relationship. There are high crustal average V P/ V S values beneath the two stations. The crustal thickness is 44 km,and the crustal average wave velocity ratio is 1. 849 beneath station BCH. There is a sharp discontinuity in the middle of the crust beneath station BCH at a depth of 21 km. There is a low average P wave velocity and low V P/ V S from the surface to the discontinuity beneath station BCH.The depth of the discontinuity is consistent with the lower interface of the focal depth from accurate location in the Jiashi earthquake source area adjacent to station BCH; and may be the crustal brittle-ductile conversion boundary. The crustal thickness is 69 km,and the crustal average wave velocity ratio is 1. 847 beneath station TAG,a thicker crust and high V P/ V S may indicate that materials in the lower crustal are prone to plastic flow,which is responsible for the thickening of the crust.     

一种求气井二项式方程系数的新方法

针对开发早期气田缺乏产能试井资料的实际情况，由于无法用传统的压力降法计算产能方程，故而基于最优化算法，提出了一种利用稳定生产数据和井控储量求取气井产能方程系数的新方法。在只知道稳定生产数据情况下便可进行计算分析。该方法在气田进行了实际应用，并和实际资料以及传统试凑法计算的结果进行了比较，表明方法的计算结果较为可靠。     

乌鲁木齐河流域地下水水位监测网设计

文章阐述了乌鲁木齐河流域区域地下水水位监测网的优化设计。基于ARCGIS技术,运用水文地质学方法在叠加合成地下水动态类型分区图的基础上优化设计了区域地下水水位监测网密度;采用时间序列分析方法确定了地下水水位监测频率。首期施工安装了11个新的长期专门监测孔;对73个现有监测孔进行了维修并安装了孔口保护装置,安装了28套水位自动监测仪,初步实现了地下水水位的自动监测。     

厚度对月壤微波辐射亮温的影响

基于嫦娥系列卫星微波辐射计数据的月壤厚度反演是中国月球科学研究的重要目标之一。基于辐射传输方程,数值模拟了不同频率、（FeO+TiO₂）含量和表面温度条件下厚度对月壤微波辐射亮温的影响;基于嫦娥二号卫星微波辐射计（Chang’E Lunar Microwave Sounder,CELMS）数据,结合Apollo 计划获取的月壤厚度资料及其他月壤厚度资料,系统分析了厚度对CELMS观测数据的影响。结果表明：频率、（FeO+TiO₂）含量、表面温度对亮温的影响远大于厚度对亮温的影响,是基于CELMS数据进行月壤厚度反演的重要影响因素;低频、低（FeO+TiO₂）含量、低温条件下,厚度对CELMS数据的影响最大;利用3 GHz、凌晨时刻的CELMS数据进行月陆地区月壤厚度反演可行。研究结果对基于嫦娥系列卫星CELMS数据的月壤厚度反演具有重要参考意义。