上海大气折射指数振动及其与降水量和太阳黑子的关系

用交叉谱分析方法研究近地面大气折射指数N单位平均值、月降水总量与太阳黑子相对数之间多频振动特征。结果发现:初夏,N单位与太阳黑子(或降水量)在准5年及准2年(或准7年、准4年及准3年)周期附近有十分密切的关系;初秋,N单位与太阳黑子在准5年、准2年周期附近密切相关;N单位与降水量除在短周期准3年、准2年附近有密切关系外,在长周期准35年附近亦有较密切的关系。     

遥感图像处理中比值法的解析及其应用

本文从物理光学的基本数学模型出发，将卫星图像分解成直接光照区和阴影区两个分模型，运用朗伯面的光照原理，说明经大气散射校正后的比值图像与照度、太阳入射角和漫射光无关。这种图像处理技术可加大地物光谱反差、消除阴影效应、有效地区分同一属性的地质体并可判译可能与矿化有关的色形图像异常。文章结合作者近年来对遥感构造研究的部分成果，表明经大气散射校正后的比值图像，对华南与钨锡矿化有关的隐伏或半隐伏小岩体的蚀变带、华北金伯利岩及其共生的碱性岩脉的预测有着广泛的应用前景。     

球面方模板地形改正公式及其应用

在给出球面圆盘重力公式的基础上,导出了便于使用高程数据库和电子计算机的球面方盘重力公式,通过实际算例,证明了该公式高精度和可用性.     

几种地形校正方法的研究

本文推证了三种典型的地形校正方法(局部地形改正(C),剩余地形改正(RTM)爱黎-海斯卡宁型地形均衡改正(t_C)之间的数学关系,对其特性进行了分析比较;讨论了它们实现的途径(数据处理方法)及其计算特征;最后还应用某地区的实测地形高数据进行了实际计算,得出了一些有益的结论。     

灌木植被分布区阻力特性理论及试验研究

为探明河道灌木植被分布区阻水规律，对灌木植被主干、分枝产生的水流阻力特性及其定量特征进行研究。提出原型植被体积修正系数和灌木植被水力半径确定方法，理论推导灌木植被阻力系数计算公式，并结合水槽试验建立植被阻力系数与植被水力半径为特征长度的植被雷诺数之间的关系式。研究结果表明：引入原型植被体积修正系数和灌木植被水力半径使灌木植被阻力计算更为准确；植被阻力系数与植被雷诺数之间呈指数函数关系，随植被雷诺数的增加呈单调减小的趋势，与水槽试验结果吻合很好。     

Lateral variations of the local magnitude at Ebre station,Northeastern Iberian Peninsula

Since 1984, a seismic surveillance at the Baix Ebre Region (NE of the Iberian Peninsula) has been carried out from a seismic network consisting of two digital and one analog stations. Large discrepancies between the recorded amplitudes and the magnitude estimates given by different agencies have been observed. To explain these discrepancies, that consist of a large reduction of amplitude and a strong dependence of the azimuth, a local magnitude formula for the area has been computed, using the analog records obtained at EBR short-period station. Global results show an average station correction factor between the computed local magnitude and the reported magnitude of the order of 1, presenting large variations around the mean value with a clear dependence on the azimuth. A detailed analysis of this variation around the mean value reveals that earthquakes can be classified according to their location in different geological units, thus obtaining for each zone a distinct station correction factor that can fluctuate as much as 0.6 around the average. These large lateral variations of the magnitude are in good agreement with previous studies of coda-Q attenuation.     

Statistical results from a jcmt survey of MM and sub-MM emission in herbig ae/be stars

We have detected 1.1 mm continuum emission from 24 of 53 Herbig Ae/Be stars surveyed with the JCMT. Survival analysis shows that 1.1 mm luminosity is correlated with bolometric luminosity and with IRAS 25µm luminosity. For those stars that were also detected at 0.45 or 0.8 mm we find a typical flux dependence of the form S _#x03BD; ³, which is steeper than that of most classical T Tauri stars.     

Masers, Lasers and the Interstellar Medium

This paper discusses recent results obtained by myself and my colleagues in three domains of astrophysics: interstellar supersonic turbulence, circumstellar disks, and natural masers and lasers. S.A. Kaplan, S.B. Pikelner, and I.S. Shklovskii were among those who, 30-40 years ago, laid the foundation of these domains.H2O masers become an effective probe of supersonic turbulence associated with mass outflow from very young stars. They demonstrate a very low (1) fractal dimension of the spatial set on which turbulence dissipates its kinetic energy, and, thereby, a strong intermittency of the turbulence. They also indicate that supersonic turbulence, like incompressible turbulence, has an inner scale, on which the bulk of turbulent energy dissipates in low-Mach, random shocks. H2O masers themselves find thereby a new pumping source in these random shocks.Masers in hydrogen recombination lines, discovered 8 years ago, originate in a circumstellar disk surrounding a massive star MWC 349A. They give a possibility to investigate kinematics and structure of the disk. Far-infrared nydrogen recombination lines, recently detected in MWC349A from the Kuiper Airborn Observatory, proved to be amplified as well. They are the first known natural amplifiers of electromagnetic waves in the laser wavelength domain. Analysis of their radiation, along with the radiation in other recombination lines, gives a possible key to understanding the lack of optical lasers in the Universe.     

宽角反射、折射地震数据与重力数据综合解释龙门山及邻近地区地壳结构

青藏高原东部的隆升机制一直都是地学界的研究热点,研究学者们提出和发展了多种岩石圈变形模型,而存在多种模型的主要原因之一是对青藏高原东部地壳及岩石圈结构认识不足。本文主要针对SinoProbe-02项目横跨龙门山断裂带、全长400多公里的宽角、折射地震数据及重力数据进行联合反演和综合解释。研究结果表明,龙门山及邻近地区地壳结构可明确划分为上地壳、中地壳和下地壳。上地壳上层为沉积层,龙门山断裂带以西大部分区域被三叠纪复理岩覆盖,而在龙日坝断裂与岷江断裂之间出现了密度为2.7g/cm³的高速异常体;向东靠近龙门山地区,沉积层厚度逐渐减薄。中地壳速度变化不均一,而且变形强烈;若尔盖盆地和龙门山断裂带下方出现明显低速带;中地壳在龙门山西侧厚度加厚,在岷江断裂下方和四川盆地靠近龙门山断裂带地区附近厚度达到最大。莫霍面整体深度从东往西增厚,最厚可达56 km。本次研究得到的地壳结构和密度分布分析结果表明现有的地壳厚度和物质组成不足以支撑龙门山及邻近地区目前所达到的隆升高度,因此四川盆地刚性基底西缘因挤压作用产生的弯曲应力也是该地区抬升的重要条件之一。     

微波湿度计资料在GRAPES模式中偏差订正方法研究

根据微波湿度计MHS(Microwave Humidity Sounder)辐射率资料及GRAPES(Global/Regional Assimilation and Pr Ediction System)模式的特点,建立适用于MHS资料的偏差订正系统,该系统包括扫描和气团偏差订正,其中气团偏差订正考虑水汽资料的特性,采用三种不同预报因子组合的方案。偏差订正结果表明:MHS各个通道的扫描偏差表现出不同特征;偏差订正后观测残差基本服从均值为零的高斯分布,且观测残差的均值有所降低并随时间变化平稳;三种气团偏差订正方案都有明显的订正效果,其中方案三的订正效果最佳。