A unified linear theory of wavelike perturbations under general ocean conditions

A linearized instability analysis model with five unknowns was proposed to describe disturbance motions under general oceanic background conditions, including large-scale current shear, density stratification, frontal zone, and arbitrary topography. A unified linear theory of wavelike perturbations for surface gravity waves, internal gravity waves and inertial gravity waves was derived for the adiabatic case, and the solution was then found using Fourier integrals. In this theory, we discarded the assumptions widely accepted in the literature concerning derivations of wave motions such as the irrotationality assumption for surface gravity waves, the rigid-lid approximation for internal gravity waves, and the long-wave approximation for inertial gravity waves. Analytical solutions based on this theory indicate that the complex dispersion relationships between frequency and wave-number describing the propagation and development of the three types of wavelike perturbation motions include three components: complex dispersion relationships at the sea surface; vertical invariance of the complex frequency; and expressions of the vertical wave-number (phase). Classical results of both surface waves and internal waves were reproduced from the unified theory under idealized conditions. The unified wave theory can be applied in the dynamical explanation of the generation and propagation properties of internal waves that are visible in the satellite SAR images in the southern part of the China Seas. It can also serve as the theoretical basis for both a numerical internal-wave model and analytical estimation of the ocean fluxes transported by wavelike perturbations.     

How Fast Could a Proto-pulsar Rotate?

According to two estimated relations between the initial period andthe dynamo-generated magnetic dipole field of pulsars, we calculate the statisticaldistributions of pulsar initial periods. It is found that proto-pulsars are very likelyto have rotation periods between 20 ms and 30 ms, and that most of the pulsarsrotate initially at a period ＜ 60 ms. Our result supports the asymmetric neutrinoemission model for pulsar kick.     

射电脉冲星观测资料及其启示

在本文中先简要介绍了８０年代以来射电脉冲星方面的观测进展，然后详细介绍了射电脉冲星的第一手观测资料，包括空间分布，传播特性，时间特性，脉冲轮廓与偏振以及频谱特性等，并详细综述观测资料对我们提供的信息及给我们的启示，为理论模型的建立和检验提供了基础。     

依据GPS数据研究伽师及帕米尔东北侧1994～1998年地壳水平运动及其与强震群的关系

利用伽师强震群区及帕米尔东北侧地区 1994～ 1998年的GPS监测成果 ,用DDA方法模拟了伽师强震群前后该地区地壳运动和应力应变的变化过程。结果表明 :在此期间伽师地区的应变以南北向挤压为主 ,伽师附近最大主应变变化达到 5× 10 - 8/a ,最大剪应变变化也超过 2 .5×10 - 8/a ,明显高于周边地区。伽师强震群的发生与GPS监测成果反映的该地区地壳运动和应力应变的变化存在明显的对应关系。GPS监测成果反映出在伽师地区有一应力应变变化的集中区域。通过在伽师强震群震中分布块体中强行沿其最大剪应力方向 (NE)增加一新的破裂 ,可使该块体应力应变下降至与周围块体相均衡 ,且能量可能沿柯坪断裂向东北方向传递。新增断裂的运动呈左旋 ,并导致其所在块体呈右旋运动     

伊利石40Ar-39Ar年龄的统计分析与成藏期

为了确定鄂尔多斯盆地苏里格气田的成藏年代,通过提取砂岩储层中的黏土质填隙物,分离分级成 < 0.5、0.5~1.0、1.0~2.0μm的分样品,进行伊利石激光阶段加热40Ar-39Ar定年.等时线年龄是自生伊利石与碎屑伊利石的混合年龄.通过趋势分析和回归分析分别获得极小的趋势年龄和极小的回归年龄,该年龄比较接近自生伊利石年龄.测试结果表明,伊利石的等时线年龄介于160.9~232.0 Ma之间,为自生伊利石与碎屑伊利石的混合年龄.采用数理统计方法获得极小趋势年龄和极小回归年龄分别为151.7 Ma和152.4 Ma,该年龄比较接近自生伊利石年龄,代表了热流体活动和油气成藏时间.      

Quantitative monitoring of gravity erosion using a novel 3D surface measuring technique: validation and case study

Natural Hazards - Gravity erosion is one of the most remarkable natural hazards in mountainous regions, especially on the Loess Plateau of China. Nevertheless, the measurement of failure mass is...     

基于3S技术的土地利用信息动态变更调查新机制研究——以成都市为例

新形势下的土地变更调查任务不断增加,要求不断提高,手段不断强化,时间紧、任务重是当前土地变更调查面临的重大问题。针对以上问题,本文提出了一种动态变更的技术流程,通过深入研究土地规划实施、土地综合整治、地籍管理、耕地保护、执法监察等业务及相关关系,围绕"及时发现、快速调查、持续更新、如实上报、共享应用"5个方面的问题,以3S技术、网络技术、数据库技术等为支撑,提出以二调成果为基础,从土地管理业务内部及时发现变化,以发现驱动土地利用信息日常性持续动态变更的新思路。以成都市为例,开展基于3S技术的土地利用信息动态变更调查的方法在实际工作中的应用研究,实现了土地利用信息的"一图多用",并对变更结果进行了分析。