基于准地转垂直运动方程对Q矢量的进一步探讨   总被引：1，自引：0，他引：1       下载免费PDF全文

周小刚  柳士俊  王秀明  陶祖钰 《地球物理学报》2011,54(10):2495-2502

Q矢量是诊断大气大尺度垂直运动的重要物理量.在f平面近似下,从原始运动方程组出发可以推导出Q矢量以及相关的半地转Q矢量、非地转Q矢量和湿Q矢量等表达式,但这种传统的推导方法没有考虑大气准地转运动的属性.本文利用数学物理变换,直接从准地转ω方程出发推导出Q矢量及其相关表达式,从而克服了传统方法在大气准地转运动属性表达方面...  相似文献   

A local geoid determination based on ellipsoid approximation in Western China     

Essam Ghanem  LI Jiancheng 《地球空间信息科学学报》2013,16(3):6-10

A new methodology for precise geoid determination with finest local details based on ellipsoidal approximation is presented. This methodology is formulated through the “fixed-free two-boundary value problem” based on the observable of the type modulus of gravity intensity, gravity acceleration and gravity potential at the GPS positioned stations, with support of the known geoid's potential value, W0.  相似文献   

Complete Eulerian-mean tracer equation for coarse resolution OGCMs     

M. S. Dubovikov  V. M. Canuto 《地球物理与天体物理流体动力学》2013,107(3):197-214

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针对深层流体识别的两项弹性阻抗反演与Russell流体因子直接估算方法研究   总被引：5，自引：5，他引：0       下载免费PDF全文

印兴耀  张世鑫  张峰 《地球物理学报》2013,56(7):2378-2390

Russell流体因子是判识深层储层含流体特征的敏感指示参数.针对深层地震资料缺失大角度入射信息以及信噪比普遍较低的特点,开展了基于贝叶斯理论框架的两项弹性阻抗反演与Russell流体因子直接估算方法研究.首先,在饱和孔隙弹性介质理论的指导下,推导了包含Russell流体因子和纵波阻抗参数的两项反射系数近似公式,并且进一步得到了新的两项弹性阻抗方程.其次通过模型的近似精度分析,验证了新弹性阻抗方程满足小角度近似精度要求.最后提出了贝叶斯弹性阻抗反演和Russell流体因子的直接估算方法,通过模型试算表明直接估算方法不仅充分利用了弹性阻抗反演的高抗噪性与实用性,并且有效的避免了间接累计误差对流体因子计算精度的影响,实际应用则进一步验证了直接估算的Russell流体因子可以提高深层储层流体识别的可靠性.  相似文献   

Conservative identification of nodal transmissivities: theory,computational experiments and application to the Rharb coastal aquifer (Morocco)     

B. EL MANSOURI  Y. LOUKILI  D. ESSELAOUI 《水文科学杂志》2013,58(3):377-389

Abstract

In order to calculate the transmissivity from the inverse problem corresponding to the groundwater flow in an isotropic horizontal aquifer, a numerical conservative approach is tested. The method deals with triangulation of the domain and applies the conservation of mass to elements of the mesh using the harmonic mean for internodal transmissivities. An optimal sweeping algorithm is used to evaluate nodal transmissivities from one element to another with a minimal relative error accumulation. The practical importance of the method is demonstrated through two synthetic examples representing those experienced in the field, then through application to a Moroccan aquifer. The computed hydraulic head is well fitted to the reference one, which confirms the validity of the identified transmissivity model.  相似文献   

Magnetic buoyancy instabilities incorporating rotation     

D. W. Hughes 《地球物理与天体物理流体动力学》2013,107(1-4):99-142

Abstract

Recent calculations suggest that the bulk of the solar toroidal field may be stored in a thin, convectively stable region situated between the convection zone proper and the radiative zone. Determining the stability properties of such a field is therefore important with implications for both the generation and escape of magnetic flux. The plane layer, linear stability analysis of Hughes (1985) is extended to incorporate the effects of uniform rotation. Detailed studies are made of interchange, or “axisymmetric” modes and of undular, or wavelike, motions, considering modes of both low and high frequency. The force due to rotation acts to constrain the fluid motions, a feature which is strongly stabilizing for direct modes, but can, in certain circumstances, be destabilizing for oscillatory motions.

For the interchange modes we show that the instability discussed at length by Hughes (1985), driven by fields increasing with height, is still present and indeed may be enhanced by rotational effects. We also study the more conventional instabilities, discussing the transformation between direct and oscillatory modes and considering in detail some peculiar properties of the oscillatory instabilities.

The more relevant instabilities in an astrophysical context are likely to be undular modes. Previous studies of low frequency modes driven by top heavy field gradients are extended to consider modes of various frequencies for a wide range of parameter values. Of particular interest is the occurrence of two distinct modes of instability for bottom heavy field gradients. We also exhibit some of the peculiar stability boundaries which can result when none of the competing influences in the problem is dominant.  相似文献   

OJ287双黑洞轨道计算:3.5阶后牛顿近似     

武曙光  张杨  付正文 《天文学报》2012,53(3):185-196

大质量双黑洞OJ287是一个强引力辐射源.为了探测其引力波信号,需要知道波形,而这主要是由轨道运动所决定.为此,从广义相对论3.5阶后牛顿近似的运动方程出发对OJ287的轨道进行仔细研究,取大黑洞位置固定作为近似,给出了后牛顿近似下3.5阶的次黑洞轨道解,比他人2.5阶的工作高了一阶.次黑洞撞击吸积盘面到光学爆发存在时间延迟,这对于确定轨道参数有很大影响.利用径向距离与爆发时间关系的线性模型,对最近7次爆发时刻的观测值拟合,给出了更精确的OJ287双黑洞的轨道参数及其运动轨道.分析了计算结果,研究运动特征,并且发现了两个新性质:次黑洞进动在初期增加,在晚期接近并和时,进动达到最大值,然后减小并越过0而趋于负值.尚不能确定晚期的这个行为是否由3.5阶近似不够准确所造成.运动方程中耗散性的辐射项,后牛顿2.5阶和3.5阶的系数具有相反的符号.这意味着3.5阶项反而是从外界吸收能量.但2.5阶与3.5阶之和仍然是向外辐射引力波的,体系能量变化率为负.这个工作的计算结果可以用来更精确地计算OJ287的引力辐射.  相似文献   

Born序列频散方程和Born-Kirchhoff传播算子   总被引：2，自引：0，他引：2       下载免费PDF全文

符力耘 《地球物理学报》2010,53(2):370-384

传统的Kirchhoff传播算子结构简洁,适用于描述横向均匀介质中波的传播.Ray-Kirchhoff传播算子较为精确地描述了波在非均匀介质中传播的运动学特征,其理论上的先天不足依赖于介质的复杂性.本文通过Born序列逼近波在非均匀介质中传播的大角度波分量,提出一种Born-Kirchhoff传播算子,将传统Kirchhoff传播算子的适用范围扩展至非均匀介质,同时描述波的运动学和动力学特征,其精度取决于Born序列逼近的阶数.利用Born序列频散方程,可以精确分析各阶Born-Kirchhoff传播算子对波长、传播角和非均质性的尺度依赖特征,其中,一阶Born-Kirchhoff传播算子的精度高于传统的相屏传播算子.波数域的Born-Kirchhoff传播算子对于高波数波是奇异的,导致波数域数值计算发散,但其空间域版本是非奇异的,无条件数值稳定,可通过Kirchhoff求和数值实施.本文给出各阶Born-Kirchhoff传播算子及其频散方程,可用于不同程度非均匀介质中的波传播模拟,复杂构造地震成像和速度估计.本文利用零阶和一阶Born-Kirchhoff传播算子计算简单二维模型的合成地震图,并与边界元法进行了比较.  相似文献   

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赵刚  张思慧  张恒璟  黄声和  叶国凤 《大地测量与地球动力学》2013,33(5):136-139

?????????IGS???????вο??????????仯???????仯????????????????????????????仯??????RBF?????????缰С??????????????????MATLAB7.0????????IGS???????????????GRNN?????????С??????????????????????????????????????????????????????д??????仯????????????????????????????仯?????????????????????  相似文献   

基于散乱数据的球面自然样条插值法     

王丽丽  徐应祥 《成都信息工程学院学报》2012,27(5):520-524

针对球面散乱数据插值问题,结合三元多项式自然样条方法的基本原理,提出一种新的逼近球面上散乱数据的自然样条插值方法,利用新的方法对给定区域内的三元函数进行数值逼近实验。将数值实验误差与理论误差对比(5%),结果验证了这种方法在球面散乱数据逼近问题上能够有效的使最大误差控制在2%以内。研究结果表明,这是一种比较有效的球面散乱数据逼近方法。  相似文献