网络地图问题及其解决方案     

石云  刘万青 《测绘与空间地理信息》2007,30(1):48-50

网络地图或网上地图是指在因特网上浏览、制作和使用的地图,越来越多的人从网络上获取地图和相关信息,但是,它在方便大众的同时也存在很多问题,文章分析和总结了当前网络地图的主要特点和存在的问题,并在此基础上,讨论网络地图相关问题的解决方案以及可以采取的措施。  相似文献   

单纯形—模拟退火混合算法反求水文地质参数及其并行求解   总被引：6，自引：0，他引：6       下载免费PDF全文

江思珉  朱国荣  胡西嘉  季月华 《地质论评》2007,53(1)

本文利用单纯形法局部搜索速度快和模拟退火算法全局寻优的特点,同时为了克服各自算法的弊病,提出采用单纯形—模拟退火混合算法(SMSA)进行水文地质逆问题的求解。论文详细描述了SMSA算法的具体操作算子的实现,并将该算法应用于一个大型水源地的地下水模拟反演。计算结果表明,SMSA算法在水文地质参数反演计算具有求解速度快,精度高的特点,而且易于实现并行运算。  相似文献   

单纯形一模拟退火混合算法反求水文地质参数及其并行求解          下载免费PDF全文

江思珉朱国荣  胡西嘉季月华 《地质论评》2007,53(1):92-97

本文利用单纯形法局部搜索速度快和模拟退火算法全局寻优的特点，同时为了克服各自算法的弊病，提出采用单纯形一模拟退火混合算法（SMSA）进行水文地质逆问题的求解。论文详细描述了SMSA算法的具体操作算子的实现，并将该算法应用于一个大型水源地的地下水模拟反演。计算结果表明，SMSA算法在水文地质参数反演计算具有求解速度快，精度高的特点，而且易于实现并行运算。  相似文献   

深部找矿与蒋氏TEM双定源回线装置方案     

蒋邦远 《物探化探计算技术》2007,(Z1)

双定源回线装置的水平场Hx,其强度大、均匀,有利于探测深部陡倾斜金属矿藏,并可用作远距离井中测量的场源。此方案可用于危机矿山的找矿工作。  相似文献   

河道洪水反流向演算过程迭代方法   总被引：3，自引：1，他引：3  

钟平安  张慧  邴建平  刘伟莉 《水文》2007,27(2):37-39

在流域防洪调度中需要考虑河槽的调蓄作用,河道洪水反流向演算可以简化河库联合调度模型的求解;马斯京根法是河道洪水演算的常用方法,但不能直接用于解决洪水反流向演算问题;提出了马斯京根法和迭代试算相结合的过程迭代算法;实例表明方法是实用有效的。  相似文献   

A level-set corrector to an adaptive multiscale permeability prediction     

Inga Berre  Martha Lien  Trond Mannseth 《Computational Geosciences》2007,11(1):27-42

We consider the inverse problem of permeability estimation for two-phase porous-media flow. The novel approach is based on regularization by zonation, where the geometry and size of the regions are chosen adaptively during the optimization procedure. To achieve this, we have utilized level-set functions to represent the permeability. The available data are sparsely distributed in space; hence, it is reasonable to confine the estimation to coarse-scale structures. The level-set approach is able to alter the boundaries between regions of different permeability without strict restrictions on their shape; however, when the data are sparse, a reasonable initial guess for the permeability is required. For this task, we use adaptive multiscale permeability estimation, which has the potential of identifying main permeability variations. These are described by a piecewise constant function, where the constant values are attained on rectangular zones. In the current work, we develop a level-set corrector strategy, assuming adaptive multiscale permeability estimation as a predictor.  相似文献   

The Restricted Hill Four-Body Problem with Applications to the Earth–Moon–Sun System     

D. J. Scheeres 《Celestial Mechanics and Dynamical Astronomy》1998,70(2):75-98

Starting from the four-body problem a generalization of both the restricted three-body problem and the Hill three-body problem is derived. The model is time periodic and contains two parameters: the mass ratio ν of the restricted three-body problem and the period parameter m of the Hill Variation orbit. In the proper coordinate frames the restricted three-body problem is recovered as m → 0 and the classical Hill three-body problem is recovered as ν → 0. This model also predicts motions described by earlier researchers using specific models of the Earth–Moon–Sun system. An application of the current model to the motion of a spacecraft in the Sun perturbed Earth–Moon system is made using Hill's Variation orbit for the motion of the Earth–Moon system. The model is general enough to apply to the motion of an infinitesimal mass under the influence of any two primaries which orbit a larger mass. Using the model, numerical investigations of the structure of motions around the geometric position of the triangular Lagrange points are performed. Values of the parameter ν range in the neighborhood of the Earth–Moon value as the parameter m increases from 0 to 0.195 at which point the Hill Variation orbit becomes unstable. Two families of planar periodic orbits are studied in detail as the parameters m and ν vary. These families contain stable and unstable members in the plane and all have the out-of-plane stability. The stable and unstable manifolds of the unstable periodic orbits are computed and found to be trapped in a geometric area of phase space over long periods of time for ranges of the parameter values including the Earth–Moon–Sun system. This model is derived from the general four-body problem by rigorous application of the Hill and restricted approximations. The validity of the Hill approximation is discussed in light of the actual geometry of the Earth–Moon–Sun system. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Isolated Periodic Orbits and Stability in Separable Potentials     

E. Meletlidou  S. Ichtiaroglou 《Celestial Mechanics and Dynamical Astronomy》1998,71(4):289-300

A method for determining the main families of isolated periodic orbits and their characteristic exponents in planar potentials which are separated by a point transformation is proposed. Since these orbits are continued analytically with the same stability, these results are persistent under small perturbations. The method is applied to the two fixed centers problem, the Paul trap and the dipole expansion of an electrostatic potential. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Mass-Weighted Symplectic Forms for the N-Body Problem     

F. Varadi  M. Ghil  W. M. Kaula 《Celestial Mechanics and Dynamical Astronomy》1998,72(3):187-199

Mass-weighted symplectic forms provide a unified framework for the treatment of both finite and vanishingly small masses in the N-body problem. These forms are introduced, compared to previous approaches, and their properties are discussed. Applications to symplectic mappings, the definition of action-angle variables for the Kepler problem, and Hamiltonian perturbation theory are outlined This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

EJECTION–COLLISION ORBITS AND INVARIANT PUNCTURED TORI IN A RESTRICTED FOUR‐BODY PROBLEM     

Dante L. Maranhão  Jaume Llibre 《Celestial Mechanics and Dynamical Astronomy》1998,71(1):1-14

We study the motion of an infinitesimal mass point under the gravitational action of three mass points of masses μ, 1–2μ and μ moving under Newton's gravitational law in circular periodic orbits around their center of masses. The three point masses form at any time a collinear central configuration. The body of mass 1–2μ is located at the center of mass. The paper has two main goals. First, to prove the existence of four transversal ejection–collision orbits, and second to show the existence of an uncountable number of invariant punctured tori. Both results are for a given large value of the Jacobi constant and for an arbitrary value of the mass parameter 0<μ≤1/2. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献