坐标转换参数的求解方法及其应用

根据坐标转换参数的解算模型,介绍几种常见的坐标转换参数的求解方法及其参数个数与精度;探讨选择坐标转换参数的条件及转换参数的应用,从而阐明转换参数对GPS技术的推广和全球资料的统一的重要作用。     

基于Harris算子的遥感影像自适应特征提取方法

提出一种基于Harris算子的遥感影像自适应特征点信息提取新方法。在进行特征点自动提取时,该方法通过设计一种自适应的迭代策略,实现了特征点阈值的自动确定。在兼顾局部纹理信息的基础上,通过对影像预先的分块处理和邻近点剔除,保证了特征点在全幅影像中的均匀分布。杭州地区TM影像特征点的提取试验表明,该方法自动化程度高,提取的特征点分布均匀合理,能满足几何配准和几何纠正精度要求,具有较高的实用价值。     

Textural and mineralogical evidence for a Cadomian tectonothermal event in the eastern Mediterranean (Sandıklı-Afyon area, western Taurides, Turkey)

In the Sandıklı-Afyon area, the very low-grade metamorphic Sandıklı Basement Complex with clastic sediments and Late Neoproterozoic felsic igneous rocks are unconformably overlain by a cover succession with red continental clastic rocks, tholeiitic basalts and siliciclastic rocks with Early Cambrian trace fossils. Illite crystallinity studies reveal that both the basement and cover units were metamorphosed at high anchizonal to epizonal conditions ( 300 °C). Textural data together with the detailed evaluation of the P–T–b₀ grid, however, indicate that this thermal event has multiple phases. The first tectonothermal event was realized at pressures of  4.2 kb on the basis of b₀-data and resulted in development of blastomylonites. This is supported by the presence of dynamo-metamorphosed pebbles within the basal conglomerates of the Lower Paleozoic cover series. The second event is post-Ordovician–pre-Jurassic in age, occurred at lower pressures  3.2 kb and produced a weakly developed cleavage in the siliciclastic rocks of the cover. The mineralogical/textural data across the basement-cover boundary therefore indicate the removal of an entire metamorphic zone and thus a metamorphic hiatus.

These data suggest that the Taurides were affected by a Late Neoproterozoic event as part of the peri-Gondwana during the Cadomian orogeny.     

基于约束点的无拓扑多边形数据压缩算法

分析了常规压缩算法(如Douglas-Peucker算法)压缩无拓扑多边形数据会产生公共边界不一致现象,认为出现此现象的原因是多边形公共边界的压缩起始点选择不一致,进而提出了一种新的基于约束点的无拓扑多边形数据压缩算法。算法原理包括:首先将多边形公共边界的两个端点作为约束点处理,使得多边形从约束点处逻辑上分成几段;然后利用常规压缩算法进行分段压缩,使每一多边形公共边界的压缩初始点一致,从而保证了无拓扑多边形数据的一致性压缩;最后大量试验验证了此算法的有效性。     

A VLBI Delay Model for Radio Sources at a Finite Distance

A relativistic delay model for Earth-based very long baseline interferometry (VLBI) observation of sources at finite distances is derived. The model directly provides the VLBI delay in the scale of terrestrial time. The effect of the curved wave front is represented by using a pseudo source vector K = (R ₁ + R ₂)/(R ₁ + R ₂), and the variation of the baseline vector due to the difference of arrival time is taken into account up to the second-order by using Halley’s method. The precision of the new VLBI delay model is 1 ps for all radio sources above 100 km altitude from the Earth’s surface in Earth-based VLBI observation. Simple correction terms (parallax effect) are obtained, which can also adopt the consensus model (e.g. International Earth Rotation and Reference Frames Service conventions) to finite-distance radio source at R > 10 pc with the same precision. The new model may enable estimation of distance to the radio source directly with VLBI delay data.     

测高数据处理中网格化问题的探讨

本文从卫星测高数据处理中网距的选取、数据点的图形结构、网格算子等三个方面加以讨论,提出了频域中数据网格化的方法,最后利用两个周期的Topex/Poseidon卫星测高数据进行计算分析,得出了一些卫星测高数据网格化的经验。     

Neutral Points at the Cometary Diamagnetic Cavity Boundary as Possible Source of Cometary Rays

The point source of neutral gas undergoing ionization and expanding into an uniform magnetic field is considered. Friction between the neutral and ionized particles results in the formation of the magnetic field barrier and diamagnetic cavity surrounding the source. At least one neutral point inevitably arises at the boundary of the cavity. When the neutral gas production rate grows, two neutral points may arise at this boundary. In the vicinity of these points magnetic field lines converge, along with the plasma flow which is magnetic field aligned in the steady state. As a result, two plasma jets originate from the neutral points. Possible relation of these jets to cometary rays is discussed. This revised version was published online in July 2006 with corrections to the Cover Date.     

Nonlinear Stability of the Lagrangian Libration Points in the Chermnykh Problem

In this paper we consider the problem of motion of an infinitesimal point mass in the gravity field of an uniformly rotating dumb-bell. The aim of our study is to investigate Liapunov stability of Lagrangian libration points of this problem. We analyze the stability of libration points in the whole range of parameters ω, μ of the problem. In particular, we consider all resonance cases when the order of resonance is not greater than five. This revised version was published online in August 2006 with corrections to the Cover Date.     

基于拟Fejer点上的复插值算子的一致逼近阶

设Ｄ是复平面上的Ｊｏｒｄａｎ区域，其边界Γ∈Ｃ￣（１＋δ）。本文得到了一类在拟Ｆｅｊｅｒ点上插值的复插值算子Γ在上一致收敛于ｆ（ｚ）∈Ｃ（Γ）的逼近阶。     

The structure of chaos in a potential without escapes

We study the structure of chaos in a simple Hamiltonian system that does no have an escape energy. This system has 5 main periodic orbits that are represented on the surface of section by the points (1)O(0,0), (2)C ₁,C ₂(±y _c, 0), (3)B ₁,B ₂(O,±1) and (4) the boundary . The periodic orbits (1) and (4) have infinite transitions from stability (S) to instability (U) and vice-versa; the transition values of are given by simple approximate formulae. At every transitionS U a set of 4 asymptotic curves is formed atO. For larger the size and the oscillations of these curves grow until they destroy the closed invariant curves that surroundO, and they intersect the asymptotic curves of the orbitsC ₁,C ₂ at infinite heteroclinic points. At every transitionU S these asymptotic curves are duplicated and they start at two unstable invariant points bifurcating fromO. At the transition itself the asymptotic curves fromO are tangent to each other. The areas of the lobes fromO increase with ; these lobes increase even afterO becomes stable again. The asymptotic curves of the unstable periodic orbits follow certain rules. Whenever there are heteroclinic points the asymptotic curves of one unstable orbit approach the asymptotic curves of another unstable orbit in a definite way. Finally we study the tangencies and the spirals formed by the asymptotic curves of the orbitsB ₁,B ₂. We find indications that the number of spiral rotations tends to infinity as . Therefore new tangencies between the asymptotic curves appear for arbitrarily large . As a consequence there are infinite new families of stable periodic orbits that appear for arbitrarily large .