珠江河网分形机理研究   总被引：3，自引：0，他引：3  

王世俊  黄胜伟  王华  罗杰 《热带地理》2007,27(2):111-115

以不同时期珠江网河历史地图及遥感影像为基础,进行了河网分形计算,并从河道发育、人为活动等多个角度分析了珠江网河分形机理。在发育过程中,1883-2001年间河网分维值逐渐减小;在空间上,正干水道中潮道分维值大于分汊河道。分析认为,人为活动是导致珠江网河分形变化的主要因素:联围筑闸消灭横向支汊、口门整治及河道固化减小了河道冲决的几率、河道挖沙引起的水沙分流比变化改变了河道冲淤特性。  相似文献   

河口挡潮闸对三角洲潮汐不对称时空变化的影响     

沈倩颖  季小梅  张蔚  徐龑文 《热带海洋学报》2021,40(5):1-9

三角洲内部潮汐不对称性与三角洲地貌演变方向有重要关系。目前诸多研究关注海洋、陆地边界的改变对三角洲内的潮汐不对称性演变规律的影响。实际上, 大规模的河口工程也会对三角洲内的潮汐不对称性产生影响。在众多河口工程中, 河口挡潮闸由于直接削弱口门处海洋潮动力, 影响最为直接。荷兰三角洲是潮动力主导型三角洲, 受洪潮灾害影响较为严重, 为此在荷兰西南部修建了世界上著名的三角洲挡潮闸工程。文章以荷兰莱茵河-默兹河三角洲为研究对象, 分析以挡潮闸为主的河口工程对三角洲内河网潮汐不对称性演变特征的影响。选取莱茵河-默兹河三角洲13个潮位站点的50~60年的水文资料, 利用非平稳调和分析方法计算分析三角洲内部潮汐传播特性, 并进一步研究潮汐涨落潮历时不对称性演变特征, 揭示河口挡潮闸工程对潮汐河网中潮汐动力和潮汐不对称性的影响。研究表明, 莱茵河-默兹河三角洲为显著的涨潮占优型河口, 潮汐不对称现象总体向上游沿程增强。河口挡潮闸修建后受河网径流量和潮动力剧烈变化的影响, 封闭的南部通道内的潮波大幅度削弱, 潮汐不对称现象在下游增强在上游减弱。北部、中部通道其他站点则因为通道径流增大, 潮汐不对称现象增强, 中部站点变化更为显著。  相似文献   

胶州湾口海底沙波的类型、特征及发育影响因素   总被引：4，自引：1，他引：3  

边淑华  夏东兴  陈义兰  赵月霞 《中国海洋大学学报(自然科学版)》2006,36(2):327-330

采用多波束资料对胶州湾口的海底沙波类型、特征进行了研究,发现研究区主要有线性沙波(二维)、沙丘(三维)2种沙波类型。结合水流流速、海底构造和表层沉积物综合分析发现:海底沙波缓坡朝向与优势流向不完全一致,为强流作用的产物,在涨、落潮作用下均可形成;沉积物的多寡是研究区海底沙波类型分布的决定因素,海底松散沉积物较为丰富的地区形成二维沙波。在水动力强大的胶州湾口,沉积物多分布在构造低洼地带,使二维线性沙波的分布与海底断裂延伸方向一致。  相似文献   

Proton and He^2＋ Temperature Anisotropies in the Solar Wind Driven by Ion Cyclotron Waves     

Quan-Ming Lu  Shui Wang School of Earth  Space Sciences  University of Science  Technology of China  Hefei   《中国天文和天体物理学报》2005,5(2):184-192

We carried out one-dimensional hybrid simulations of resonant scattering of protons and He^2 ions by ion cyclotron waves in an initially homogeneous, collisionless and magnetized plasma. The initial ion cyclotron waves have a power spectrum and propagate both outward and inward. Due to the resonant interaction with the protons and He^2 ions, the wave power will be depleted in the resonance region. Both the protons and He^2 ions can be resonantly heated in the direction perpendicular to the ambient magnetic field and leading to anisotropic velocity distributions, with the anisotropy higher for the He^2 ions than for the protons. At the same time, the anisotropies of the protons and He^2 ions are inversely correlated with the plasma β‖p=8πnpkBT‖p/B0^2, consistent with the prediction of the quasilinear theory (QLT).  相似文献   

Surface waves across 2-D structures: a method based on coupled local modes     

V. Maupin 《Geophysical Journal International》1988,93(1):173-185

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Near-infrared imaging of H2 in molecular outflows from young stars     

C. J. Davis  R. Mundt  J. Eislöffel 《Astrophysics and Space Science》1995,224(1-2):121-124

In an attempt to identify the molecular shocks associated with the entrainment of ambient gas by collimated stellar winds from young stars, we have imaged a number of known molecular outflows in H₂ v=1-0 S(1) and wide-band K. In each flow, the observed H₂ features are closely associated with peaks in the CO outflow maps. We therefore suggest that the H₂ results from shocks associated with the acceleration or entrainment of ambient, molecular gas. This molecular material may be accelerated either in a bow shock at the head of the flow, or along the length of the flow through a turbulent mixing layer.  相似文献   

Internal shocks in a relativistic wind as a source for gamma-ray bursts?     

R. Mochkovitch  V. Maitia  R. Marques 《Astrophysics and Space Science》1995,231(1-2):441-444

We investigate the recent proposal made by Rees and Mészáros (1994) that GRBs result from internal shocks in the relativistic wind emerging from two coalesced neutron stars. Using a simple model of that wind, where a large number of layers with different Lorentz factors interact through a series of mildly relativistic shocks we compute the efficiency of the process and the time profile of the resulting burst. We show that a great variety of profiles can be obtained using plausible initial distributions of Lorentz factors in the wind. However, the rather low overall efficiency (< 10%) of the process and limits imposed on the burst duration can be used to put severe constraints on the nature of the energy source.  相似文献   

Phase-space mixing and the merging of cusps     

Walter Dehnen 《Monthly notices of the Royal Astronomical Society》2005,360(3):892-900

Collisionless stellar systems are driven towards equilibrium by mixing of phase-space elements. I show that the excess-mass function     [where     is the coarse-grained distribution function] always decreases on mixing . D ( f ) gives the excess mass from values of     . This novel form of the mixing theorem extends the maximum phase-space density argument to all values of f . The excess-mass function can be computed from N -body simulations and is additive: the excess mass of a combination of non-overlapping systems is the sum of their individual D ( f ). I propose a novel interpretation for the coarse-grained distribution function, which avoids conceptual problems with the mixing theorem.
As an example application, I show that for self-gravitating cusps (  ρ∝ r ^−γ  as   r → 0  ) the excess mass   D ∝ f ^{−2(3−γ)/(6−γ)}  as   f →∞  , i.e. steeper cusps are less mixed than shallower ones, independent of the shape of surfaces of constant density or details of the distribution function (e.g. anisotropy). This property, together with the additivity of D ( f ) and the mixing theorem, implies that a merger remnant cannot have a cusp steeper than the steepest of its progenitors. Furthermore, I argue that the cusp of the remnant should not be shallower either, implying that the steepest cusp always survives.  相似文献   

Nonlinear wave-wave interactions and wedge waves     

RayQ.Lin WillPerrie 《中国海洋湖沼学报》2005,23(2):129-143

A tetrad mechanism for exciting long waves, for example edge waves, is described based on nonlinear resonant wave-wave interactions. In this mechanism, resonant interactions pass energy to an edge wave,from the three participating gravity waves. The estimated action flux into the edge wave can be orders of magnitude greater than the transfer fluxes derived from other competing mechanisms, such as triad interactions. Moreover, the numerical results show that the actual transfer rates into the edge wave from the three participating gravity waves are two- to three- orders of magnitude greater than bottom friction.  相似文献   

重庆辐射雾的声雷达回波与大气污染特征     

但尚铭  陈国学 《成都信息工程学院学报》1996,(4)

结合气象观测和大气边界层探测资料，分析了１９９０年１月２日重庆雾的声雷达回波特征，并与１９８９年１２月３０日雾的回波作了比较。结果表明，雾顶回波高度与逆温和相对湿度的转折高度一致；雾顶回波在雾的成熟期呈现波动，在消散期有一下降过程。上午大气污染物地面浓度的变化与逆温混合层状况有密切关系，混合层较薄且持续时间较长时，地面浓度较大  相似文献