Practical spreading of driving forces for wave-driven currents     

Hyoseob Kim   《Ocean Engineering》2004,31(3-4):435-453

Profiles of wave-induced current on plane beaches are generally smooth. Previously, the smooth nature was often explained by involving lateral mixing concept. This paper describes a new spreading approach instead of the previous lateral mixing approach. The spreading of the driving forces leads to similar results on the velocity profiles of the previous approach. The results of the new method show good agreement with some laboratory measurements for a plane beach. The present method was then extended for two-dimensional plan problems. The present approach was tested against a laboratory experiment, and the computed flow field agrees reasonably well with the measured flow field. A merit of the present method is that the computational time increment is not restricted by the lateral mixing.  相似文献   

A B-spline-based method for radiation and diffraction problems     

Ranadev Datta  Debabrata Sen   《Ocean Engineering》2006,33(17-18):2240-2259

An open uniform B-spline-based panel method is developed for solution of potential flow problems. In this method, both geometry as well as the field variables are represented by the same open uniform B-spline basis function. The method is initially applied for the radiation problem in unbounded fluid. Computed results for a spheroid of different aspect ratio are found to be in excellent agreement with analytical results. The method is then applied for diffraction problem formulated based on the transient (time-domain) Green's function. Computed results for a hemisphere and Wigley hull are compared with published results and the comparison shows good agreement.  相似文献   

Wave radiation by a uniform cylinder in front of a vertical wall     

B. Teng  D. Z. Ning  X. T. Zhang 《Ocean Engineering》2004,31(2):201-224

In this paper, an exact analytical method is developed for the problem of wave radiation by a uniform cylinder in front of a vertical wall. Based on the image principle, the hydrodynamic problem of a cylinder in front of a vertical wall is transformed into the equivalent problem of double cylinders in unbounded fluid domain. Consequently, an analytical method of eigenfunction expansion is adopted to calculate the radiation of the cylinder due to the motion in surge, sway, roll and pitch, respectively. Moreover, numerical analysis has been carried out in detail in order to discuss the influences of the distance between the cylinder and the vertical wall and water depth on the added mass and radiation damping of the cylinder. It is shown that added mass and damping of the cylinder in front of a vertical wall are evidently different from those in case of the cylinder in unbounded fluid domain from the numerical results. It is also found that the added mass and radiation damping oscillate with wave number, and the oscillating frequency increases with the increasing of the distance between the cylinder and the wall.  相似文献   

Quasiintegrals of the photogravitational eccentric restricted three-body problem with Poynting–Robertson drag     

G. F. Chörny 《Celestial Mechanics and Dynamical Astronomy》2007,97(4):229-248

A restricted three-body problem for a dust particle, in presence of a spherical cometary nucleus in an eccentric (elliptic, parabolic or hyperbolic) orbit about the Sun, is considered. The force of radiation pressure and the Poynting– Robertson effect are taken into account. The differential equations of the particle’s non-inertial spatial motion are investigated both analytically and numerically. With the help of a complex representation, a new single equation of the motion is obtained. Conversion of the equations of motion system into a single equation allows the derivation of simple expressions similar to the integral of energy and integrals of areas. The derived expressions are named quasiintegrals. Relative values of terms of the energy quasiintegral for a smallest, largest, and a mean comet are calculated. We have found that in a number of cases the quasiintegrals are related to the regular integrals of motion, and discuss how the quasiintegrals may be applied to find some significant constraints on the motion of a body of infinitesimal mass.  相似文献   

Theoretical and Experimental Studies of Radiative Shocks     

C. Michaut  T. Vinci  L. Boireau  M. Koenig  S. Bouquet  A. Benuzzi-Mounaix  N. Osaki  G. Herpe  E. Falize  B. Loupias  S. Atzeni 《Astrophysics and Space Science》2007,307(1-3):159-164

This paper deals with the radiative shock from both theoretical and numerical points of view. It is based on the whole experimental results obtained at Laboratoire d'Utilisation des Lasers Intenses (LULI, école Polytechnique). Radiative shocks are high-Mach number shocks with a strong coupling between radiation and hydrodynamics which leads to a structure governed by a radiative precursor. These shocks are involved in various astrophysical systems: stellar accretion shocks, pulsating stars, interaction between supernovae and the interstellar medium. In laboratory, these radiative shocks are generated using high power lasers. New diagnostics have been implemented to study the geometrical shape of the shock and the front shock density. Data were obtained varying initial conditions for different laser intensities and temperature. The modeling of these phenomena is mainly performed through numerical simulations (1D and 2D) and analytical studies. We exhibit results obtained from several radiative hydrodynamics codes. As a result, it is possible to discuss about the influence of the geometry and physical parameters introduced in the 1D and 2D models.  相似文献   

New evidence for strong nonthermal effects in Tycho’s supernova remnant     

H. J. Völk  E. G. Berezhko  L. T. Ksenofontov 《Astrophysics and Space Science》2007,309(1-4):389-394

For the case of Tycho’s supernova remnant (SNR) we present the relation between the blast wave and contact discontinuity radii calculated within the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is demonstrated that these radii are confirmed by recently published Chandra measurements which show that the observed contact discontinuity radius is so close to the shock radius that it can only be explained by efficient CR acceleration which in turn makes the medium more compressible. Together with the recently determined new value E _sn=1.2×10⁵¹ erg of the SN explosion energy this also confirms our previous conclusion that a TeV γ-ray flux of (2–5)×10⁻¹³ erg/(cm² s) is to be expected from Tycho’s SNR. Chandra measurements and the HEGRA upper limit of the TeV γ-ray flux together limit the source distance d to 3.3≤d≤4 kpc.  相似文献   

2013和2012年夏季格陵兰岛冰盖表面融化对比及可能的影响机理分析     

陈志强  刘骥平  范广洲  胡永云 《大气科学》2015,39(4):757-766

本文重点分析了2013年夏季格陵兰冰盖表面的融化特征, 并将2013年与2012年融化极值年的异常进行对比, 探讨二者之间存在的动力和热力差异及其对冰盖表面融化的影响和机制。结果表明:2013年夏季格陵兰冰盖表面最大融化范围仅为44%, 远小于2012年的97%, 持续的时间也比2012年短20天左右, 平均的融化面积和持续时间都接近气候平均态。2013年夏季大气环流异常与2012年近乎完全相反, 格陵兰及附近海域为低压异常, 500 hPa位势高度场为负异常, 大气环流和2012年相比更具有纬向型。格陵兰岛的北部和南部出现气旋异常, 有利于输送北极的冷空气到格陵兰岛, 不仅降低了夏季格陵兰冰盖表面的平均温度, 而且也减少了格陵兰高温事件发生的频率。同时, 2013年夏季格陵兰表面向下的辐射通量异常分布大体上呈西南—东北走向, 不同于 2012年的南北分布。尽管从分布上看, 总的向下辐射通量以正的短波分量为主, 但是长短波分量相互抵消使得 2013年夏季总的向下辐射通量接近气候平均态, 这使得辐射对冰盖表面温度的影响不明显。大气环流的动力和表面辐射收支的热力共同作用导致2013年夏季格陵兰冰盖表面融化经历了相对缓和的一年。  相似文献   

Synchrotron emission model of gamma-ray pulsar PSR J2021+3651     

《New Astronomy》2015

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超强地震作用下深厚覆盖层场地重力坝抗震安全研究     

王伟  梁辉  范建朋  郭胜山 《震灾防御技术》2021,16(4):702-709

本文通过成层状地基地震动输入计算方法得到覆盖层边界自由场运动,采用粘弹性边界,考虑地基辐射阻尼效应及坝体和地基的接触非线性,针对强震区深厚覆盖层场地重力坝开展线性和非线性动力时程分析研究,结合需求能力比DCR评估其抗震性能。由线弹性动力时程分析可知,在运行基准地震OBE作用下,重力坝坝体应力均在允许范围内,其抗滑稳定安全系数不能满足要求;由非线性动力分析可知,在OBE和最大设计地震MDE作用下,重力坝发生较大滑动位移。通过在重力坝坝体下游坝后回填土加强重力坝抗震稳定性,结果表明,下游坝后回填土可有效减小坝体滑动位移,加强其抗震稳定性。本文针对深厚覆盖层场地重力坝开展的抗震安全研究为抗震设计提供了科学依据,为强震区深厚覆盖层场地重力坝的抗震分析提供参考。  相似文献   

切仑科夫线状辐射与类星体的宽发射线起源探讨     

刘当波  袁爱芳  孟宪茹  单增罗布  尤峻汉 《天文学报》2009,50(4)

当具有各向同性速度分布的相对论电子穿过稠密气体区,或者轰击稠密气体区的表面时,切仑科夫效应将会产生1种特殊的原子或离子发射线,称做切仑科夫线状发射.这一预言在光学波段已由实验室的实验所证实.研究指出了切仑科夫线状辐射在类星体和赛弗特1星系的宽发射线研究中的重要性,利用此新机制有可能解决类星体研究中的一些重大且长期没有解决的疑惑.例如宽氢线之间存在的反常强度比,特别是反常Lyα/Lyβ强度比的问题.并且进一步估计了相对论电子穿过宇宙气体时所产生的各种效应的能耗的数量级,并对各种能耗进行比较,证实了切仑科夫线状发射机制在类星体和塞弗特1型星系中的有效性.  相似文献