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171.
Mehdi Eshagh Morteza Ghorbannia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The orbital elements of a low Earth orbiting satellite and their velocities can be used for local determination of gravity anomaly. The important issue is to find direct relations among the anomalies and these parameters. Here, a primary theoretical study is presented for this purpose. The Gaussian equations of motion of a satellite are used to develop integral formulas for recovering the gravity anomalies. The behaviour of kernels of the integrals are investigated for a two-month simulated orbit similar to that of the Gravity field and steady-state ocean circulation explorer (GOCE) mission over Fennoscandia. Numerical investigations show that the integral formulas have neither isotropic nor well-behaved kernels. In such a case, gravity anomaly recovery is not successful due to large spatial truncation error of the integral formulas. Reformulation of the problem by combining the orbital elements and their velocities leads to an integral with a well-behaved kernel which is suitable for our purpose. Also based on these combinations some general relations among the orbital elements and their velocities are obtained which can be used for validation of orbital parameters and their velocities. 相似文献
172.
对电传操纵系统驾驶员诱发振荡(PIO)的现象进行了分析,指出了舵回路速率饱和是造成PIO的主要原因,并有针对对给出了一种非常规的用于解决饱和非线性问题的程序控制方法。这种方法主要是通过舵回路反馈的状态信息来改变驾驶杆输入信号的放大系数,从而达到有效抑制PIO的目的,同时用Hurwitz稳定判据进行了机理分析,最后给出了仿真验证结果,证明该方法是简单而有效的。 相似文献
173.
This contribution describes the formation of circumstellar disks and their earliest evolutionary phases when self-gravity
in the disk plays a crucial role in eliciting the transport of mass and angular momentum. We first discuss the formation of
protostellar disks within the context of analytic infall-collapse solutions. We then discuss our efforts to understand the
behavior of the newly formed disks. Our specific approach consists of performing a detailed analysis of a simplified model
disk which is susceptible to the growth of a spiral instability. Using a combination of numerical simulation and semi-analytic
analysis, we show how the dramatic early phase of mass and angular momentum transport in the disk can be explained by a second-order
nonlinear process involving self-interaction of a dominant two-armed spiral mode.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
174.
This paper studies a nonlinear robust control algorithm of the electro-hydraulic load simulator (EHLS). The tracking performance of the EHLS is mainly limited by the actuator's motion disturbance, flow nonlinearity, and friction, etc. The developed controller is developed based on the nonlinear motion loading model. The problems of the actuator's disturbance and flow nonlinearity are considered. To address the friction problem, the friction model of the loading motor is identified experimentally. The friction disturbance is compensated using the obtained friction model. Therefore, this paper considers the main three factors comprehensively. The developed algorithm is easy to apply since the controller can be obtained just with one step back-stepping design. The stability of the developed algorithm is proven via Lyapunov analysis. Both co-simulation and experiments are performed to verify the effectiveness of this method. 相似文献
175.
176.
Periodic relative orbits of two spacecraft subject to differential gravity and electrostatic forcing
Coulomb forces between charged close-flying satellites can be used for formation control, and constant electric potentials enable static equilibria solutions. In this work, open-loop time-varying potential functions, which produce periodic, two-craft, Coulomb formation motions are demonstrated for the first time. This is done in the rotating Hill-Frame, with linearized gravity, and craft position components assumed in the form of simple harmonic oscillators. Substitution of the oscillatory functions into the dynamics, further constrains these functions, and yields necessary potential histories, to produce the periodic flow. The assumed position functions, however, are not arbitrary, since the dynamical model restricts what oscillatory trajectories are allowed. Specifically, a Hill-Frame integral of motion is derived, and this is used to show certain candidate periodic functions to be inadmissible. The system dynamics are then linearized to expose stability properties of the solutions, and it is established that asymptotic stability is impossible for all orbit families. Finally, the degree of instability in the assumed motions, over free parameter ranges, is determined numerically via the Floquet multipliers of the associated full-cycle state-transition matrices. 相似文献
177.
本文对中层大气受迫Rossby波包的非线性三波相互作用问题作了进一步的数值分析,结果表明,三个波包随时间演化达到的平衡态与文献[1]的理论结果完全一致,而且仅当系统中只有中等波长波包不受外源强迫时,系统运动有可能出现两个稳定平衡态,在一定外源强度范围内,平衡态会产生尖点突变,平衡态随外源的变化有滞后分岔的特征,系统运动最终达到的平衡态不仅与外源强度的变化方式有关,而且依赖于初始状态。 相似文献
178.
主要探讨了实域上当g(x),h(x)是多基式,二阶变系数线性微分方程y″+g(x)y‘+h(x)y=0的可积性问题,沿袭了文」1「中算子矩阵理论的思想,得到了该方程要积的充分必要条件,且给出可积时的通解公式,并举例指出了文中「5,6」中收集的许多可积的二阶线性微分方程,其中相应的多项式系数的部分均是本文的特例。 相似文献
179.
Zhu Jiang Abimael F D Loula Laboratório Nacional de Computaco Científica MCT Av Getúlio Vargas Petrópolis RJ Brazil 《南京航空航天大学学报(英文版)》2001,18(Z1)
INTRODUCTIONThe stationary incompressible Navier- Stokesequations in the primitive variables( velocity uand pressure p)- vΔu + u . u + p =f . u =0u =g inΩinΩonΓ( 1 )whereΩ is a set of R2 ,Γ its boundary,v thekinematic viscosity of the fluid,f a field of givenbody forces,and g a given field defined onΓ sa-tisfying the global conservation property∫Γg . n =0 ( 2 )n denotes the unit outer normal vector toΓ.The vorticity- velocity system of Eq.( 1 ) ,byintroducing the vorticityω… 相似文献
180.