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111.
112.
舒姚涵 《民用飞机设计与研究》2017,(4):31
航空货运市场是全球航空运输市场的重要组成部分,与全球经济、贸易的发展息息相关。航空货运市场的发展趋势及需求直接影响到货机市场的发展趋势及货机行业的发展规划。而作为全球航空货运市场的运输载体,货机尤其是远程宽体货机对货物的国际间运输和交流起到了至关重要的作用。当前主流的预测方法为根据需求与供应的对应关系进行预测,预测过程相对复杂,预测的精度相对较高,不足之处在于预测工作周期较长,难以快速获得预测的结果。根据当前灰色系统理论,建立了宽体货机机队预测的灰色预测模型GM(1,1),并用分段组合的方式,较为精确地预测宽体货机未来机队的发展情况,预测较为快速,效率较高,能满足一般精度的预测需求。 相似文献
113.
为解决微纳聚合体卫星变构过程中,聚合体各部分之间的动力学耦合导致的卫星整体姿态翻转或紊乱,提出了一种对称式变构规划算法。首先建立了铰链约束下的漂浮基多刚体系统动力学模型,研究了重构过程中各运动模块对本体姿态的影响,提出当每两个运动模块位置与转动方向满足对称性条件时,两者对本体姿态的影响可在一定程度上相互抵消。基于上述理论,在A*算法中引入最优分配度量和对称性判定,设计了并行对称重构规划算法。仿真结果表明,该规划算法可实现重构过程中多模块并行、对称运动,重构过程总步数较少,运动模块对本体姿态的影响小。 相似文献
114.
运动的核弹比静止的核弹威力小?——多普勒效应、红移、光行差和动体的质能当量关系 总被引:1,自引:0,他引:1
证明爱因斯坦立足于光速不变假设和长度收缩假设的洛伦茨变换未能正确地解释多普勒效应、红移和光行差现象;他也未能给出正确的动体的质能当量关系.作者立足于完全符合相对性原理的伽利略变换,成功地解决了上述问题. 相似文献
115.
116.
高精度YAG超平光学基片高效范成法超精磨削的研究 总被引:1,自引:0,他引:1
随着YAG新型显示材料制成的高清晰度电视即将投放市场,使得YAG光学基片的批量生产和成本问题面临严峻考验.为了保证产品质量和企业生产效益,提出了大直径高精度YAG光学基片范成法超精磨削的设想.通过实验验证表明,该方法不仅能高效高质量生产合格的YAG光学基片,大幅度降低制造成本,而且为该方法在其它光学材料加工上的应用也奠定了基础. 相似文献
117.
E.G. Berezhko 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(3):429-441
We analyse the results of recent measurements of nonthermal emission from individual supernova remnants (SNRs) and their correspondence to the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is shown that the theory fits these data in a satisfactory way and provides the strong evidences for the efficient CR production in SNRs accompanied by significant magnetic field amplification. Magnetic field amplification leads to considerable increase of CR maximum energy so that the spectrum of CRs accelerated in SNRs is consistent with the requirements for the formation of Galactic CR spectrum up to the energy ∼1017 eV. 相似文献
118.
T.J. Stuchi T. Yokoyama A.A. Corrêa R.H. Solórzano D.M. Sanchez S.M.G. Winter O.C. Winter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The problem of a spacecraft orbiting the Neptune–Triton system is presented. The new ingredients in this restricted three body problem are the Neptune oblateness and the high inclined and retrograde motion of Triton. First we present some interesting simulations showing the role played by the oblateness on a Neptune’s satellite, disturbed by Triton. We also give an extensive numerical exploration in the case when the spacecraft orbits Triton, considering Sun, Neptune and its planetary oblateness as disturbers. In the plane a × I (a = semi-major axis, I = inclination), we give a plot of the stable regions where the massless body can survive for thousand of years. Retrograde and direct orbits were considered and as usual, the region of stability is much more significant for the case of direct orbit of the spacecraft (Triton’s orbit is retrograde). Next we explore the dynamics in a vicinity of the Lagrangian points. The Birkhoff normalization is constructed around L2, followed by its reduction to the center manifold. In this reduced dynamics, a convenient Poincaré section shows the interplay of the Lyapunov and halo periodic orbits, Lissajous and quasi-halo tori as well as the stable and unstable manifolds of the planar Lyapunov orbit. To show the effect of the oblateness, the planar Lyapunov family emanating from the Lagrangian points and three-dimensional halo orbits are obtained by the numerical continuation method. 相似文献
119.
H.J. Völk E.G. Berezhko L.T. Ksenofontov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(3):473-476
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 very close to the shock radius. Therefore a consistent explanation of these observations can be given in terms of efficient CR acceleration which makes the medium more compressible. 相似文献
120.
Li Jie Zhou Zhou 《中国航空学报》2008,21(1):19-27
To compute transonic flows over a complex 3D aircraft configuration, a viscous/inviscid interaction method is developed by coupling an integral boundary-layer solver with an Eluer solver in a "semi-inverse" manner. For the turbulent boundary-layer, an integral method using Green's lag equation is coupled with the outer inviscid flow. A blowing velocity approach is used to simulate the displacement effects of the boundary layer. To predict the aerodynamic drag, it is developed a numerical technique called far-field method that is based on the momentum theorem, in which the total drag is divided into three component drags, i.e. viscous, induced and wave-formed. Consequently, it can provide more physical insight into the drag sources than the often-used surface integral technique. The drag decomposition can be achieved with help of the second law of thermodynamics, which implies that entropy increases and total pressure decreases only across shock wave along a streamline of an inviscid non-isentropic flow. This method has been applied to the DLR-F4 wing/body configuration showing results in good agreement with the wind tunnel data. 相似文献