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481.
研究变元和文字出现次数受限制的规则3-SAT问题,提出了一种严格随机正则(3,s)-SAT问题,并给出了该问题的实例产生模型--SRR模型。结合一阶矩方法和生成函数展开项系数的渐近近似技术,证明了严格随机正则(3,s)-SAT问题相变点的上界,即当变元规模N较大且变元出现次数s>11时,严格随机正则(3,s)-SAT实例是高概率不可满足的。实验结果表明:由SRR模型所生成的随机实例中,当N>60且s>11时,所有的(3,s)-SAT实例均是不可满足的,而当N>150且s<11时,所有的(3,s)-SAT实例均是可满足的,即严格随机正则(3,s)-SAT实例的相变点位于s=11处,且在s=11处(子句变元比为11/3)的严格随机正则(3,s)-SAT实例,比在相变点(子句变元比)4.267处同规模的均匀随机3-SAT实例更难求解,因此,SRR模型可以很方便地在s=11处构造难解的随机3-SAT实例。 相似文献
482.
飞行器的星历积分不可避免涉及中心天体的选取问题。“嫦娥二号”卫星在拓展试验期间处于弱引力区,文章针对拓展试验期间的轨道状态,从受摄运动二体问题角度分析得出适宜选取太阳作为中心天体。进而结合真实力模型情况,使用行星星历表计算行星产生的摄动力,从理论上推导得出在忽略小天体摄动的前提下,由于摄动天体同时对中心天体和飞行器产生摄动作用,以地球为中心天体产生的摄动力类似于潮汐力,而以太阳为中心天体则不然,因而更适宜选取地球作为中心天体计算轨道运动问题 相似文献
483.
Two strategies extended the single-cascade methods from a compressible three-dimensional inverse method for radial and mixed flow turbomachines to two three-dimensional multi-cascade co-design methods for single-stage centrifugal compressors.These two three-dimensional methods and a typical quasi-three-dimensional streamline curvature through-flow inverse method were employed to design the same subsonic high-speed single-stage centrifugal compressors.The compressor performances were simulated by a commercial Reynolds averaged Navier-Stokes (RANS) equations solver.The studies show that two three-dimensional co-design methods are reasonable and feasible.It was found that:firstly the blade camber angle designed by the three-dimensional methods was larger than that designed by the quasi-three-dimensional method;and secondly with regard to two three-dimensional methods with different boundary conditions,the co-design result differences between the diffusers were small,but those between the deswirlers were relatively large. 相似文献
484.
485.
R. Bewick J.P. Sanchez C.R. McInnes 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
This paper presents a novel method of space-based geoengineering which uses the mass of a captured near Earth asteroid to gravitationally anchor a cloud of unprocessed dust in the vicinity of the L1 position to reduce the level of solar insolation at Earth. It has subsequently been shown that a cloud contained within the zero-velocity curve of the largest near Earth asteroid, Ganymed, can lead to an insolation reduction of 6.58% on Earth, which is significantly larger than the 1.7% required to offset a 2 °C increase in mean global temperature. The masses of the next largest near Earth asteroids are found to be too small to achieve the required level of insolation reduction, however, they are significant enough to be used as part of a portfolio of geoengineering schemes. 相似文献
486.
高超声速飞行器上升段最优制导间接法研究 总被引:3,自引:1,他引:2
高超声速飞行器的机身-推进一体化设计使得气动和推进之间存在强非线性耦合,本文针对高超声速飞行器的特点,提出了求解最优上升轨迹的一种可行方案。在零侧滑角和力矩瞬间平衡假设下对上升段飞行问题进行最优建模,将质量引入为状态量,以最省燃料为指标,以推力方向为最优控制量,根据极大值原理推导一阶最优条件。为数值求解两点边值问题,以解析解作为初始猜想,应用经典的有限差分方法和改进的牛顿法,在满足攻角过程约束下,通过同伦算法迭代求解最优轨迹。仿真在给定的初始约束和终端约束下进行,结果表明该制导算法能够实现对高超声速飞行器上升轨迹的优化,以参考面积为同伦参数的迭代方法,能够保证算法的收敛性和快速性。
相似文献
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487.
文章讨论利用给定的三个向量对构造不可约三对角矩阵、Jacobi矩阵和负Jacobi矩阵的反问题.在求解方法中,将已知的-些关系式等价地转化为线性方程组,利用线性方程组有解的条件,得到了所研究问题有惟一解的充要条件,并给出了数值算法和例子. 相似文献
488.
自主发展了径流及斜流涡轮的准三维流线曲率法通流设计程序,应用该程序给出了一项500 N推力级微型涡喷发动机斜流涡轮的气动设计和叶片造型.通过计算流体力学检验和整体叶轮强度检验,该微型斜流涡轮超过了预定的设计指标.为实现径流涡轮和斜流涡轮设计反问题的统一,流线曲率法的S2,m流面准径向平衡方程是沿流线方向m和流线的准法线方向口写出,该系统也可用于轴流涡轮的设计.采用了在所有计算站上的"全可控涡法"进行气动设计. 相似文献
489.
为了研究Halo轨道中继通信以及行星际轨道转移等问题,需要首先对拉格朗日点(平动点)的理论进行分析。使用考虑太阳辐射的椭圆型限制性三体建模,代替原有的圆型限制性三体建模,提高了建模的精度。提出了在L1,L2,L3点的更为精确的新解析解,经过Matlab仿真,其相对于精确数值解的误差,分别为Ammar的解析解的13.13%,29.51%,0.46%。 相似文献
490.
Modeling of LEO orbital debris populations for ORDEM2008 总被引:2,自引:0,他引:2
Y.-L. Xu M. Horstman P.H. Krisko J.-C. Liou M. Matney E.G. Stansbery C.L. Stokely D. Whitlock 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The NASA Orbital Debris Engineering Model, ORDEM2000, is in the process of being updated to a new version: ORDEM2008. The data-driven ORDEM covers a spectrum of object size from 10 μm to greater than 1 m, and ranging from LEO (low Earth orbit) to GEO (geosynchronous orbit) altitude regimes. ORDEM2008 centimeter-sized populations are statistically derived from Haystack and HAX (the Haystack Auxiliary) radar data, while micron-sized populations are estimated from shuttle impact records. Each of the model populations consists of a large number of orbits with specified orbital elements, the number of objects on each orbit (with corresponding uncertainty), and the size, type, and material assignment for each object. This paper describes the general methodology and procedure commonly used in the statistical inference of the ORDEM2008 LEO debris populations. Major steps in the population derivations include data analysis, reference-population construction, definition of model parameters in terms of reference populations, linking model parameters with data, seeking best estimates for the model parameters, uncertainty analysis, and assessment of the outcomes. To demonstrate the population-derivation process and to validate the Bayesian statistical model applied in the population derivations throughout, this paper uses illustrative examples for the special cases of large-size (>1 m, >32 cm, and >10 cm) populations that are tracked by SSN (the Space Surveillance Network) and also monitored by Haystack and HAX radars operating in a staring mode. 相似文献