排序方式: 共有16条查询结果,搜索用时 31 毫秒
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根据星群分离控制的一般要求,本文研究了卫星群的相对运动方程,分析了其相对运动特性,在合理的近似假设下对Hill方程为出发点,研究了各卫星相对距离限制下的分离控制方法。最后对精确方程与近似方程的仿真比较,表明所设计的健康控制方法是可行的,其结果是可信的。 相似文献
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为了得到控制量与控制时机对相位改变的直观公式,基于Hill方程以及迹向控制的约束条件,定性分析共面绕飞编队中控制量、控制时机与编队卫星相位之间的关系,分析结果表明:当需要改变的相位角小于90°时,可实现最省燃料的控制;当需要改变的相位角大于90°时,可进行趋于最小控制量的控制;当在相对运动椭圆上下点实施控制时,相位无变化. 相似文献
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在研究二进制、带符号的二进制(NAF,Non-Adjacent Form)等常见标量乘法算法的基础上,结合椭圆曲线基点的周期特性和预计算倍点序列方式,提出了一种新的标量乘法算法,并给出了新算法的详细步骤.点的周期性和系数决定了直接进行标量乘法运算还是转化为求其逆元,预计算倍点序列方式避免了椭圆曲线密码体制(ECC,Elliptic Curve Cryptosystem)加解密过程中大量的重复运算.为验证算法的正确性,采用密钥长度为192 bit椭圆曲线,给出了一个具体实例.实例结果和算法分析表明:与二进制和NAF算法相比,新算法虽占用了一些存储空间,但省去了倍点运算的时间开销,同时减少了点加的运算次数,极大地提高了标量乘法运算的效率.该算法的提出对完善ECC理论和加快ECC在实际中的应用具有重要意义. 相似文献
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Masaya Kimura Masanori Kawamura Katsuhiko Yamada 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1336-1346
An analytical expression for distant retrograde orbits (DROs) is obtained in this study. Owing to the fact that a planar DRO is a closed orbit and can be expressed as an approximately elliptical orbit, respective geometries and periods of DROs are analytically calculated. A switching point, where various properties of planar DROs change abruptly with an increase in the orbital radius, is determined. The Mars–Deimos system is taken as a case study in this work. The proposed method can be applied to cases where the Hill’s approximation of the restricted three-body problem is valid. Numerical calculations are performed to validate the proposed method. 相似文献
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小卫星空间圆形编队飞行队形设计与比例-微分(PD)控制 总被引:2,自引:2,他引:2
以两体相对运动动力学为基础 ,对Hill方程表示的相对运动特性进行了分析。同时给出了小卫星空间圆形编队队形设计。并且以此队形为例 ,引入了比例 -微分 (PD)控制策略对小卫星编队飞行的队形控制进行了研究 ,利用最优算法确定了控制器比例微分系数。数字仿真结果表明了该控制策略的有效性 相似文献
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S.P. Sosnitskii 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
In the three-body problem, we consider the Lagrange and Hill stability including the Lagrange stability for the manifold of symmetric motions that exists in the case where two of three bodies have equal masses. To analyze the stability, in addition to integrals of energy and angular momentum we use the Lagrange–Jacobi equality. We prove theorems on the Lagrange and Hill stability. The theorem on the Hill stability has effective application in the case where the mass of a body is much less than masses of two other bodies. In this case, as it is known, the model of the restricted three-body problem is usually applied. 相似文献