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空间微小碎片累积作用下材料光学性能退化预示模型适用性研究 总被引:1,自引:1,他引:1
航天器在轨服役期间会遭受到大量空间微小碎片和微流星体的撞击作用,其中的微米级粒子将在航天器表面产生大面积砂蚀现象,并使材料或器件功能衰退。文章介绍了NASA空间微小碎片累积损伤材料光学性能退化预示模型并推导了两个预示模型之间的关系。利用ORDEM2000碎片分布模型估算了K8玻璃累积损伤面积。以K8玻璃为例,对比研究了两个预示模型的适用性。结果表明,当航天器外表面损伤程度小于40%,可利用Canoon模型评价和预示材料光学性能退化规律;当航天器外表面损伤程度大于40%,需利用Mirtich模型评价和预示材料光学性能退化规律。 相似文献
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一种基于SIFT和KLT相结合的特征点跟踪方法研究 总被引:2,自引:0,他引:2
在目标发生明显姿态和大小变化条件下,为了利用基于特征点的跟踪算法实现对目标可靠、稳定跟踪,提出了一种SIFT算法和KLT(Kanade-Lucas-Tomasi)匹配算法相结合的特征点跟踪方法。通过对SIFT算法进行优化,使得到特征点分布相对均匀,同时不存在聚集现象;通过对KLT匹配算法进行分层迭代设计,提高了目标作快速运动时的匹配精度;最后根据特征点匹配结果,结合Greedy算法得到目标的准确位置。实验结果表明:该算法能够很好地适应目标姿态和大小的变化,实现对结构复杂目标的稳定跟踪;比KLT跟踪算法具有更好的鲁棒性和稳定性,能得到更加准确的目标位置。 相似文献
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M.?Yu.?Belyaev T.?V.?Matveeva M.?I.?Monakhov D.?N.?Rulev V.?V.?SazonovEmail author 《Cosmic Research》2018,56(1):54-67
We have reconstructed the uncontrolled rotational motion of the Progress M-29M transport cargo spacecraft in the single-axis solar orientation mode (the so-called sunward spin) and in the mode of the gravitational orientation of a rotating satellite. The modes were implemented on April 3–7, 2016 as a part of preparation for experiments with the DAKON convection sensor onboard the Progress spacecraft. The reconstruction was performed by integral statistical techniques using the measurements of the spacecraft’s angular velocity and electric current from its solar arrays. The measurement data obtained in a certain time interval have been jointly processed using the least-squares method by integrating the equations of the spacecraft’s motion relative to the center of mass. As a result of processing, the initial conditions of motion and parameters of the mathematical model have been estimated. The motion in the sunward spin mode is the rotation of the spacecraft with an angular velocity of 2.2 deg/s about the normal to the plane of solar arrays; the normal is oriented toward the Sun or forms a small angle with this direction. The duration of the mode is several orbit passes. The reconstruction has been performed over time intervals of up to 1 h. As a result, the actual rotational motion of the spacecraft relative to the Earth–Sun direction was obtained. In the gravitational orientation mode, the spacecraft was rotated about its longitudinal axis with an angular velocity of 0.1–0.2 deg/s; the longitudinal axis executed small oscillated relative to the local vertical. The reconstruction of motion relative to the orbital coordinate system was performed in time intervals of up to 7 h using only the angularvelocity measurements. The measurements of the electric current from solar arrays were used for verification. 相似文献
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The results of numerical calculation of the dependences of the electron density, the eigenfrequency and the dielectric plasma permeability on the geometric parameters and the altitude of body motion in the near and far wake behind a thin conical body with a spherical nose blunting have been presented. The electron density maximum has been shown to be located in the region of the neck of the near wake behind the body, which determines the type of this region (supercritical or subcritical). This in turn affects the propagation of radio waves through this plasma region. A comparative analysis was performed for two different bodies with the same ballistic coefficient values. No characteristic distinctions were revealed in the values of electron density or the plasma eigenfrequency in the near and far wake behind these bodies. However, it has been shown that there are differences in the values of the distance from the bottom cross section to the neck of the near wake behind these bodies. 相似文献
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In the paper, the problem of designing interplanetary trajectories with several swing-bys and deep-space maneuvers is solved using the method of virtual trajectories developed by the authors. The algorithms for the calculation of both heliocentric and planetocentric trajectory arcs are presented, including the case of resonant trajectories. The results of applying the method of virtual trajectories to the problem of designing an interplanetary transfer to Jupiter are given and compared with the baseline trajectories for the Juno, Europa Clipper, and Laplace missions. 相似文献
610.