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排序方式: 共有244条查询结果,搜索用时 343 毫秒
111.
基于混杂系统的空间飞行器悬停控制 总被引:3,自引:1,他引:2
基于空间飞行器的轨道动力学原理,利用混杂系统模型研究了悬停轨道问题,建立了悬停轨道的混杂系统模型;借此模型,针对目标星轨道为椭圆的情况,提出了等距离悬停轨道控制和椭圆悬停轨道控制两种方案,分别推导出在这两种方案下对悬停星所施加的控制力。数值仿真结果表明,分别对悬停星施加相应的控制力,能够实现对目标星的悬停。 相似文献
112.
W.D. Song R.L. Wang J. Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
A simple analysis method for orbit anomaly detection, called semi-major axis change method (SACM) was presented by using a relationship between the change of orbit parameters and velocity increments. In this method, the mean value and standard deviation of the semi-major axis change in different time intervals were first calculated according to historical data. Then, these two parameters, the mean value and standard deviation of the semi-major axis change, are chosen as basis variables and combined as an anomalous criterion. For orbit objects with different characteristic, anomalous thresholds were given in different time intervals for identifying the anomalies of the orbital objects. Finally, this method is used for low earth orbit (LEO) satellites and American–Russian breakup debris. By adopting this method, the characteristics of the orbit change were given. The accuracy rate of anomaly analysis for LEO satellites and American–Russian breakup debris can reach to 100%, which demonstrates that the method was rapid and valid. 相似文献
113.
为了研究以波箔型径向气体箔片轴承为支承的轴承-转子系统动力学特性,专门设计了波箔型径向气体箔片轴承试验台,质量为0.458kg的转子在该试验台上实现了超过80000r/min的运转速度.径向轴承为波箔型径向气体箔片轴承,止推轴承为多叶箔片轴承.试验结果表明:波箔型径向气体箔片轴承能够实现转子高速运行,在转子起飞后具有良好的运行稳定性,其轴承支承处振动位移幅值一直维持在20μm之内.由于驱动涡轮受到不平衡气流力的作用,转轴升速时的起飞转速要高于降速时的起飞转速. 相似文献
114.
Aaron J. Rosengren Daniel J. Scheeres Jay W. McMahon 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The classical Laplace plane is a frozen orbit, or equilibrium solution for the averaged dynamics arising from Earth oblateness and lunisolar gravitational perturbations. The pole of the orbital plane of uncontrolled GEO satellites regress around the pole of the Laplace plane at nearly constant inclination and rate. In accordance with Friesen et al. (1993), we show how this stable plane can be used as a robust long-term disposal orbit. The current graveyard regions for end-of-life retirement of GEO payloads, which is several hundred kilometers above GEO depending on the spacecraft characteristics, cannot contain the newly discovered high area-to-mass ratio debris population. Such objects are highly susceptible to the effects of solar radiation pressure exhibiting dramatic variations in eccentricity and inclination over short periods of time. The Laplace plane graveyard, on the contrary, would trap this debris and would not allow these objects to rain down through GEO. Since placing a satellite in this inclined orbit can be expensive, we discuss some alternative disposal schemes that have acceptable cost-to-benefit ratios. 相似文献
115.
随着遥感卫星分辨率的不断提高,动量轮扰振对遥感成像的影响逐渐成为卫星总体设计时需要关注的问题。目前对动量轮微振动的研究多侧重于时域分析,经常把卫星平台和载荷分立开来单独研究。鉴于平台和相机之间具有耦合作用,分立研究会带来较大误差。动量轮的输出响应并不是一个单一频率的时域信号,不同频谱对相机的影响不同,频谱分析往往更能反映问题。文章联合卫星平台和相机进行整星建模,分析了微振动扰振从动量轮处传递到相机光学元件的频谱特征,得到动量轮扰振不同频谱对相机造成的具体影响。分析结果显示,低于相机基频的动量轮扰振频谱造成相机光轴晃动,相机特征频率区间的扰振频谱不仅会放大光轴晃动,还会造成相机内部的光学元件光轴不一致。最后文章定量计算比较了这两种影响带来的MTF下降。 相似文献
116.
针对伴随微纳卫星资源受限、轨控需要尽可能节省燃料的现实问题,基于希尔(Hill)方程,研究推导了共面编队伴飞卫星的轨控时机和轨控方向对相对运动椭圆短半轴控制效率的影响。理论推导和仿真均表明:当控制量大小|ΔV|与相对运动椭圆短半轴b满足|ΔV|≤nb/2关系时(n为参考星平均轨道角速度),在相对运动椭圆上下点进行横向或反横向控制,最大效率地将相对运动椭圆短半轴改变了|Δb|=2|ΔV|/n。其中,在上点反横向或下点横向进行控制,可以最大效率地增大椭圆短半轴;在上点横向或下点反横向进行控制,可以最大效率地减小椭圆短半轴。 相似文献
117.
《中国航空学报》2021,34(10):248-264
This study presents a method for measuring the imbalance in a small-sized cylindrical roller. The roller imbalance was calibrated on the built static-pressure-air flotation measurement machine. The impact of the roller imbalance on the dynamic characteristics of a cage were then studied on the aero-bearing test rig. The displacement spectrums with different roller imbalance of the obtained cage orbits under various bearing speed and radial load were used to evaluate the cage stability. The results show that the cage cannot form a stable operating state at a lower bearing speed with or without the unbalanced rollers. The cage with balanced rollers gradually develops stable motion with the increase of the bearing speed. The existence of a small roller imbalance causes the stability of the cage to deteriorate. With an increase in the bearing speed and radial load, the cage with the unbalanced rollers runs unsteadily accompanied by a high-frequency vibration when the roller imbalance is large enough. The vibration amplitude of the cage in the horizontal direction is greater than that in the vertical direction during an unstable operation, which is similar in the stable status. 相似文献
118.
Despoina K. Skoulidou Aaron J. Rosengren Kleomenis Tsiganis George Voyatzis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3646-3674
The Medium Earth Orbit (MEO) region hosts satellites for navigation, communication, and geodetic/space environmental science, among which are the Global Navigation Satellites Systems (GNSS). Safe and efficient removal of debris from MEO is problematic due to the high cost for maneuvers needed to directly reach the Earth (reentry orbits) and the relatively crowded GNSS neighborhood (graveyard orbits). Recent studies have highlighted the complicated secular dynamics in the MEO region, but also the possibility of exploiting these dynamics, for designing removal strategies. In this paper, we present our numerical exploration of the long-term dynamics in MEO, performed with the purpose of unveiling the set of reentry and graveyard solutions that could be reached with maneuvers of reasonable cost. We simulated the dynamics over 120–200?years for an extended grid of millions of fictitious MEO satellites that covered all inclinations from 0 to 90°, using non-averaged equations of motion and a suitable dynamical model that accounted for the principal geopotential terms, 3rd-body perturbations and solar radiation pressure (SRP). We found a sizeable set of usable solutions with reentry times that exceed years, mainly around three specific inclination values: 46°, 56°, and 68°; a result compatible with our understanding of MEO secular dynamics. For m/s (i.e., achieved if you start from a typical GNSS orbit and target a disposal orbit with ), reentry times from GNSS altitudes exceed years, while low-cost ( m/s) graveyard orbits, stable for at lest 200?years, are found for eccentricities up to . This investigation was carried out in the framework of the EC-funded “ReDSHIFT” project. 相似文献
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