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原子钟的测量噪声会被引入到频率稳定度评估过程,尤其是对中短期频率稳定度的影响更大。重叠Allan方差可以克服调频闪变噪声和调频随机游走噪声随时间变化出现的非平稳问题,但由于受到测量噪声的影响,评估结果仍会出现误差。为此,本文通过对原子钟的数学模型和噪声特性进行分析,提出了原子钟频率稳定度评估的加窗平滑噪声处理方法,通过对时差观测序列合理的加窗设计和平滑处理,抑制测量噪声对评估结果的影响。实验结果表明,利用铷钟观测序列的100点平滑可以有效地提高短期频率稳定度结果(100~1 000)s的可信度。 相似文献
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针对应用于飞行器增压系统的双级气体减压器,从单级气体减压器的有限体积瞬变仿真模型出发建立了其数值模型,并搭建了双级减压器特性研究系统的模块化仿真模型.通过大量的时域仿真研究了某两型具有细微设计差异的减压器各结构参数对其工作稳定性的影响规律,并比较了两者间的异同,随后根据工程需要,选取减压器二级阀芯运动速度的样本方差作为稳定性指标,重点研究了某减压器二级阀芯质量、低压腔体积、反馈腔体积及膜片刚度变化对稳定性的影响程度.仿真结果表明,设计人员可以优先减小该减压器的二级阀芯质量或增大膜片刚度从而更快地改善其稳定性,该分析方法可以帮助相关设计人员以最小的代价获得满足工程要求的结果. 相似文献
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小转矩电动式负载模拟器的设计 总被引:14,自引:3,他引:14
设计了适用于小转矩范围的电动式负载模拟器,并分析了其结构和动态性能. 介绍了电动式负载模拟器的结构和工作原理,建立了电动式负载模拟器的数学模型,并对系统稳定性进行了理论分析和仿真研究.在系统中引入多重反馈和前馈,再辅以控制方法进行电机控制,收到了良好的效果.仿真数据表明,所设计的电动式负载模拟器在小转矩范围内能够达到电液负载模拟器的控制性能指标. 相似文献
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Q. Liu Z. Wu M. Zhu W.Q. Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The increase of balloon applications makes it necessary for a comprehensive understanding of the thermal and dynamic performance of scientific balloons. This paper proposed a novel numerical model to investigate the thermal and dynamic characteristics of scientific balloon in both ascending and floating conditions. The novel model consists of a dynamic model and thermal model, the dynamic model was solved numerically by a computer program developed with Matlab/Simulink to calculate the velocity and trajectory, the thermal model was solved by the Fluent program to find out the balloon film temperature distribution and inner Helium gas velocity and temperature field. These models were verified by comparing the numerical results with experimental data. Then the thermal and dynamic behavior of a scientific balloon in a real environment were simulated and discussed in details. 相似文献
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Yue Wang Shijie Xu Mengping Zhu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered. 相似文献
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