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对紧凑拉伸(CT)试样的柔度转动修正方法进行了研究,理清了现行柔度转动修正方法存在的问题,给出了新的转动修正方法,并提出了考虑转动效应的CT试样的裂纹嘴张开位移(CMOD,V0)与加载线张开位移(VLL)的转换公式。弹塑性有限元分析表明,CT试样产生刚性转动的中心并不在试样的剩余韧带中心,而是在偏靠裂纹尖端的位置;转动半径 R 基本不受材料本构关系的影响,仅与CT试样的裂纹长度a与宽度W之比(a/W)有关,从而提出了R与a/W之间的单调多项式;当裂纹尖端产生较大程度的塑性变形时,需要考虑转动效应对CT试样裂纹张开位移(COD)测量的影响, J积分的塑性功计算须采用经转动修正后的COD。采用两种延性材料Cr2Ni2MoV和16MnR对COD转换公式进行了实验验证,结果表明,基于转动分析的COD转换公式由于考虑了裂纹尖端附近区域的弹塑性变形行为,用于断裂韧性测试中的塑性功计算更加符合实际,且同实验结果符合良好;直通型紧凑拉伸(FFCT)试样的刚性转动对较大裂纹扩展情形下的JR阻力曲线影响较大。 相似文献
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In this paper, we propose an uncertainty analysis and design optimization method and its applications on a hybrid rocket motor(HRM) powered vehicle. The multidisciplinary design model of the rocket system is established and the design uncertainties are quantified. The sensitivity analysis of the uncertainties shows that the uncertainty generated from the error of fuel regression rate model has the most significant effect on the system performances. Then the differences between deterministic design optimization(DDO) and uncertainty-based design optimization(UDO) are discussed. Two newly formed uncertainty analysis methods, including the Kriging-based Monte Carlo simulation(KMCS) and Kriging-based Taylor series approximation(KTSA), are carried out using a global approximation Kriging modeling method. Based on the system design model and the results of design uncertainty analysis, the design optimization of an HRM powered vehicle for suborbital flight is implemented using three design optimization methods: DDO, KMCS and KTSA. The comparisons indicate that the two UDO methods can enhance the design reliability and robustness. The researches and methods proposed in this paper can provide a better way for the general design of HRM powered vehicles.In this paper,we propose an uncertainty analysis and design optimization method and its applications on a hybrid rocket motor(HRM)powered vehicle.The multidisciplinary design model of the rocket system is established and the design uncertainties are quantified.The sensitivity analysis of the uncertainties shows that the uncertainty generated from the error of fuel regression rate model has the most significant effect on the system performances.Then the differences between deterministic design optimization(DDO)and uncertainty-based design optimization(UDO)are discussed.Two newly formed uncertainty analysis methods,including the Kriging-based Monte Carlo simulation(KMCS)and Kriging-based Taylor series approximation(KTSA),are carried out using a global approximation Kriging modeling method.Based on the system design model and the results of design uncertainty analysis,the design optimization of an HRM powered vehicle for suborbital flight is implemented using three design optimization methods:DDO,KMCS and KTSA.The comparisons indicate that the two UDO methods can enhance the design reliability and robustness.The researches and methods proposed in this paper can provide a better way for the general design of HRM powered vehicles. 相似文献
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形状自适应的小波变换编码可以编码任意形状的物体,不但保持了物体的纹理信息,而且编码不会带来不必要的冗余.但是当对任意形状的物体进行小波变换时,会由于变换序列的长度、下采样位置的不同而带来一些变化.文章利用懒小波对任意形状的掩膜进行变换,并且采用9-7滤波器的提升小波形式,很好地解决了这些问题.最终通过修正的形状自适应的SPIHT算法,对任意形状物体的内部纹理进行编码压缩.与原始算法相比,性能提高了大约0.2 dB. 相似文献
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为研究系留气球稳定性,建立了系留气球的三维非线性动力学模型.缆绳采用有限差分法,球体采用经典的六自由度方程,其中气动力导数以静导数、动导数和附加质量表示.以主节点运动为边界条件,以静态构型为初始条件,建立完整耦合动力学方程.利用直接求解非线性偏微分方程的方法对该系统进行时域响应分析,考察了风速对纵向和横侧向稳定性的影响,并给出相应的响应曲线.直接求解非线性耦合方程的成功,表明该数学模型及其解法是可行的. 相似文献
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L. Liu Y. Dong G. Bao W.-T. Ni D.N.A. Shaul 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
As ASTROD I travels through space, its test mass will accrue charge due to exposure of the spacecraft to high-energy particles. This test mass charge will result in Coulomb forces between the test mass and the surrounding electrodes. In earlier work, we have used the GEANT 4 toolkit to simulate charging of the ASTROD test mass due to cosmic-ray protons of energies between 0.1 and 1000 GeV at solar maximum and at solar minimum. Here we use GEANT 4 to simulate the charging process due to solar energetic particle events and interplanetary electrons. We then estimate the test mass acceleration noise due to these fluxes. The predicted charging rates range from 2247 e+/s to 47,055 e+/s, at peak intensity, for the four largest SEP events in September and October 1989. Although the noise due to charging exceeds the ASTROD I budget for the two larger events, it can be suppressed through continuous discharging. The acceleration noise during the two small events is well below the design target. The charging rate of the ASTROD I test mass due to interplanetary electrons in this simulation is about −11% of the cosmic-ray protons at solar minimum, and over −37% at solar maximum. In addition to the Monte Carlo uncertainty, an error of ±30% in the net charging rates should be added to account for uncertainties in the spectra, physics models and geometry implementations. 相似文献
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