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811.
快速成形法及应用可能分析 总被引:2,自引:0,他引:2
郭永卫 《航空精密制造技术》1998,(1)
简要介绍快速成形技术和一种典型快速成形机的工作原理,并阐述了此技术的主要用途、应用方法及应用可行性分析。 相似文献
812.
There are huge potential applications of 3-D braided composite in aerospace engineering because of the non-delamination feature of the composite under impact loading. This paper presents the analysis of energy absorption features of 3-D braided composite under compression with different strain rates. The 3-D 4-step rectangular braided composite coupons were tested on a material tester MTS 810.23 and a split Hopkinson pressure bar (SHPB) apparatus to obtain out-of-plane and in-plane compression stress vs. strain curves at quasi-static and high strain rate state. The failure modes and energy absorption features of the 3-D braided composite under different strain rates were analyzed both in time domain and frequency domain. The energy absorbed by the 3-D braided composite increases with the strain rate. From fast Fourier transform (FFT) analysis of compression stress vs. time histories, the power of energy absorption of the 3-D braided composite increases with strain rate and mostly concentrate on the high frequency region. While for quasi-static compression, the power distributes in very narrow frequency region and also is less than that in high strain rates. This feature corresponds to the different damage and energy absorption mechanisms of the 3-D braided composite under quasi-static and high strain rate compression. 相似文献
813.
为了研究DSM11镍基高温合金的抗热腐蚀性能,对该合金在650、750、850℃条件下涂覆5%NaCl+95%Na 2 SO 4 混合盐膜
进行腐蚀试验。利用金相显微镜(OM)、扫描电子显微镜(SEM)、能谱仪(EDS)和X射线衍射仪(XRD)等手段,对合金被腐蚀200 h
后的表面形貌、物相组成、元素和腐蚀层的分布情况以及腐蚀机理进行分析。结果表明:随着试验温度的升高,合金表面腐蚀程度
逐渐加重、腐蚀产物组成逐渐复杂、失重加大、腐蚀产物层厚度增大;合金的腐蚀产物层均可分为3层,最外层和中间层主要为氧
化物,内层由颗粒状氧化物和硫化物组成,O和S的侵入现象表明合金发生了较明显的内氧化与内硫化现象;在3种温度下,合金
表面生成连续稳定的Al 2 O 3 保护层,抑制了热腐蚀反应的进行,对基体存在有效的保护作用,表明合金具有一定的抗热腐蚀性能。 相似文献
814.
点云去噪的效果对三维扫描过程后续的曲面拟合与造型设计至关重要,如何快速准确提取特征点已成为研究热点,然而点云去噪的关键之处在于奇异值与离群值的检测。提出耦合多特征点参数的去噪模型,分别讨论每个特征点参数对去噪模型的影响程度;采用群智能算法求解出一组最优参数权重,以此确定点云去噪模型,从而达到三维散乱点云最优去噪效果;通过对Bunny 模型进行去噪仿真以及某一型号的蒙皮进行去噪实验,对去噪模型进行验证。结果表明:本文提出的点云去噪模型相较于半径滤波器、统计滤波器、改进体素滤波结合高斯滤波模型,迭代更快、耗时更少,具有更好的去噪效果。 相似文献
815.
Initial virtual flight test for a dynamically similar aircraft model with control augmentation system 总被引:3,自引:0,他引:3
To satisfy the validation requirements of flight control law for advanced aircraft,a wind tunnel based virtual flight testing has been implemented in a low speed wind tunnel.A 3-degree-offreedom gimbal,ventrally installed in the model,was used in conjunction with an actively controlled dynamically similar model of aircraft,which was equipped with the inertial measurement unit,attitude and heading reference system,embedded computer and servo-actuators.The model,which could be rotated around its center of gravity freely by the aerodynamic moments,together with the flow field,operator and real time control system made up the closed-loop testing circuit.The model is statically unstable in longitudinal direction,and it can fly stably in wind tunnel with the function of control augmentation of the flight control laws.The experimental results indicate that the model responds well to the operator's instructions.The response of the model in the tests shows reasonable agreement with the simulation results.The difference of response of angle of attack is less than 0.5°.The effect of stability augmentation and attitude control law was validated in the test,meanwhile the feasibility of virtual flight test technique treated as preliminary evaluation tool for advanced flight vehicle configuration research was also verified. 相似文献
816.
三维工序模型的演进式构建方法 总被引:1,自引:0,他引:1
为实现以三维工序模型为核心的三维工艺构建,基于从毛坯模型到最终产品模型的演进过程,对三维工序模型的生成方法进行研究.在制造特征信息模型的基础上,结合基准信息建立了面向工序模型生成的工序信息模型.提出制造特征信息在工序模型中的映射机制,解决该模式下工序模型信息缺失的问题.以工序信息模型为模板,首先定义加工特征基元,然后通过实例化实现工序模型的变换.最后,通过集成工艺决策系统,构建三维工序模型生成系统,为后续工艺尺寸标注和工艺展示提供模型支持. 相似文献
817.
多用酸洗缓蚀剂DSCH-1的研究 总被引:1,自引:0,他引:1
由含氮的脂肪胺、芳香胺等多种常用的有机缓蚀剂复配制成的DSCH-1 缓蚀剂,在硝酸中对20# 锅炉钢和紫铜的缓蚀效率达99.7% ,在盐酸中对20# 锅炉的钢的缓蚀效率达98.5% ,对紫铜的缓蚀效率也较高。Fe3+ 离子浓度对DSCH-1 缓蚀性能有较大的影响 相似文献
818.
S. Karakula W. Tkaczyk F. Giovannelli 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
In the spherical accretion onto massive objects, the matter may be heated up to temperatures as high as 1012 °K. In such a hot plasma, the thermal bremsstrahlung (e-e and e-p) and π° decay from inelastic collisions of protons are the main γ-ray sources. We determined the γ -ray production spectra from the π° decay and from bremsstrahlung for different temperatures. The expected γ-ray spectra were evaluated too in order to fit experimental data. We have fitted COS B data from 3C 273 using a two temperatures plasma model. The best fit is for
(M8 is the black hole mass in 108 M) which gives
. The hard X-ray measurements do not contradict the bremsstrahlung spectrum. 相似文献
Full-size image (1K)
819.
Naoya Maeda Satoko Takasaki Hideaki Kawano Shinichi Ohtani P.M.E. Décréau J.G. Trotignon S.I. Solovyev D.G. Baishev Kiyohumi Yumoto 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
By applying the cross-phase method and the amplitude-ratio method to magnetic field data obtained from two ground stations located close to each other, we can determine the frequency of the field line resonance (FLR), or the field line eigenfrequency, for the field line running through the midpoint of the two stations. From thus identified FLR frequency we can estimate the equatorial plasma mass density (ρ) by using the T05s magnetospheric field model [Tsyganenko, N.A., Sitnov, M.I. Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms, J. Geophys. Res. 110, A03208, 2005] and the equation of Singer et al. [Singer, H.J., Southwood, D.J., Walker, R.J., Kivelson, M.G. Alfven wave resonances in a realistic magnetospheric magnetic field geometry, J. Geophys. Res. 86 (A6) 4589–4596, 1981]. 相似文献
820.
M.S. Skidmore R.M. Ambrosi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(9):1019-1029
Understanding the evolution of Mars requires determining the composition of the surface and atmosphere of the planet. The European Space Agency’s ExoMars rover mission, which is expected to launch in 2016, is part of the Aurora programme. The instruments on the rover will search for evidence of life on Mars and will map a sub-section of the Martian surface, extracting compositional information. Currently our understanding of the bulk composition (and mineralogy) of Mars relies on orbital data from instruments on-board satellites such as 2001 Mars Odyssey, Mars Reconnaissance Orbiter and Mars Express, in addition to in-situ instrumentation on rovers such as Spirit and Opportunity. γ-ray spectroscopy can be used to determine the composition of Mars, but it has yet to be successfully carried out in-situ on Mars. This study describes some of the results obtained from the γ-ray spectrometer on 2001 Mars Odyssey during solar proton events and discusses whether the increased emissions are useful in γ-ray spectroscopy. The study shows that although increased γ-ray emissions were expected from the Martian surface during a solar proton event, they were not detected from orbit probably due to insufficient signal-to-background. However, this does not preclude the possibility of measuring changes in γ-ray flux corresponding to changes in solar activity on the surface of the planet. 相似文献