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161.
地球同步轨道高压太阳电池阵充放电效应研究 总被引:4,自引:2,他引:4
地球同步轨道(GEO)高压太阳电池阵表面静电放电(ESD)引起二次放电可能导致太阳电池阵永久性短路损坏。文章主要针对GEO高压太阳电池阵充放电效应问题,重点分析了高压太阳电池阵表面ESD和二次放电产生的物理过程,并利用负高压偏置方法开展了GEO高压太阳电池阵表面ESD和二次放电地面模拟试验。试验验证了反转电位梯度电场是导致GEO高压太阳电池阵表面产生ESD的触发因素之一,同时得到了GaAs高压太阳电池阵样品表面产生ESD和二次放电的电压阈值。 相似文献
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一种基于模拟退火的支持向量机超参数优化算法 总被引:7,自引:0,他引:7
基于统计学习理论的支持向量机技术以探求小样本情况下如何获得更好的机器学习规律而见长,与基于经验风险最小化原则的机器学习方法相比能够获得更佳的泛化能力,相关超参数的选择对其分类或回归性能有较大影响.针对径向基核支持向量机超参数优化问题,提出了一种改进的基于模拟退火算法的高效多目标优化算法,并详细讨论了优化寻优过程中搜索空间、初始可行解、初温和最优目标函数的设计方法.通过在多个标准数据集上的测试验证,证实了本文所提算法的可行性和有效性. 相似文献
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Brigitte Knapmeyer-Endrun Naomi Murdoch Balthasar Kenda Matthew P. Golombek Martin Knapmeyer Lars Witte Nicolas Verdier Sharon Kedar Philippe Lognonné William B. Banerdt 《Space Science Reviews》2018,214(5):94
Based on an updated model of the regolith’s elastic properties, we simulate the ambient vibrations background wavefield recorded by InSight’s Seismic Experiment for Interior Structure (SEIS) on Mars to characterise the influence of the regolith and invert SEIS data for shallow subsurface structure. By approximately scaling the synthetics based on seismic signals of a terrestrial dust devil, we find that the high-frequency atmospheric background wavefield should be above the self-noise of SEIS’s SP sensors, even if the signals are not produced within 100–200 m of the station. We compare horizontal-to-vertical spectral ratios and Rayleigh wave ellipticity curves for a surface-wave based simulation on the one hand with synthetics explicitly considering body waves on the other hand and do not find any striking differences. Inverting the data, we find that the results are insensitive to assumptions on density. By contrast, assumptions on the velocity range in the upper-most layer have a strong influence on the results also at larger depth. Wrong assumptions can lead to results far from the true model in this case. Additional information on the general shape of the curve, i.e. single or dual peak, could help to mitigate this effect, even if it cannot directly be included into the inversion. We find that the ellipticity curves can provide stronger constraints on the minimum thickness and velocity of the second layer of the model than on the maximum values. We also consider the effect of instrumentation resonances caused by the lander flexible modes, solar panels, and the SEIS levelling system. Both the levelling system resonances and the lander flexible modes occur at significantly higher frequencies than the expected structural response, i.e. above 35 Hz and 20 Hz, respectively. While the lander and solar panel resonances might be too weak in amplitude to be recorded by SEIS, the levelling system resonances will show up clearly in horizontal spectra, the H/V and ellipticity curves. They are not removed by trying to extract only Rayleigh-wave dominated parts of the data. However, they can be distinguished from any subsurface response by their exceptionally low damping ratios of 1% or less as determined by random decrement analysis. The same applies to lander-generated signals observed in actual data from a Moon analogue experiment, so we expect this analysis will be useful in identifying instrumentation resonances in SEIS data. 相似文献
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发兰,磷化是钢铁表面处理应用最为广泛的工艺。该研究得出了最新工艺配方,使发兰,磷化工艺具有低温性,低渣量,快速性,低成本的特点。 相似文献
167.
本文对乐安河流域160名儿童发中Cu、Zn、Pb、Cd、Ni、Mn、Fe七种微量元素的含量进行了测定和分析。经比较发现,新建与中洲之间,Cu、Mn、Fe含量差异有极显著性(p<0.01),Zn、Pb含量差异有显著性(p<0.05);新建与戴村之间Cu、Zn含量差异有显著性;新建与蔡家湾之间,Mn、Fe含量差异有显著性;以上差异都是实验点(中洲、戴村、蔡家湾)高于对照点(新建)。Cd、Ni含量各点之间浓度值相近。对受试儿童身高、体重、胸围的调查结果表明,对照点均高于实验点。结果显示,重金属污染对乐安河流域儿童的健康可能造成不同程度的影响 相似文献
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Proton Events and X-ray Flares in the Last Three Solar Cycles 总被引:3,自引:0,他引:3
A database joining the available information about proton enhancements near the Earth and their possible solar sources is organized on the basis of proton measurements of the GOES and IMP-8 satellites, the data of neutron monitors, and GOES X-ray measurements. One thousand one hundred and forty-four proton events with energy > 10 MeV have been selected in the period from 1975 to 2003. More than a half of these events can be reliably related to X-ray solar flares. A statistical analysis shows the probability of observing solar protons near the Earth and their maximum flux value to be strongly dependent on the importance of a flare and its heliolongitude. Proton events are recorded after all suitably located (western) flares with X-ray importance > X5. The heliolongitude of a flare predetermines the character of the time profile of proton events in many respects. The relationship of proton events with the other characteristics of flares is established. The flares associated with proton enhancements are characterized by longer duration, slower rise to the X-ray maximum, smaller temperature, and larger length of the X-ray loops.__________Translated from Kosmicheskie Issledovaniya, Vol. 43, No. 3, 2005, pp. 171–185.Original Russian Text Copyright © 2005 by Belov, Garcia, Kurt, Mavromichalaki. 相似文献
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