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71.
袁干 《南京航空航天大学学报》1989,(2)
本文主要介绍一种新型脉冲雷达高度表,装于CK1E超低空靶机模型上静态测高的试验方法和结果。结果分析表明该高度表适用于CK1E靶机的飞行控制系统,作为高度传感器,在超低空进行精确而稳定的测高成功。 相似文献
72.
为了对航空公司混合渠道进行更有效协调,根据渠道协调特点,运用区间分析法构建了需求不确定情况下航空公司混合渠道协调的模糊规划模型,并对模型进行了多维度数值模拟.结果表明,模型对不确定需求具有鲁棒性,适用于需求不确定下航空公司混合渠道协调;随着分销渠道比例下降,渠道协调鲁棒性呈现先升后降趋势;随着需求区间变大,模糊规划模型的隶属度呈现下降趋势.因此航空公司应适当降低分销渠道比例,同时加强市场调查缩小机票需求不确定区间范围;代理人应选择代理销售需求不确定性低的机票产品,并与航空公司合作适当降低分销渠道比例从而获得鲁棒双赢策略. 相似文献
73.
某型直升机装备的两超短波电台在使用中出现某些频点下的互相干扰现象,尽管地面采取了相应措施却均未改善。本文在常规修理方法的基础上,采用了一些新方法找到了此故障的根源,并为类似电台干扰问题提供参考。 相似文献
74.
雷达-电子战-通信的一体化 总被引:11,自引:0,他引:11
为充分发挥武器系统的作战效能,对作战平台上的雷达-电子战-通信一体化技术进行了研究。阐述了雷达与电子战、雷达与通信一体化的必要性和特点,并对一体化的关键技术,如以线性调频与伪随机编码信号的组合为共用信号、共用孔径及其波束控制技术等进行了分析。最后给出了一个采用软件无线电技术的雷达-无线电-通信一体化系统的方案。 相似文献
75.
76.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(5):2521-2533
We have analysed energetic storm particle (ESP) events in 116 interplanetary (IP) shocks driven by front-side full and partial halo coronal mass ejections (CMEs) with speeds 400 km s?1during the years 1996–2015. We investigated the occurrence and relationships of ESP events with several parameters describing the IP shocks, and the associated CMEs, type II radio bursts, and solar energetic particle (SEP) events. Most of the shocks (57 %) were associated with an ESP event at proton energies 1 MeV.The shock transit speeds from the Sun to 1 AU of the shocks associated with an ESP event were significantly greater than those of the shocks without an ESP event, and best distinguished these two groups of shocks from each other. The occurrence and maximum intensity of the ESP events also had the strongest dependence on the shock transit speed compared to the other parameters investigated. The correlation coefficient between ESP peak intensities and shock transit speeds was highest (0.73 0.04) at 6.2 MeV. Weaker dependences were found on the shock speed at 1 AU, Alfvénic and magnetosonic Mach numbers, shock compression ratio, and CME speed. On average all these parameters were significantly different for shocks capable to accelerate ESPs compared to shocks not associated with ESPs, while the differences in the shock normal angle and in the width and longitude of the CMEs were insignificant.The CME-driven shocks producing energetic decametric–hectometric (DH) type II radio bursts and high-intensity SEP events proved to produce also more frequently ESP events with larger particle flux enhancements than other shocks. Together with the shock transit speed, the characteristics of solar DH type II radio bursts and SEP events play an important role in the occurrence and maximum intensity of ESP events at 1 AU. 相似文献
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A novel architecture for computing the fast Fourier transform ( FFT ) on programmable devices is presented.To improve the system operation speed , a hybrid parallel FFT algorithm is used.Results indicate that the use of an 8×8parallel structure for realizing the 64-point FFT leads to a 8times higher processing speed compared with its counterparts employing other series of techniques. 相似文献
80.
S.S. Nikte A.K. Sharma D.P. Nade M.V. Rokade R.N. Ghodpage P.T. Patil R.V. Bhonsle 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
A dual dipole antenna has been installed at low latitude station Kolhapur (Geographic 16.8°N, 74.25°E), Maharashtra, India for the study of cosmic radio noise absorption using Solid State Riometer (which operates at 30 MHz) during pre phase of 24th solar maxima. The aim for this type of study over Kolhapur was to know the response of lower (D region) ionosphere over low latitude by cosmic radio noise absorption using riometer technique during quite period as well as sudden ionospheric disturbances (SID). The observations are being taken for 3 years. Two different sites (∼40 km away from each other) were used for the installation of riometer equipment assuming minimum local noise. It is found that solar noise to cosmic radio noise hence resulting in signal saturation. The night time signal is relatively free of interference but sometimes local noise is responsible for spike-like signatures. Hence it is concluded that Kolhapur (a low latitude station) is not suitable for the study of cosmic radio noise absorption on 30 MHz with riometer and dual dipole antenna. Proper choice for operating frequency of riometer and antenna gain is suggested for low latitude use of this technique for ionospheric deviative and nondeviative absorption studies. 相似文献