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351.
本文讨论了一种新型永磁无刷直流发电机的构成和工作原理,并指出稀土永磁方波电机与工作于方波方式的升压型功率变换器协调工作,是实现最佳配合的一种新方案.文中还详细分析了该电机的特性:输出电压U_0、导通比D_y、输入电流I_i与转速n的关系;输出电压的脉动△u_0、输入电流的脉动△I_i、外特性和效率。样机实验表明,分析是正确的。 电力电子器件的发展,将日益显示这种新型电机的生命力。我国稀土资源丰富,发展稀土电机有广阔的前景,稀土电机的发展与电力电子变换器的发展关系十分密切.本文就是从两者的结合方面进行分析讨论的。为机电一体化电机的开发和设计提供了理论和技术基础。 相似文献
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353.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(4):1915-1921
This paper presents the results of the analysis of the evolution of coronal holes (CHs) on the Sun during the period May 13, 2010 – March 20, 2022, covering Solar Cycle 24. Our study uses images in the extreme-ultraviolet iron line (Fe XII 193 Å) obtained with the Atmospheric Imager Assembly of the Solar Dynamics Observatory (AIA/SDO). To localize CHs and determine their areas, we used the Heliophysics Event Knowledgebase (HEK). We separate the CHs into polar and non-polar and study the evolutionary features of each group. During this period, an asymmetry between the Northern (N) and Southern (S) Hemispheres (N-S or hemispheric asymmetry) is detected both in the solar activity (SA) indices and in the localization of the maximum areas of the polar and non-polar CHs. It is shown that the hemispheric asymmetry of the areas of polar and non-polar CHs varies significantly over time and that the nature of these changes is clearly related to the SA cycle. We find that for most of the period, the polar CHs were predominated generated in the S- hemisphere while the non-polar CHs were dominant in the N- hemisphere. It is found that the maximum and minimum of the hemispheric imbalance in the areas of non-polar CHs are close in time to the maximum and minimum of the asymmetry of the SA indices (the number and areas of sunspots). The maximum hemispheric imbalance of the polar CH areas is observed at the maximum of Cycle 24, and the minimum imbalance is found at the cycle minimum. These results confirm our assumption that these two types of CHs are of a different nature and that the non-polar CHs, like sunspots, are elements of the general magnetic activity. 相似文献
354.
H.S. Sawant J.R. Cecatto H. Mészárosová C. Faria F.C.R. Fernandes M. Karlický M.C. de Andrade 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The digital, decimetric (950–2500 MHz) Brazilian Solar Spectroscope (BSS, Sawant, H.S., Subramanian, K.R., Faria, C., et al. Brazilian Solar Spectroscope (BSS). Solar Phys. 200, 167–176, 2001) with high time (10–1000 ms) and frequency (1–10 MHz) resolution is in regular operation since April, 1998, at the National Space Research Institute (INPE) at São José dos Campos, Brazil. The BSS has now been upgraded with a new digital data acquisition and data processing system. The new version of the BSS has improved the observational possibilities with the capability to record up to 200 frequency channels available in the selectable frequency range 950–2500 MHz. The GPS receiver permits the acquisition of data with time accuracy in the order of 0.1 ms. The software system of the BSS is composed by two distinct modules: the first, data acquisition system provides a flexible Graphical User Interface (GUI) that allows one to choose the observational parameters. The second module is the real time visualization system that permits real time visualization of the observed dynamic spectrum and additionally allows procedures for visualization and preliminary analysis of the recorded solar spectra. Using the new visualization system, we have realized two new types of dm-radio fine structures: narrow band type III bursts with positive as well as negative group frequency drift and dots emissions arranged in zebra-like and fiber-like chains. Furthermore, we have found flare generated fast wave trains according to their tadpole signature in wavelet power spectra for a decimetric type IV radio event (June 6, 2000 flare). 相似文献
355.
设计了由陀螺、GPS姿态敏感器、红外地平仪和太阳敏感器构成的太阳同步极轨卫星姿态确定系统。提出联邦滤波器结构和算法,推导了各子系统的量测方程和姿态确定系统的误差状态方程。为规避对量测值进行非相关处理,采用减小GPS姿态敏感器输出的姿态滤波值作为系统滤波器量测值的频率的方法。仿真结果表明,采用联邦滤波器对多敏感器卫星姿态确定系统进行信息融合,具有计算量小、精度高、可靠性好等优点。 相似文献
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357.
Janusz Nicewicz Grzegorz Michalek 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Space weather is significantly controlled by halo coronal mass ejections (HCMEs) originating close to the central meridian and directing toward the Earth. Unfortunately, coronagraphic observations (especially for HCMEs) are subject to a projection effect which makes it impossible to determine the true radial velocity and width of CMEs. However, these parameters can be estimated by correcting for the projection effect using the asymmetric cone model (Michalek, 2006). A set of 20 CMEs, observed as halo events in the LASCO field of view and simultaneously as limb events in the STEREO/SECCHI field of view, are used to check the accuracy of the asymmetric cone model. For this purpose, characteristics of the considered CMEs (angular widths and radial speeds) measured in STEREO/SECCHI images are compared with those obtained by the asymmetric cone model. We demonstrate that the widths and speeds determined by both methods are very similar. Correlation coefficients for speeds and angular widths are 0.99 and 0.96, respectively. We have also shown that the projection effect is unpredictable and could sometimes be very significant (up to 100% of the velocity measured in the LASCO field of view). On average, the SOHO/LASCO projected speeds for the HCMEs are 23% smaller than the radial velocities obtained from the STEREO/SECCHI images. 相似文献
358.
传统中小功率十二相整流型同步发电机电压等级较低,整流装置通常采用4套不控整流单元并联结构。随着舰船中压直流综合电力技术的发展,整流发电系统的容量和电压等级大幅提升,十二相整流单元采用两并两串的拓扑结构可以适应发电机绕组较高的电压设计值,同时整流端中性线可引出用于电力推进调速装置的均压控制。分析了两并两串拓扑结构的不同联接组合型式,重点对两种可行的拓扑结构下的直流侧电压波形进行了解析计算,并通过仿真与试验验证了理论分析的正确性,证明了(Y1//Y3)+(Y2//Y4)拓扑结构为最优组合方式,具有最佳的直流电压品质。 相似文献
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