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81.
相控阵雷达搜索方式下波位编排与优化 总被引:1,自引:0,他引:1
分析不同波位编排方式对相控阵雷达能量需求与搜索性能的影响,给出了搜索方式下较为优化的波位编排方式。然后在分析相控阵雷达波束展宽效应的基础上,提出了非均匀划分扫描空域并对波束展宽效应进行补偿的方法,对波位编排方式进一步优化。最后利用该方法仿真分析了波束宽度与天线增益的变化,结果表明可有效补偿波束展宽效应带来的影响。 相似文献
82.
针对单发鸭式布局飞机,通过低速风洞试验,研究了矢量喷流对飞机大迎角气动力的影响特性。研究结果表明:发动机喷口直径变大使得飞机大迎角升力和阻力系数增加,并产生低头力矩系数。喷流使得飞机大迎角升力和阻力系数明显增加,并产生低头力矩系数;大喷口状态喷流影响比小喷口状态高50%左右。发动机喷管上/下偏转时,矢量喷流对飞机上下表面气流诱导不对称,喷管上偏减小升力和阻力系数、产生抬头力矩系数,喷管下偏增加升力和阻力系数、产生低头力矩系数,且喷管下偏影响明显比上偏大。在此基础上,基于数值模拟结果对喷流与飞机主流的相互作用机理进行了分析。 相似文献
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84.
The developing secondary flow fields in the entrance section of a rotating straight channel were experimentally investigated using Particle Image Velocimetry (PIV). The effects of streamwise position, Reynolds number and rotation number on the development of the secondary flow fields were revealed. The results show that the absolute values of vorticity flux of the trailing side roll cells increase with increasing radius of the measured plane and rotation number. When the absolute value of vorticity flux exceeds a critical value, the merging of the trailing side roll cells appears. Moreover, when the number of the trailing side vortex pairs is even, the absolute values of vorticity flux of the leading side vortices increase along streamwise direction. Otherwise, the absolute values decrease along the streamwise direction. By the circulation analysis, this phenomenon was found to have relationship with the merging of the trailing side roll cells, and further concluded that the secondary flow field in a rotating channel has to be treated as a whole. At last, the increase of the Reynolds number was found to be able to induce the merging position moves upstream. 相似文献
85.
针对光壁面超声速燃烧室的点火需求,利用中心嵌入式等离子体射流在模拟马赫数6,总温1860K的直连式试验台上实现了煤油燃料的可靠点火和稳定燃烧,研究了超声速燃烧室起动过程中等离子体建立与维持特征,获取了不同当量比下火焰传播与燃烧特性。试验表明:在自身工质的高压射流维持下,等离子体点火器可以在点火起动的不同压力变化环境中保持稳定;中心等离子体射流产生一定尺度的高温区域且含有丰富的自由基,但需要在恰当的中心喷油流量形成的混气当量比下产生等离子体诱导火焰;诱导火焰沿燃烧室轴向传播进而发展形成了稳定的超声速燃烧。 相似文献
86.
Flow Field Investigation in a Trapezoidal Duct with Swirl Flow Induced by Impingement Jets 总被引:1,自引:0,他引:1
LIU Haiyonga b QIANG Hongfua LIU Songlingb LIU Cunliangb a Section Xi’an High-Tech Institute Xi’an China bSchool of Power Energy Northwestern Polytechnical University Xi’an China 《中国航空学报》2011,24(1):8-17
An enlarged model of trapezoidal duct near the leading-edge in the blade is built up. The effects of impingement jets, swirl flow, cross flow and effusion flow are considered. Experiments are performed to measure flow fields in this confined passage and exit holes on one of its side walls. Cross flow and effusion flow are induced in the channel by the outflow of side exit hole (SEH) and film cooling hole (FCH), which are oriented on one end wall and bottom wall of the passage. Detailed flow structures are measured for two impingement angles of 35° and 45° with 6 combinations of outflow ratios. Results show that the small jets impinge the target wall effectively while the large jets contribute to inducing and impelling a strong counter-clockwise vortex in the upper part of the passage. Cross flow plays a dominate role for the flow structures in the passage and exit holes. It deflects jets, enhances swirl and deteriorates side exit conditions. Impingement angle is another significant factor for the flow characteristics. Its effect reveals more evidently with cross flow. Within the present test conditions, the mass flow rates and outflow positions of FCHs have no distinct effect on the main flow structures. 相似文献
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88.
非对称出口合成双射流激励器矢量特性实验研究 总被引:1,自引:0,他引:1
合成双射流(DSJ)激励器由于自身具有独特的矢量控制特性,为合成射流技术应用于主动流动控制提供了新途径。采用了基于射流核心区速度矢量的评价方法,并通过纹影和粒子图像测速法(PIV)流场显示实验研究了非对称出口压电式合成双射流激励器驱动参数(电压和频率)对射流矢量特性的影响。结果表明:合成双射流向出口面积大的一侧偏转,矢量偏转角随电压变化呈现先增大后减小的趋势,存在一个最佳驱动电压幅值,使得矢量偏转角最大;驱动频率变化对矢量偏转角的影响较显著,其对射流矢量的控制机理较复杂,实现矢量偏转角1.53°~36.65°可调,矢量偏转角出现两个峰值,且在振动膜共振频率处,矢量偏转角最小。 相似文献
89.
Stphane Corbel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2867-2871
Relativistic jets are now believed to be a fairly ubiquitous property of accreting compact objects, and are intimately coupled with the accretion history. Associated with rapid changes in the accretion states of the binary systems, ejections of relativistic plasma can be observed at radio frequencies on timescale of weeks before becoming undetectable. However, recent observations point to long term effects of these ejecta on the interstellar medium with the formation of large scale relativistic jets around binary systems. 相似文献
90.