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71.
为了提高全球定位系统(Global Positioning System,GPS)接收机的灵敏度,信号捕获过程需要加长积分时间。分析了比特跳变对加长相干积分时间的限制,从而提出一种能够完全避免比特符号跳变的捕获算法。该算法通过对多组数据采用相干积分和非相干积分相结合的方法,比较各组积分结果并选取积分最大值,用来判决是否捕获。算法中相干积分时间为19ms,目的是使积分最大值组完全避开数据位跳变,避免导航数据符号跳变对相干积分值的影响。该算法在避开比特跳变的基础上最大程度地提高相干积分时间,提高GPS接收机的捕获灵敏度。仿真结果表明,该算法能有效地捕获到载噪比(Carrier to Noise Rate,CNR)低至26dB·Hz的信号,可有效提高GPS接收机的捕获灵敏度。  相似文献   
72.
The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm2 sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5 full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm2 sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm2 sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm2 sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R S every 2–3 h (every ∼10 min from ∼20 R S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.  相似文献   
73.
为了研究螺栓孔的位置度误差对装配力学特性的影响,建立了考虑位置度误差的误差模型和有限元模型,研究了位置度误差对单个短精密螺栓连接结构的连接刚度和孔边应力的影响,建立了短精密螺栓组的位置度误差计算模型和有限元模型,分析了上、下被连接件的安装角度、第1颗螺栓的装人位置对短精密螺栓组结构的连接刚度的影响.研究发现:位置度误差...  相似文献   
74.
为了研究冲压发动机导弹爬升段和高空巡航段的燃油最优弹道,提高射程,提出了较为通用的一体化优化设计方法。研究了冲压发动机、导弹气动力与弹道之间的耦合特性,建立了导弹动力学模型,将弹道的最优控制问题转化为参数优化问题。为求解该参数优化问题,针对传统粒子群(PSO)算法求解优化问题时存在的早熟收敛的不足,提出了一种算法结构,改善粒子群算法的性能,求其最优解。数值结果表明:改进的算法相对其他几种粒子群算法具备更优秀的性能。所优化弹道相比导弹试验数据,以飞行时间增加3.3%为代价,节约了4.46%燃油。多组高弹道的仿真结果表明,巡航高度应不超过动压边界前提下,高弹道巡航有利于节约燃油,增加导弹射程。  相似文献   
75.
涡轮叶冠间隙流场PIV测量   总被引:1,自引:0,他引:1  
为了研究带有冷却气流的涡轮叶冠间隙流场流动特性,采用粒子图像测速仪(PIV)技术得到了叶冠间隙流场中各个典型截面的瞬时流场显示,并对叶冠间隙流场特性进行了研究.研究发现:由于叶冠腔内有两股叶尖冷却气流的注入,叶尖泄漏流流过叶冠间隙时会与两股冷却流相互掺混,从而使腔内气流的流动状态变得非常复杂,因此在叶冠突肩之后以及叶冠腔内流体汇合处会有大小方向各异的涡流产生.同时,两股冷却气流均对泄漏流有一定的阻挡作用,前孔冷却流的阻挡作用更为明显.随前孔与后孔岀流比增加,前孔流及后孔流对泄露流的阻挡作用增强.   相似文献   
76.
辅助动力装置喘振控制方法   总被引:15,自引:2,他引:15  
以带负载压气机的辅助动力装置(APU)为研究对象,分析了其引气工作特点及负载压气机喘振机理,提出采用出口换算流量小于最小稳定工作流量的方法来控制负载压气机稳定工作,当APU出口换算流量小于最小稳定工作流量2%时,通过打开喘振控制阀(SCV)防止APU喘振.设计了比例积分微分(PID)控制器控制SCV开度,试车数据与相同条件下的逼喘仿真试验结果对比表明,所提出的方法既可避免负载压气机喘振,又可保证出口压力满足引气要求.   相似文献   
77.
翼型表面结冰准定常数值模拟   总被引:2,自引:0,他引:2  
对翼型表面的结冰过程进行了准定常数值模拟。在每个时间步长内完成网格随着壁面边界的移动而更新、周围流场和水滴撞击特性重新计算、冰形计算及壁面边界的重构工作,如此循环直至所需的结冰计算时间。采用拉格朗日轨迹追踪法获得水滴撞击特性,应用考虑壁面粗糙度影响的边界层积分法计算壁面的对流换热系数,在此基础上求解Messinger结冰热力学模型,冰层始终沿壁面外法线方向生长。对NACA0012翼型在不同环境下生成的三种典型冰形进行了预测,并与实验结果进行了比较,表明本文所述方法的有效性。  相似文献   
78.
韩维  李成  商兴华 《飞机设计》2011,31(4):60-63
通过建立非线性模型对机群的完好率进行研究。针对完好飞机,重点研究飞行批次对完好率的影响;对于故障飞机,重点研究中修级维修和串件维修对修复率的影响,进而得出在基层级维修能力下机群满足总体完好率要求的持续时间。  相似文献   
79.
在搜索人数一定,用时最短的条件下,为了搜索完目标区域,根据搜索完区域的时间即为最后到达的人员所需时间,建立了最大最小化的规划模型,通过lingo程序,进行求解.并对划分的小矩形区域个数和队员人数也做了分类讨论.针对地面搜索问题进行了研究和讨论具有一定现实意义.  相似文献   
80.
New Horizons: Anticipated Scientific Investigations at the Pluto System   总被引:1,自引:0,他引:1  
The New Horizons spacecraft will achieve a wide range of measurement objectives at the Pluto system, including color and panchromatic maps, 1.25–2.50 micron spectral images for studying surface compositions, and measurements of Pluto’s atmosphere (temperatures, composition, hazes, and the escape rate). Additional measurement objectives include topography, surface temperatures, and the solar wind interaction. The fulfillment of these measurement objectives will broaden our understanding of the Pluto system, such as the origin of the Pluto system, the processes operating on the surface, the volatile transport cycle, and the energetics and chemistry of the atmosphere. The mission, payload, and strawman observing sequences have been designed to achieve the NASA-specified measurement objectives and maximize the science return. The planned observations at the Pluto system will extend our knowledge of other objects formed by giant impact (such as the Earth–moon), other objects formed in the outer solar system (such as comets and other icy dwarf planets), other bodies with surfaces in vapor-pressure equilibrium (such as Triton and Mars), and other bodies with N2:CH4 atmospheres (such as Titan, Triton, and the early Earth).  相似文献   
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