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271.
《中国航空学报》2021,34(5):163-182
Hot compressive experiments of the laser solid formed (LSFed) TC4 titanium alloy were conducted at a wide temperature range of 650–950 °C and strain rate of 0.01–10 s−1. The Arrhenius-type constitutive models of the LSFed TC4 alloy were established at the temperature range of 800–950 °C and of 650–800 °C, respectively. The average relative error between the predicted stresses and experimental values in those two temperature ranges are 10.4% and 8.3%, respectively, indicating that the prediction models constructed in this paper are in a good agreement with experimental data. Processing maps were established by the principle of dynamic materials modeling on the basis of the data achieved from the hot compression experiments. The processing parameters corresponding to the stable and unstable regions of material deformation can be determined from the processing maps. The microstructure evolution of the stable and unstable regions of the samples after tests were observed. Finally, the effect of hot compressive parameters on the microstructure were investigated to research the dynamic recrystallization and the texture of the deformed LSFed TC4 alloy.  相似文献   
272.
由于盘铣刀具直径大,切削余量大,造成钛合金盘铣开槽过程中铣削力较大,进而引起刀具振动,缩短刀具寿命。为实现对钛合金盘铣开槽过程的优化与控制,本文设计单因素实验和正交实验,利用三向压电式测力仪测量铣削力数据,采用线性回归技术建立铣削力模型并以“F”检验法对模型进行显著性检验;利用极差分析法分析工艺参数对铣削力的影响规律,利用响应曲面法分析工艺参数对铣削力的交互影响规律。研究结果表明:对于切削深度变化敏感度依次为铣削力Fx>进给速度>主轴转速;对于进给速度变化敏感度依次为铣削力Fy>切削深度>主轴转速;对于铣削力Fz变化敏感度依次为主轴转速>切削深度。铣削力随着主轴转速的增大而减小,随着切削深度和进给速度的增大而增大。另外铣削力Fx大于FyFz,对加工性能和刀具磨损起主导作用。  相似文献   
273.
We report the results of ionospheric measurements from DPS-4 installed at Multan (Geog coord. 30.18°N, 71.48°E, dip 47.4°). The variations in F2-layer maximum electron density NmF2 and its peak height hmF2 are studied during the deep solar minimum between cycles 23 & 24 i.e 2008–2009 with comparisons conducted with the International Reference Ionosphere (IRI) versions 2012 & 2016. We find that the hmF2 observations peak around the pre-sunrise and sunrise hours depending on the month. Seasonally, the daytime variation of NmF2 is higher in the Equinox and Summer, while daytime hmF2 are slightly higher in the Equinox and Winter. High values of hmF2 around midnight are caused by an increase of upward drifts produced by meridional winds. The ionosphere over Multan, which lies at the verge of low and mid latitude, is affected by both E×B drifts and thermospheric winds as evident from mid-night peaks and near-sunrise dips in hmF2. The results of the comparison of the observed NmF2 and hmF2 for the year 2008–2009 with the IRI-2012 (both NmF2 and hmF2) and IRI-2016 (only hmF2) estimates indicate that for NmF2, IRI-2012 with Consultative Committee International Radio (CCIR) option produces values in better agreement with observed data. Whereas, for hmF2, IRI-2016 with both International Union of Radio Science (URSI) and CCIR SHU-2015 options, predicts well for nighttime hours throughout the year. However, the IRI-2012 with CCIR option produces better agreement with data during daytime hours. Furthermore, IRI-2012 with CCIR option gives better results during Equinox months, whereas, IRI-2016 with both URSI and CCIR SHU-2015 options predict well for Winter and Summer.  相似文献   
274.
LOX/LCH_4变推力发动机技术初步研究   总被引:2,自引:1,他引:1  
对国内外变推力发动机和LOX/LCH4发动机的研究进展进行了总结,在此基础上,提出了一种LOX/LCH4变推力发动机系统方案。在深入分析的基础上,对此方案进行了功率平衡和推力室传热计算,结果表明该系统方案完全能够实现10:1推力变比。LOX/LCH4变推力发动机可以广泛应用于多种运载器和航天器中,对我国探月及后续的载人登月工程均可以提供技术支持,对LOX/LCH4发动机的技术发展和未来的载人登陆火星等任务都具有深远影响。  相似文献   
275.
袁经纬  李卓  汤海波  程序 《航空学报》2021,42(10):524390-524390
随着钛合金装备在航空、航天、航海等领域的使用逐渐增多,其服役环境日益严苛,对构件材料的抗腐蚀性能及室温应力蠕变性能提出了更高要求。针对钛合金耐蚀性及抗压缩蠕变的性能,分析了激光增材制造TC4合金不同热处理状态试样电化学及室温压缩蠕变性能,并结合蠕变曲线修正了蠕变第Ⅰ阶段本构方程的参数。结果表明,双重退火处理会显著减小增材制造TC4钛合金中α板条长径比与尺寸,而固溶时效可使α板条长径比增大、尺寸减小,导致了材料耐蚀性、屈服极限以及抗压缩蠕变性能的变化。沉积态合金经过固溶时效后自腐蚀电流降低64.92%,稳态蠕变应变率降低46.31%,蠕变应变降低50%。而经过双重退火后合金自腐蚀电流降低26.14%,稳态蠕变应变率提升111.20%,蠕变应变提升48.68%。相比于铸锻工艺制备TC4合金蠕变本构方程,修正后的拟合系数与蠕变曲线吻合度更高。  相似文献   
276.
针对极低温吸附制冷技术的热沉制冷系统,系统分析了极低温吸附制冷的特性,研究了热沉温度对极低温吸附制冷性能的影响,研制了一台极低温吸附制冷机样机,工质气体为氦4,在1.5W@4.2K G-M制冷机基础上实现了50μW@0.8K的制冷性能,验证了基于机械制冷系统的更高热沉温度技术的可行性,这一成果为深空探测和载人空间站相关研究提供了技术支撑。  相似文献   
277.
《中国航空学报》2021,34(8):112-121
Uniaxial ratcheting behaviour and low cycle fatigue (LCF) failure mechanism of nickel-based single crystal superalloy DD6 with [001] orientation are investigated through the stress-controlled LCF tests with stress ratio of −1. Then the deformation behaviour during the whole-lifetime from the beginning of the experiment to the fracture of the specimen, as well as the fractographic/metallographic morphology, are compared with the strain-controlled LCF experimental results. Through the scanning electron microscope (SEM) observations, it is shown that the failure characteristics under stress-controlled LCF loading are similar with those under strain-controlled loading. Nevertheless, unlike strain-controlled LCF loading, even under fully reversed cycle loading for stress-controlled LCF, DD6 shows significant ratcheting behaviour due to the tension-compression asymmetry. In addition, the LCF lifetimes under stress control are significantly shorter than the LCF lifetimes under strain control, and the culprit might be the detrimental effect of ratcheting strain on LCF lifetime. Based on these phenomena, an improved crystal plasticity constitutive model on the basis of slip-based Walker constitutive model is developed through modifying the kinematic hardening rule in order to overcome the inaccurate prediction of decelerating stage and stable stage of ratcheting behaviour. Furthermore, combining the continuum damage mechanics, a damage-coupled crystal plasticity constitutive model is proposed to reflect the damage behaviour of DD6 and the accelerating stage of ratcheting behaviour. The simulation results for the stress-controlled LCF deformation behaviour including the whole-lifetime ratcheting behaviour show good agreement with the experimental data.  相似文献   
278.
In this paper, optimal trajectories of a spacecraft traveling from Earth to Moon using impulsive maneuvers (ΔV maneuvers) are investigated. The total flight time and the summation of impulsive maneuvers ΔV are the objective functions to be minimized. The main celestial bodies influencing the motion of the spacecraft in this journey are Sun, Earth and Moon. Therefore, a three-dimensional restricted four-body problem (R4BP) model is utilized to represent the motion of the spacecraft in the gravitational field of these celestial bodies. The total ΔV of the maneuvers is minimized by eliminating the ΔV required for capturing the spacecraft by Moon. In this regard, only a mid-course impulsive maneuver is utilized for Moon ballistic capture. To achieve such trajectories, the optimization problem is parameterized with respect to the orbital elements of the ballistic capture orbits around Moon, the arrival date and a mid-course maneuver time. The equations of motion are solved backward in time with three impulsive maneuvers up to a specified low Earth parking orbit. The results show high potential and capability of this type of parameterization in finding several Pareto-optimal trajectories. Using the non-dominated sorting genetic algorithm with crowding distance sorting (NSGA-II) for the resulting multiobjective optimization problem, several trajectories are discovered. The resulting trajectories of the presented scheme permit alternative trade-off studies by designers incorporating higher level information and mission priorities.  相似文献   
279.
S4R功率调节技术在航天器上的仿真研究与实现   总被引:1,自引:1,他引:0  
雷卫军  李言俊 《宇航学报》2008,29(3):977-982
对于大功率母线的航天器,传统的母线功率调节技术因为诸多缺点已经不能适应母线功率不断增大的要求。S4R作为一种新型的卫星母线调节技术能够很好的控制母线电压,同时具有优良的电池充、放电特性和很高的效率。在对国、内外S4R技术研究的基础上,从S4R的工作原理出发,给出了S4R功率调节技术的实现策略。在此基础上进行了实际电路的仿真分析,最后给出了部分实际的工作波形.并展望了其应用前景。  相似文献   
280.
Recent papers have suggested that the slow solar wind is a super-position of material which is released by reconnection from large coronal loops. This reconnection process is driven by large-scale motions of solar magnetic flux driven by the non-radial expansion of the solar wind from the differentially rotating photosphere into more rigidly rotating coronal holes. The elemental composition of the slow solar wind material is observed to be fractionated and more variable than the fast solar wind from coronal holes. Recently, it has also been reported that fractionation also occurs in 3He/4He. This may be interpreted in the frame-work of an existing model for fractionation on large coronal loops in which wave-particle interactions preferentially heat ions thereby modifying their scale-heights. This revised version was published online in June 2006 with corrections to the Cover Date.  相似文献   
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