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81.
高焓激波风洞喷管流场非平衡特性研究 总被引:1,自引:0,他引:1
高焓激波风洞是开展高超声速流动研究的重要地面模拟设备,但其产生的高焓气流在喷管中的膨胀过程是一种典型的热化学非平衡流动,试验段特征参数通过直接实验测量难以完全确定。本文通过求解耦合双温度模型的轴对称Navier-Stokes方程,研究了高焓激波风洞中典型状态下气流的热化学非平衡流动特性,分析了焓值对非平衡特性的影响规律。结果表明,喷管出口自由流均匀区域达到出口截面直径的75%以上,能够为实验提供足够的空间;喷管出口自由流处于热化学非平衡状态,在喷管喉道后约1/5喷管长度处气流即已处于冻结流状态,组分浓度和振动温度随气流流动基本不变;焓值在8.4MJ/kg~19.5MJ/kg之间变化时,非平衡程度随着焓值的增加而增强,但是低焓值时非平衡程度的增强更加剧烈。 相似文献
82.
This paper presents the novel use of the particle swarm optimization(PSO)to generate the end-to-end trajectory for hypersonic reentry vehicles in a quite simple formulation.The velocitydependent bank angle profile is developed to reduce the search space of unknown parameters based on the constrained PSO algorithm.The path constraints are enforced by setting the fitness function to be infinite on condition that the particles violate the maximum allowable values.The PSO algorithm also provides a much easier means to satisfy the terminal conditions by adding penalty terms to the fitness function.Furthermore,the approximate reentry landing footprint is fast constructed by incorporating an interpolation model into the standardized bank angle profiles.Numerical simulations demonstrate that the PSO method is a feasible and flexible tool to generate the end-to-end trajectory and landing footprint for hypersonic reentry vehicles. 相似文献
83.
某型机18框上半框零件由于外形结构尺寸大、多腔,数控加工过程中零件变形大,加工质量不易保证。该零件经首件数控试切及鉴定,零件尺寸精度、表面质量符合设计图纸及装配要求,通过使用hypermill编程软件,编程效率得到极大的提高,缩短了零件的生产周期。 相似文献
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J. Smolinski J. L. Climenhaga Y. Huang Sh. Jiang M. Schmidt O. Stahl 《Space Science Reviews》1993,66(1-4):231-236
The profiles of H observed during the 1970–1992 period in the binary hypergiant HR 8752 (G0 Ia) are presented. We distinguish five typical H profiles designated as A, B, C, D and E types according to the number of emission and absorption features. The profiles of H are complex and contain several emission and absorption components, with: –130 km/s in emission or absorption, –84 km/s in absorption, –49 km/s in emission and about +6 km/s in emission. All of them are rather stable in radial velocities except of the main absorption component in the P Cygni profile with –84 km/s. The frequency of appearance and the periods of duration of the occurrence of the components is discussed. The duration times range between about 3 to 10 months for various components. The red emission component E2 is particularly interesting. Possible explanations of its origin are discussed.A long-term acceleration of the absorption component in the P Cygni profile is found; it can be interpreted as monotonous acceleration of the stellar wind. 相似文献
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Aerodynamic optimization design for high pressure turbines based on the adjoint approach 总被引:1,自引:1,他引:1
A first study on the continuous adjoint formulation for aerodynamic optimization design of high pressure turbines based on S2surface governed by the Euler equations with source terms is presented.The objective function is defined as an integral function along the boundaries,and the adjoint equations and the boundary conditions are derived by introducing the adjoint variable vectors.The gradient expression of the objective function then includes only the terms related to physical shape variations.The numerical solution of the adjoint equation is conducted by a finitedifference method with the Jameson spatial scheme employing the first and the third order dissipative fluxes.A gradient-based aerodynamic optimization system is established by integrating the blade stagger angles,the stacking lines and the passage perturbation parameterization with the quasi-Newton method of Broyden–Fletcher–Goldfarb–Shanno(BFGS).The application of the continuous adjoint method is validated through a single stage high pressure turbine optimization case.The adiabatic efficiency increases from 0.8875 to 0.8931,whilst the mass flow rate and the pressure ratio remain almost unchanged.The optimization design is shown to reduce the passage vortex loss as well as the mixing loss due to the cooling air injection. 相似文献
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