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321.
飞机冲压空气涡轮系统的动态特性分析   总被引:3,自引:0,他引:3  
夏天翔  卢岳良  柯兵 《航空学报》2020,41(3):423242-423242
冲压空气涡轮是飞机能源失效时使用的关键应急系统。首先依据冲击空气涡轮(RAT)工作原理确定其物理架构;然后对涡轮部件、能源转换装置、展开装置和展开随动机构等4个主要部件进行力学分析,建立各部件的力学方程组。依据该力学方程组,建立涉及力学、液压、刚体动力学的多学科冲压空气涡轮系统模型。使用该模型仿真了某真实系统在不同工况和设计参数下的动态特性,研究了关键设计参数对系统性能的影响,为冲压空气涡轮系统正向设计提供依据。最终,某型冲压空气涡轮系统风洞试验数据验证了所提系统模型的准确性。  相似文献   
322.
为解决在高超声速脉冲风洞中进行大长细比等特殊模型测力实验所面临的惯性补偿问题,笔者提出了多加速度计振动分离惯性补偿方法。这一方法应用在长细比达20 :1 的模型气动力实验中,得到了较为理想的实验结果  相似文献   
323.
风洞模型投放试验轻模型法重力效应影响   总被引:1,自引:0,他引:1  
董金刚  谢峰  张晨凯  马汉东  秦永明 《航空学报》2020,41(6):523434-523434
风洞模型投放试验是研究超声速机弹分离问题的一种有效手段,相似参数的选取是影响试验准度的关键因素。有初始弹射速度的超声速机弹分离研究中,通常采用"轻模型法"得到模型的运动学及动力学相似参数,但该相似参数中模型重力模拟不足。为了研究重力效应对投放试验结果的影响,采用CTS试验技术对全尺寸真实参数与缩比尺寸轻模型法相似参数条件下得到的结果进行了对比研究。研究结果表明:在载弹与载机分离过程中,载弹位姿相互耦合,垂直下落位移的快慢会影响载弹姿态角的变化;轻模型法相似参数条件下,载弹垂直下落位移较慢,虚拟重力的修正方法只能近似修正下落位移,不能对导弹姿态角进行修正,而姿态角会影响下落的位移;机弹分离安全性方面,轻模型法相似参数条件下的试验结果较真实参数偏危险。  相似文献   
324.
飞机大迎角横侧气动特性是决定其机动性及敏捷性的主要因素之一。本文就采用机头边条改善飞机大迎角横侧气动特性进行了讨论。着重对机头边条的大小、安装位置等对飞机稳定性的影响进行讨论。试验是在气动中心低速所4m×3m和3.2m风洞中进行的。  相似文献   
325.
跨声速风洞斜孔壁非线性流动试验   总被引:1,自引:0,他引:1  
刘光远  张林  陈德华  林学东  贾智亮 《航空学报》2019,40(5):122497-122497
为分析跨声速风洞斜孔壁近壁区域的流动特性,评估气流偏角-压力系数的非线性关联,在0.6 m跨超声速风洞中开展了基于七孔探针的流动特性测量试验。通过气流偏角和压力系数分布分析了斜孔壁流动的差阻特性,以及马赫数、模型升力对斜孔壁流动的影响,最后基于试验结果发展了计算斜孔壁特性参数的微分法,并与经验方法结果进行对比。结果表明,斜孔壁流动呈现出明显的差阻性和非线性,在负压差范围内,近壁流动仍以出流为主;高亚声速时,空风洞模型区孔壁流动特性趋于实壁;安装模型后,随着升力的增大,升力面对应的孔壁区域流动向入流发展,孔壁流动特性趋于开口边界。  相似文献   
326.
战术导弹折叠翼两种展开方法及测试结果比较   总被引:1,自引:0,他引:1  
为了满足型号设计的需要,掌握战术导弹折叠尾翼在发射初始时的展开特性,对两种折叠翼快速展开的测试技术进行了试验研究。详细说明了两种测试方法的原理、测试量之间的比较、测试结果的分析。两种方案均在北京空气动力研究所(BIA)的一座低速风洞中进行了多次重复试验比较,测试结果表明两种方法均成熟可靠,可以用于战术导弹的实际设计中。  相似文献   
327.
A numerical model, based on Parker’s transport equation, describing the modulation of anomalous cosmic rays and containing diffusive shock acceleration is applied. The role of radial perpendicular diffusion at the solar wind termination shock, and as the dominant diffusion coefficient in the outer heliosphere, is studied, in particular the role it plays in the effectiveness of the acceleration of anomalous protons and helium when its latitude dependence is changed. It is found that the latitudinal enhancement of radial perpendicular diffusion towards the heliospheric poles and along the termination shock has a prominent effect on the acceleration of these particles. It results in a ‘break’ in the energy spectrum for anomalous protons at ∼6.0 MeV, causing the spectral index to change from E−1.38 to E−2.23, but for anomalous helium at ∼3.0 MeV, changing the spectral index from E−1.38 to E−2.30. When approaching the simulated TS, the changes in the modulated spectra as they unfold to a ‘steady’ power law shape at energies below 50 MeV are much less prominent as a function of radial distances when radial perpendicular diffusion is increased with heliolatitude.  相似文献   
328.
The results of modeling of ionospheric disturbances observed in the East Asian region during moderate storms are presented. The numerical model for ionosphere–plasmasphere coupling developed at the ISTP SB RAS is used to interpret the data of observations at ionospheric stations located in the longitudinal sector of 90–130°E at latitudes from auroral zone to equator. There is obtained a reasonable agreement between measurements and modeling results for winter and equinox. In the summer ionosphere, at the background of high ionization by the solar EUV radiation in the quiet geomagnetic period the meridional thermospheric wind strongly impacts the electron concentration in the middle and auroral ionosphere. The consistent calculations of the thermospheric wind permit to obtain the model results which are closer to summer observations. The actual information about the space-time variations of thermosphere and magnetosphere parameters should be taken into account during storms.  相似文献   
329.
The question of multifractality is of great importance because it allows us to investigate interplanetary hydromagnetic turbulence. The multifractal spectrum has been investigated with Voyager (magnetic field) data in the outer heliosphere and with Helios (plasma) data in the inner heliosphere. We use the Grassberger and Procaccia method that allows calculation of the generalized dimensions of the solar wind attractor in the phase space directly from the cleaned experimental signal. We analyze time series of plasma parameters of the low-speed streams of the solar wind measured in situ by Helios in the inner heliosphere. The resulting spectrum of dimensions shows a multifractal structure of the solar wind attractor. In order to quantify that multifractality, we use a simple analytical model of the dynamical system. Namely, we consider the generalized self-similar baker’s map with two parameters describing uniform compression and natural invariant measure on the attractor of the system. The action of this map exhibits stretching and folding properties leading to sensitive dependence on initial conditions. The obtained solar wind singularity spectrum is consistent with that for the multifractal measure on the weighted baker’s map.  相似文献   
330.
Feng  Xueshang  Wu  S.T.  Wei  Fengsi  Fan  Quanlin 《Space Science Reviews》2003,107(1-2):43-53
It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   
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