首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   3612篇
  免费   219篇
  国内免费   30篇
航空   1782篇
航天技术   1351篇
综合类   77篇
航天   651篇
  2022年   27篇
  2021年   42篇
  2019年   25篇
  2018年   55篇
  2017年   65篇
  2016年   44篇
  2015年   38篇
  2014年   77篇
  2013年   103篇
  2012年   87篇
  2011年   164篇
  2010年   115篇
  2009年   142篇
  2008年   208篇
  2007年   116篇
  2006年   109篇
  2005年   116篇
  2004年   80篇
  2003年   117篇
  2002年   90篇
  2001年   104篇
  2000年   88篇
  1999年   102篇
  1998年   107篇
  1997年   101篇
  1996年   88篇
  1995年   105篇
  1994年   109篇
  1993年   64篇
  1992年   76篇
  1991年   40篇
  1990年   47篇
  1989年   74篇
  1988年   39篇
  1987年   32篇
  1986年   34篇
  1985年   114篇
  1984年   79篇
  1983年   79篇
  1982年   60篇
  1981年   103篇
  1980年   25篇
  1979年   27篇
  1978年   33篇
  1977年   25篇
  1976年   23篇
  1975年   39篇
  1972年   33篇
  1971年   25篇
  1967年   23篇
排序方式: 共有3861条查询结果,搜索用时 0 毫秒
761.
分析了小卫星的姿态动力学及运动学方程;利用姿态动力学方程为一动力学参数矢量的线性函数这一事实,考虑存在参数不确定性,提出了一种自适应控制方法;证明了这种方法可以保证控制系统全局渐近稳定。仿真结果验证了该方法的有效性。  相似文献   
762.
Tether Satellite System Collision Study   总被引:1,自引:0,他引:1  
Chobotov  V.A.  Mains  D.L. 《Space Debris》1999,1(2):99-112
A study was performed to determine the probability of collision with resident space objects and untrackable debris for the tether component of the Tethered Satellite System (TSS) after it broke away from the Space Shuttle orbiter (mission STS-75) in February 1996. Both an analytical and a numerical approach were used in this study, and the results obtained with these two methods were found to be in good agreement. These results show that the deployed tether is expected to have been impacted by several particles 0.1mm or larger in size. The probability of collision with objects 10cm in size or larger was on the order of 10–3 per month. Since the severed tether reentered within one month after deployment, the collision hazard to other objects while in orbit was small. The analytical methods used in this study are useful for tether collision evaluations in general.  相似文献   
763.
遗传算法在电子战干扰规划中的应用   总被引:3,自引:1,他引:3       下载免费PDF全文
电子对抗干扰资源任务规划问题对于充分发挥干扰机作战效能,取得最佳干扰效益有重要作用.结合现代电子战特点,利用搜索论推导出了干扰机压制概率的计算公式,建立了干扰任务分配模型,并阐述了传统匈牙利方法在这一问题处理上的局限性.结合智能优化算法,提出了基于遗传算法的干扰资源优化分配模型.解决了优化分配模型所需的符号编码方式,并给出了相关的选择、交叉、变异等遗传算子的具体设计.利用该模型,解决了2个实例.结果表明,该模型在干扰资源任务配置问题上具有很强的实用性,遗传算法可以有效地辅助指挥员解决干扰资源部署决策这一复杂而困难的问题.  相似文献   
764.
    
We present the results of processing three 256-min series of observations of quasi-periodic oscillations of the field of line-of-sight velocities in three sunspots. The Doppler shifts were determined simultaneously for six spectral lines formed at different heights in the solar atmosphere. In addition to the well-known high-frequency (periods of 3–5 min) oscillations, a band of low-frequency oscillations with periods of 60–80 min is revealed in the spectra of the sunspot umbra and magnetic elements located in immediate proximity of the sunspot. Unlike the short-period modes, the power of the long-period mode of line-of-sight velocity oscillations in the sunspot decreases sharply with height: these oscillations are distinctly seen in the line formed at a height of 200 km and almost are not seen in the line with the formation height of 500 km. This is indicative of different physical nature of the short-period and long-period oscillations of a sunspot. If the former are caused by slow magnetosonic waves within the field tube of the spot, the latter are representative of global vertical-radial oscillations of a magnetic element (spot, pore) as a whole near the position of a stable equilibrium.  相似文献   
765.
We present new measurements concerning generation of light flash during hypervelocity impacts. We use iron particles (10−13 to 10−17 kg) with velocities over the range 1 to 42 km/s impacting semi-infinite targets (aluminium and molybdenum). The main results of previous work in the field are found to be reproduced with some slight deviations. For iron projectiles with given mass and velocity the energy of the flash (normalized to mass) is proportional to velocity to the power of 3.5 for aluminium targets and 3.9 for molybdenum targets. The duration of the flash is of order 1 microsecond. Simultaneous measurements of the generation of impact plasma do not change this. The onset of plasma generation of the bulk target material does not affect the total light flash energy. We discuss the duration of the flash compared to a simple calculation of temperature in the target and plasma vs time.  相似文献   
766.
Alfvn waves are found to be ubiquitous in the solar wind.Recent progress in observational studies of the waves is reviewed to formulate a microscopic picture for the Alfvenic fluctuations. The main aspects of the observational properties of these waves,including the wave intervals, propagation,evolution,origin and generation,are presented.Then Alfven wave heating and acceleration of the solar wind plasma are briefly introduced.The relation of the waves to rotational and tangential discontinuities,magnetic decreases,and other relatively large-scale structures such as flux tubes/ropes,magnetic clouds and interplanetary coronal mass ejections in the solar wind is particularly investigated.Finally,some remaining open questions are also indicated due to their fundamental importance of understanding of the physical nature of Alfven waves and the role of the waves in heating and accelerating the solar wind.  相似文献   
767.
考虑卫星本体表面包覆绝热材料的实际物理状态,根据数值传热学和有限容积法建立了目标表面温度场和红外辐射计算模型.建立卫星结构模型,基于热控涂层性能退化,提出红外辐射灵敏度概念,并建立了卫星红外辐射灵敏度计算模型.对在轨飞行卫星的瞬态温度场进行数值模拟,与遥测数据对比分析.最后,分析了空间卫星的红外辐射和红外辐射灵敏度.结...  相似文献   
768.
    
A database of electron temperature (Te) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature Te at different latitudes, altitudes, local times and seasons. The Te data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general Te changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, Te increases with increasing solar activity. But this increase is not linear as assumed in most empirical Te models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward.  相似文献   
769.
Red-cell mass determinations were performed before and after the first two Skylab missions. The data showed a 14% mean decrease in red-cell mass after the 28-day mission and a 12% mean decrease after the 59-day mission. The red-cell mass returned to premission levels more slowly after the shorter (28-day) than after the longer mission. Plasma volume decreases were found after each mission. with the crew from the longer mission showing the greater change (13% vs. 8.4%). Postmission decreases in red-cell mass and plasma volume have been a general finding in crewmen who return from short or long spaceflight.  相似文献   
770.
航空声学风洞的声学设计研究   总被引:1,自引:0,他引:1  
随着航空运输业的发展,飞机的噪声问题日益引起人们的关注.开展航空声学试验研究的地面试验设备主要是航空声学风洞.笔者阐述了航空声学风洞声学设计的基本要求、应考虑的主要问题,提出了航空声学风洞声学设计的方法等.并将这些研究成果应用于引导风洞研制中,得到了在开口试验段风速80m/s时,气流外2m测点处背景噪声76.5dB(A)的结果.  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号