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   2896篇
  免费   588篇
  国内免费   639篇
航空   2558篇
航天技术   548篇
综合类   420篇
航天   597篇
  2024年   7篇
  2023年   69篇
  2022年   98篇
  2021年   156篇
  2020年   148篇
  2019年   144篇
  2018年   154篇
  2017年   188篇
  2016年   199篇
  2015年   171篇
  2014年   218篇
  2013年   175篇
  2012年   216篇
  2011年   232篇
  2010年   170篇
  2009年   184篇
  2008年   163篇
  2007年   182篇
  2006年   184篇
  2005年   132篇
  2004年   84篇
  2003年   129篇
  2002年   99篇
  2001年   85篇
  2000年   66篇
  1999年   62篇
  1998年   58篇
  1997年   72篇
  1996年   57篇
  1995年   37篇
  1994年   52篇
  1993年   26篇
  1992年   23篇
  1991年   26篇
  1990年   17篇
  1989年   22篇
  1988年   16篇
  1984年   2篇
排序方式: 共有4123条查询结果,搜索用时 890 毫秒
881.
The electron density profiles in the bottomside F2-layer ionosphere are described by the thickness parameter B0 and the shape parameter B1 in the International Reference Ionosphere (IRI) model. We collected the ionospheric electron density (Ne) profiles from the FORMOSAT-3/COSMIC (F3/C) radio occultation measurements from DoY (day number of year) 194, 2006 to DoY 293, 2008 to investigate the daytime behaviors of IRI-B parameters (B0 and B1) in the equatorial regions. Our fittings confirm that the IRI bottomside profile function can well describe the averaged profiles in the bottomside ionosphere. Analysis of the equatorial electron density profile datasets provides unprecedented detail of the behaviors of B0 and B1 parameters in equatorial regions at low solar activity. The longitudinal averaged B1 has values comparable with IRI-2007 while it shows little seasonal variation. In contrast, the observed B0 presents semiannual variation with maxima in solstice months and minima in equinox months, which is not reproduced by IRI-2007. Moreover, there are complicated longitudinal variations of B0 with patterns varying with seasons. Peaks are distinct in the wave-like longitudinal structure of B0 in equinox months. An outstanding feature is that a stable peak appears around 100°E in four seasons. The significant longitudinal variation of B0 provides challenges for further improving the presentations of the bottomside ionosphere in IRI.  相似文献   
882.
光学侧窗热环境极为严酷,可采用液体对流内冷却技术对光学侧窗进行热防护。以有限元法对光学侧窗温度场进行了分析研究,研究结果表明:该方法计算精度可靠;液体对流内冷却技术能有效起到降温的作用。同时还定量的给出了冷却液用量对结构温度场的影响,为设计的经济可行性提供了保障。  相似文献   
883.
为将富油燃烧/快速淬熄/贫油燃烧(RQL)用于高温升燃烧室设计,以实现温升与排放的良好统一,对不同主燃孔位置下 的单头部矩形燃烧室流动、淬熄区气流混合、燃烧和排放特性进行数值模拟。结果表明:燃烧室中心回流区的长度和高度随着主 燃孔轴向距离的增大而增大。随着主燃孔轴向距离的增大,主燃孔射流深度增加,射流角度逐渐向下游偏转,导致淬熄区内气流 的混合效果减弱;随着主燃孔位置的后移,富油区内的当量比显著增大,导致CO和碳烟的生成量迅速增加,淬熄区内的沿程高温 区域面积逐渐缩小,燃烧效率逐渐降低。当X/H=0.7时,燃烧室沿程NO生成量始终处在较大值;而当X/H=0.9时,燃烧室沿程NO 生成量始终处于较小值,但CO的生成量增大。  相似文献   
884.
IMPROVEMENTOFPHASEGRADIENTAUTOFOCUSALGORITHMLiLiwei(李立伟),MaoShiyi(毛士艺),AsifRaza,LiuYing(刘莹)(DepartmentofElectronicEngineering...  相似文献   
885.
采用电解充氢和三点慢弯曲试验方法研究了23NiCo钢的淬火态以及200℃、450℃、482℃和600℃回火处理的试样的氢脆敏感性。结果表明,23NiCo钢的氢脆抗力与组织中奥氏体的形态、分布有关。482℃回火,在马氏体板条边界形成薄膜状的逆转奥氏体,钢的氢脆抗力有大幅度的提高。此时,延长充氢时间(4~10h)对断裂行为没有影响。  相似文献   
886.
利用Ansys对镀锌锅上方空间的温度场进行模拟。在模拟过程中,利用Ansys软件中的FlotranCFD模块建立模型,计算锌锅上方空间的流场和温度场分布情况,分析温度的主要影响因素,为热镀锌生产线的工程设计提供了理论依据。此方法也为温度分析提供了一种新的思路。  相似文献   
887.
Theoretical analysis and numerical calculations of Love wave propagation in layered graded composites with imperfectly bonded interface are described in this paper. On the basis of WKB method, the approximate analytic solutions for Love waves are obtained. By the interface shear spring model, the dispersion relations for Love waves in layered graded composite structures with rigid, slip, and imperfectly bonded interfaces are given, and the effects of the interface conditions on the phase velocities of Love waves in SiC/Al lay- ered graded composites are discussed. Numerical analysis shows that the phase velocity decreases when the defined flexibility parameter is greater. For the general imperfectly bonded interface, the phase velocity changes in the range of the velocities for the rigid and slip interface conditions.  相似文献   
888.
Three-dimensional computational fluid dynamics analyses have been employed to study the compressible and turbulent flow of the shock train in a convergent–divergent nozzle. The primary goal is to determine the behavior, location, and number of shocks. In this context, full multi-grid initialization, Reynolds stress turbulence model (RSM), and the grid adaption techniques in the Fluent software are utilized under the 3D investigation. The results showed that RSM solution matches with the experimental data suitably. The effects of applying heat generation sources and changing inlet flow total temperature have been investigated. Our simulations showed that changes in the heat generation rate and total temperature of the intake flow influence on the starting point of shock, shock strength, minimum pressure, as well as the maximum flow Mach number.  相似文献   
889.
基于C8051F020单片机和DTD465无线数传模块设计了多路温度双向无线遥测系统.温度测量采用铂电阻;无线数传模块基于FSK调制,采用高效前向纠错信道编码技术;系统为低功耗设计.介绍了测量站和主控站的软件,以及数据通信协议.系统已成功地应用于汽车导航实验中,使用结果表明,本系统软硬件设计完善,可靠性高,使用方便.  相似文献   
890.
Radiometric measurements of the thermal radiation originating from the moon’s surface were obtained using an infrared detector operating at wavelengths between 8 and 14 μm. The measurements cover a full moon cycle. The variation of the moon’s temperature with the lunar phase angle was established. The lunar temperatures were 391 ± 2.0 K for the full moon, 240 ± 3.5 K for the first quarter, and 236 ± 3 K for the last quarter. For the rest of the phase angles, the lunar temperature varied between 170 and 380 K. Our results are comparable with those obtained previously at these phase angles. For the new moon phase, the obtained temperature was between 120 and 133 K. With the exception of the new moon phase, our measurements at all the phase angles were consistent with those obtained using Earth-based data and those obtained by the Diviner experiment and the Clementine spacecraft. At the new phase, our measurements were comparable with those obtained from the ground but were significantly higher than those obtained by the Diviner and Clementine data. We attribute this inconsistency to either the calibration curve of our detector, which does not perform well at very low temperatures, or to infrared emission from the atmosphere. A simple linear model to predict the lunar temperature as a function of the phase angle was proposed. The experimental errors that affect the measured temperatures are discussed.  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