全文获取类型
收费全文 | 1456篇 |
免费 | 238篇 |
国内免费 | 224篇 |
专业分类
航空 | 970篇 |
航天技术 | 343篇 |
综合类 | 198篇 |
航天 | 407篇 |
出版年
2024年 | 8篇 |
2023年 | 27篇 |
2022年 | 38篇 |
2021年 | 67篇 |
2020年 | 52篇 |
2019年 | 38篇 |
2018年 | 62篇 |
2017年 | 66篇 |
2016年 | 62篇 |
2015年 | 66篇 |
2014年 | 93篇 |
2013年 | 78篇 |
2012年 | 107篇 |
2011年 | 116篇 |
2010年 | 86篇 |
2009年 | 90篇 |
2008年 | 85篇 |
2007年 | 96篇 |
2006年 | 95篇 |
2005年 | 72篇 |
2004年 | 73篇 |
2003年 | 41篇 |
2002年 | 63篇 |
2001年 | 52篇 |
2000年 | 42篇 |
1999年 | 32篇 |
1998年 | 39篇 |
1997年 | 20篇 |
1996年 | 33篇 |
1995年 | 25篇 |
1994年 | 18篇 |
1993年 | 16篇 |
1992年 | 14篇 |
1991年 | 13篇 |
1990年 | 14篇 |
1989年 | 15篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1986年 | 1篇 |
1984年 | 1篇 |
排序方式: 共有1918条查询结果,搜索用时 15 毫秒
1.
研究微小卫星综合电子系统的SiP技术实现方法。首先介绍微小卫星综合电子系统结构的组成和采用SiP技术的必要性,然后对综合电子系统进行功能模块划分,并对其通用扩展模块进行详细的SiP设计,包括抗辐照器件选型、原型验证、SiP原理图、基板管壳一体化设计、建模仿真、制造加工、实装测试验证等,通过SiP技术实现了一种星载综合电子系统中通用扩展SiP芯片产品,经过实际验证测试,在保证模块功能和性能的前提下,整体模块重量从230 g减轻到48 g,体积由180 mm?130 mm?17 mm减小到46 mm?46 mm?8 mm,很好地满足了星载功能模块小型化、轻量化设计需求。 相似文献
2.
应用伏特拉级数法分析了电容耦合FET振荡系统在外加信号下的注入锁定现象,推导出输出信号和注入锁定带宽表达式。与一般非线性系统分析方法相比,伏特拉级数法在建立好系统模型后只需进行代数运算,从而避开了求解非线性,非齐次高阶微分方程的复杂过程。 相似文献
3.
4.
弹道交班自适应算法研究 总被引:1,自引:0,他引:1
为实现复合制导不同制导弹道的平滑过渡,用二阶吻合法设计了一不同制导律间的指令交接导引段。建立了自适应弹道交接导引算法的模型。理论分析和仿真结果表明,该算法具较好的弹道过载平滑能力,有一定的应用价值。 相似文献
5.
The significance of external influences on the environment of Earth and its atmosphere has become evident during recent years.
Especially, on time scales of several hundred years, the cosmogenic isotope concentration during the Wolf-, Spoerer-, Maunder-
and Dalton-Minimum indicates an increased cosmic ray flux. Because these grand minima of solar activity coincide with cold
periods, a correlation of the Earth climate with the cosmic ray intensities is plausible. Any quantitative study of the effects
of energetic particles on the atmosphere and environment of the Earth must address their transport to Earth and their interactions
with the Earth’s atmosphere including their filtering by the terrestrial magnetosphere. The first problem is one of the fundamental
problems in modern cosmic ray astrophysics, and corresponding studies began in the 1960s based on Parker’s cosmic ray modulation
theory taking into account diffusion, convection, adiabatic deceleration, and (later) the drift of energetic particles in
the global heliospheric magnetic field. It is well established that all of these processes determining the modulation of cosmic
rays are depending on parameters that are varying with the solar magnetic cycle. Therefore, the galactic cosmic ray intensities
close to Earth is the result of a complex modulation of the interstellar galactic spectrum within the heliosphere. The modern
view of this cosmic ray modulation is summarized in our contribution. 相似文献
6.
The earth's foreshock is a region where particularly large amplitude MHD waves are commonly observed. They exhibit various
waveforms, suggesting that nonlinear interaction between the waves is in progress. In a previous paper (Hada et al., 2003) we have introduced a method to quantitatively evaluate the strength of phase coherence among the waves from a given
time series data. Here we further develop our method by applying wavelet filtering technique. From the analysis it was found
that, although the turbulence is consisted of waves with a wide range of plasma rest frame frequencies, only those frequencies
lower than the ion gyrofrequency are responsible for generating the phase coherence.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
7.
P.B. Marty S. Bardeau O. Czoske H. Ebeling J.P. Kneib R. Sadat I. Smail 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2509-2515
We present an analysis of seven clusters observed by XMM-Newton as part of our survey of 17 most X-ray luminous clusters of galaxies at z 0.2 selected for a comprehensive and unbiased study of the mass distribution in massive clusters. Using the public software FTOOLS and XMMSAS we have set up an automated pipeline to reduce the EPIC MOS and pn spectro-imaging data, optimized for extended sources analysis. We also developped a code to perform intensive spectral and imaging analysis particularly focussing on proper background estimate and removal. XMM-Newton deep spectro-imaging of these clusters allowed us to fit a standard β-model to their gas emission profiles as well as a standard MEKAL emission model to their extracted spectra, and test their inferred characteristics against already calibrated relations. 相似文献
8.
9.
阐述了研制全天球实时恒星模拟器的意义以及国内外发展趋势,介绍第二代恒星模拟器的系统组成、特点、技术指标以及解决的技术问题。 相似文献
10.
本文利用弹性力学和断裂力学方法对纤维增强复合材料的横向拉伸强度进行了分析,其中考虑了90度开裂层厚度和开裂邻层的约束效应的影响,推导出正交各向异性对称铺层中昨合就位横向拉伸强度的数学表达式,得出开裂层的厚度和约束邻层铺设角对就位横向拉伸强度都有影响的结论,理论计算与Flaggs实验结果吻合较好。 相似文献