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   2438篇
  免费   407篇
  国内免费   180篇
航空   1689篇
航天技术   404篇
综合类   222篇
航天   710篇
  2024年   25篇
  2023年   66篇
  2022年   107篇
  2021年   91篇
  2020年   83篇
  2019年   106篇
  2018年   98篇
  2017年   79篇
  2016年   84篇
  2015年   78篇
  2014年   113篇
  2013年   87篇
  2012年   102篇
  2011年   101篇
  2010年   93篇
  2009年   97篇
  2008年   101篇
  2007年   120篇
  2006年   126篇
  2005年   99篇
  2004年   70篇
  2003年   89篇
  2002年   61篇
  2001年   56篇
  2000年   74篇
  1999年   56篇
  1998年   64篇
  1997年   64篇
  1996年   59篇
  1995年   68篇
  1994年   59篇
  1993年   53篇
  1992年   63篇
  1991年   56篇
  1990年   63篇
  1989年   45篇
  1988年   21篇
  1987年   33篇
  1986年   4篇
  1985年   24篇
  1984年   17篇
  1983年   17篇
  1982年   15篇
  1981年   6篇
  1980年   12篇
  1979年   9篇
  1978年   3篇
  1977年   2篇
  1975年   3篇
  1959年   1篇
排序方式: 共有3025条查询结果,搜索用时 390 毫秒
961.
Atmospheric erosion of CO2-rich Earth-size exoplanets due to coronal mass ejection (CME)-induced ion pick up within close-in habitable zones of active M-type dwarf stars is investigated. Since M stars are active at the X-ray and extreme ultraviolet radiation (XUV) wave-lengths over long periods of time, we have applied a thermal balance model at various XUV flux input values for simulating the thermospheric heating by photodissociation and ionization processes due to exothermic chemical reactions and cooling by the CO2 infrared radiation in the 15 microm band. Our study shows that intense XUV radiation of active M stars results in atmospheric expansion and extended exospheres. Using thermospheric neutral and ion densities calculated for various XUV fluxes, we applied a numerical test particle model for simulation of atmospheric ion pick up loss from an extended exosphere arising from its interaction with expected minimum and maximum CME plasma flows. Our results indicate that the Earth-like exoplanets that have no, or weak, magnetic moments may lose tens to hundreds of bars of atmospheric pressure, or even their whole atmospheres due to the CME-induced O ion pick up at orbital distances 相似文献   
962.
Abundant graphite particles occur in amphibolite-grade quartzite of the Archean-Paleoproterozoic Wutai Metamorphic Complex in the Wutaishan area of North China. Petrographic thin section observations suggest that the graphite particles occur within and between quartzite clasts and are heterogeneous in origin. Using HF maceration techniques, the Wutai graphite particles were extracted for further investigation. Laser Raman spectroscopic analysis of a population of extracted graphite discs indicated that they experienced a maximum metamorphic temperature of 513 +/- 50 degrees C, which is consistent with the metamorphic grade of the host rock and supports their indigenicity. Scanning and transmission electron microscopy revealed that the particles bear morphological features (such as hexagonal sheets of graphite crystals) related to metamorphism and crystal growth, but a small fraction of them (graphite discs) are characterized by a circular morphology, distinct marginal concentric folds, surficial wrinkles, and complex nanostructures. Ion microprobe analysis of individual graphite discs showed that their carbon isotope compositions range from -7.4 per thousand to -35.9 per thousand V-PDB (Vienna Pee Dee Belemnite), with an average of -20.3 per thousand, which is comparable to bulk analysis of extracted carbonaceous material. The range of their size, ultrastructures, and isotopic signatures suggests that the morphology and geochemistry of the Wutai graphite discs were overprinted by metamorphism and their ultimate carbon source probably had diverse origins that included abiotic processes. We considered both biotic and abiotic origins of the carbon source and graphite disc morphologies and cannot falsify the possibility that some circular graphite discs characterized by marginal folds and surficial wrinkles represent deflated, compressed, and subsequently graphitized organic-walled vesicles. Together with reports by other authors of acanthomorphic acritarchs from greenschist-amphibolite-grade metamorphic rocks, this study suggests that it is worthwhile to examine carbonaceous materials preserved in highly metamorphosed rocks for possible evidence of ancient life.  相似文献   
963.
964.
研究了不同边缘连接设计对座舱透明件承载能力的影响.测定了拉伸破坏载荷和冲击能,结果表明,材料种类、边缘连接形式、孔边距等多种因素均会影响边缘连接件的承载能力.  相似文献   
965.
二次通用旋转组合设计试验在造粒技术领域的应用研究   总被引:1,自引:0,他引:1  
本文研究了利用二次通用旋转组合设计来进行多因素影响的振动流化床喷雾造粒试验,建立数学模型,得出了具有一定参数价值的最佳操作参数。  相似文献   
966.
矢量二元收扩喷管热射流复杂流场特征研究   总被引:4,自引:0,他引:4  
提出了一种二元收-扩矢量喷管的概念,用热射流实验台对二元矢量喷管进行了过膨胀状态下的喷管模型热态实验。测量了喷管壁面静压和喷管出口总压分布,用红外热成像技术给出了二元喷管热射流场的清晰画面,并对流场特征进行了描述和分析。研究表明,在非设计状态,二元喷管管内有明显的流动分离现象,喷口射流总压严重畸变,在热射流流场中,射流流场呈现双势核结构。  相似文献   
967.
气动力矩和重力梯度矩实现微小卫星三轴姿态控制   总被引:2,自引:0,他引:2  
提出运用低轨道两个主要环境力矩 (重力梯度矩和气动力矩 )实现微小卫星三轴姿态被动控制方案。重力梯度矩提供俯仰和滚转恢复力矩 ,气动力矩提供偏航和俯仰恢复力矩 ;通过姿态稳定性分析和姿控过程动态仿真 ,结果表明此卫星具有结构简单、姿态稳定精度高的优点。  相似文献   
968.
利用地磁场给飞轮卸载的新方法   总被引:1,自引:0,他引:1  
通过对圆轨道地磁场强度的变化规律分析 ,将卫星磁力矩器产生的磁矩按傅立叶级数展开 ,根据卫星所需卸载角动量大小 ,按照最优控制理论求出三轴磁矩取值 ,得出飞轮卸载控制律。最后文章给出飞轮卸载稳定性分析和仿真结果 ,表明这种飞轮卸载方法简单而且省能量。  相似文献   
969.
某型飞机进气道与发动机地面匹配实验研究   总被引:3,自引:2,他引:1  
通过某型飞机进气道与某型涡喷发动机匹配的地面台架试验,用40点总压和20支周向安装的三孔针组成的测量环获得了进气道出口截面总压的分布和周向气流速度分布。计算了稳态压力周向与径向畸变,获得了它们随发动机进气流量的变化规律。发现了进气道出口的旋流与对涡,并对其形成的原因做了初步分析。测量了发动机主要性能参数如推力、排气温度等在安装飞机进气道后的变化,并分析了引起变化的原因。   相似文献   
970.
Stable carbon isotope ratios (delta(13)C) were determined for alanine, proline, phenylalanine, valine, leucine, isoleucine, aspartate (aspartic acid and asparagine), glutamate (glutamic acid and glutamine), lysine, serine, glycine, and threonine from metabolically diverse microorganisms. The microorganisms examined included fermenting bacteria, organotrophic, chemolithotrophic, phototrophic, methylotrophic, methanogenic, acetogenic, acetotrophic, and naturally occurring cryptoendolithic communities from the Dry Valleys of Antarctica. Here we demonstrated that reactions involved in amino acid biosynthesis can be used to distinguish amino acids formed by life from those formed by nonbiological processes. The unique patterns of delta(13)C imprinted by life on amino acids produced a biological bias. We also showed that, by applying discriminant function analysis to the delta(13)C value of a pool of amino acids formed by biological activity, it was possible to identify key aspects of intermediary carbon metabolism in the microbial world. In fact, microorganisms examined in this study could be placed within one of three metabolic groups: (1) heterotrophs that grow by oxidizing compounds containing three or more carbon-to-carbon bonds (fermenters and organotrophs), (2) autotrophs that grow by taking up carbon dioxide (chemolitotrophs and phototrophs), and (3) acetoclastic microbes that grow by assimilation of formaldehyde or acetate (methylotrophs, methanogens, acetogens, and acetotrophs). Furthermore, we demonstrated that cryptoendolithic communities from Antarctica grouped most closely with the autotrophs, which indicates that the dominant metabolic pathways in these communities are likely those utilized for CO(2 )fixation. We propose that this technique can be used to determine the dominant metabolic types in a community and reveal the overall flow of carbon in a complex ecosystem.  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