全文获取类型
收费全文 | 2573篇 |
免费 | 553篇 |
国内免费 | 628篇 |
专业分类
航空 | 2372篇 |
航天技术 | 551篇 |
综合类 | 470篇 |
航天 | 361篇 |
出版年
2024年 | 13篇 |
2023年 | 55篇 |
2022年 | 113篇 |
2021年 | 135篇 |
2020年 | 123篇 |
2019年 | 128篇 |
2018年 | 124篇 |
2017年 | 128篇 |
2016年 | 142篇 |
2015年 | 138篇 |
2014年 | 156篇 |
2013年 | 159篇 |
2012年 | 164篇 |
2011年 | 204篇 |
2010年 | 157篇 |
2009年 | 181篇 |
2008年 | 158篇 |
2007年 | 145篇 |
2006年 | 132篇 |
2005年 | 118篇 |
2004年 | 93篇 |
2003年 | 95篇 |
2002年 | 82篇 |
2001年 | 61篇 |
2000年 | 61篇 |
1999年 | 87篇 |
1998年 | 71篇 |
1997年 | 55篇 |
1996年 | 77篇 |
1995年 | 56篇 |
1994年 | 62篇 |
1993年 | 62篇 |
1992年 | 62篇 |
1991年 | 46篇 |
1990年 | 47篇 |
1989年 | 31篇 |
1988年 | 29篇 |
1987年 | 2篇 |
1986年 | 2篇 |
排序方式: 共有3754条查询结果,搜索用时 437 毫秒
51.
S. M. Krimigis D. G. Mitchell D. C. Hamilton S. Livi J. Dandouras S. Jaskulek T. P. Armstrong J. D. Boldt A. F. Cheng G. Gloeckler J. R. Hayes K. C. Hsieh W.-H. Ip E. P. Keath E. Kirsch N. Krupp L. J. Lanzerotti R. Lundgren B. H. Mauk R. W. McEntire E. C. Roelof C. E. Schlemm B. E. Tossman B. Wilken D. J. Williams 《Space Science Reviews》2004,114(1-4):233-329
The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R
S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm2 sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm2 sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm2 sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm2 sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R
S every 2–3 h (every ∼10 min from ∼20 R
S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date. 相似文献
52.
杨胜群%孟庆武%耿林%吴林%陈彦宾 《宇航材料工艺》2007,37(3):58-60
为了提高钛合金的表面耐磨性,利用氧乙炔热喷涂枪,在TC4合金表面上制备出镍包石墨涂层。采用MXP-2000型销盘式摩擦磨损实验机,进行钛合金及其镍包石墨涂层的干摩擦磨损实验,并利用扫描电镜对磨损表面进行观察和分析。实验结果发现,镍包石墨涂层的摩擦系数只有钛合金的一半左右,前者磨损量为后者的1/6,说明镍包石墨涂层可以大大提高钛合金的表面耐磨性能。TC4合金的磨损机制以黏着磨损为主,喷涂层的磨损机制以磨粒磨损为主,喷涂层中的石墨润滑相是其耐磨性高的主要原因。 相似文献
53.
郭丽春 《沈阳航空工业学院学报》2006,23(3):47-49
分布式防火墙为网络安全提供了技术支持,可为企事业单位提供多层次、多协议的全方位安全体系。采用主机驻留的方式保护网络中的关键结点服务器、数据和工作站免受非法入侵的破坏,采用多层过滤,入侵检测,日志记录等手段为不同服务器和主机实施安全策略。较好地解决了企业内网与外网以及内部子网之间的非法攻击问题。 相似文献
54.
55.
高速列车进入带缓冲结构隧道的压力变化研究(I) 总被引:1,自引:0,他引:1
给出了列车穿越带有缓冲结构的隧道压力变化的三维粘性流场数值模拟过程,控制方程为三维粘性、可压缩、非定常流的N.S方程,空间离散采用了中心有限体积法格式,时间采用预处理二阶精度多步后差分格式进行离散,对列车与隧道之间的相对运动采用移动网格技术处理。对不同的缓冲结构缓解隧道内瞬变压力及压力梯度的作用进行了研究。研究结果表明,缓冲结构的设置能够有效地降低隧道内的压力和压力梯度的最大值,其原因在于缓冲结构延长了压缩波压力上升的时间,降低列车突入隧道时所形成的最大压力梯度;另一方面由于压缩波在缓冲结构和列车、隧道之间多次的反射,也降低了压力峰值。 相似文献
56.
利用NI 的PXI-6281高速数据采集卡来完成角速度波动信号的采集,借鉴信号失真度的概念,分析角速度反馈信号的基波和高次谐波大小,求取高次谐波与基波幅值比,作为角速度波动率. 相似文献
57.
粘流与无粘流的相互作用计算 总被引:1,自引:1,他引:1
本文总结了粘流/无粘流的各种计算方法和结果。重点在于介绍定常流动中的弱相互作用。首先叙述了弱相互作用的数学模型。给出了不可压流动和跨音速流动中粘流/无粘流相互作用的某些正耦合的计算结果。讨论了在分离区附近边界层正方法失效的原因。然后介绍了边界层反方法和适用于带分离的流动中半反方法耦合的粘流/无粘流的相互作用方法。文中也简单地总结了三维情况的应用和强相互作用。 相似文献
58.
刘颖 《沈阳航空工业学院学报》2001,18(2):1-6
本文利用格林函数、Banach空间中的压缩映象原理及Schauder不动点定理证明了四阶方程y( 4 ) =f(t,y ,y′,y″,y ) ( 1 )满足下列四点边界条件y(i) ( t1) =a1,y(j) ( t2 ) =a2 ,y(k) ( t3) =a3,y(l) ( t4 ) =a4 ( 2 )的边值问题解的存在性和唯一性。其中 t1, t2 , t3, t4 ,∈ {t1,t2 ,t3,t4 }且互不相同 ,a 相似文献
59.
给出了一种基于欧拉方程的跨声速翼型设计方法。方法以Takanashi提出的“正反迭代余量修正”设计原理为基础,在气动力分析模块中,以欧拉方程为基本控制方程,并采用Walz边界层方法对其进行粘性修正;反设计模块采用经过改进的二维翼型设计方法。方法的程序经过几个设计实例主题证明是有效而实用的。 相似文献
60.
根据本文给出的守恒方程和计算方法,对激波与沉积可燃粉尘的相互作用进行了数值研究,讨论了激波作用下的颗粒的上扬、点火与燃烧的基本特征以及波后燃烧粉尘云的内部结构。 相似文献