全文获取类型
收费全文 | 5983篇 |
免费 | 1837篇 |
国内免费 | 964篇 |
专业分类
航空 | 5209篇 |
航天技术 | 1187篇 |
综合类 | 584篇 |
航天 | 1804篇 |
出版年
2024年 | 47篇 |
2023年 | 162篇 |
2022年 | 441篇 |
2021年 | 432篇 |
2020年 | 426篇 |
2019年 | 360篇 |
2018年 | 333篇 |
2017年 | 430篇 |
2016年 | 320篇 |
2015年 | 383篇 |
2014年 | 379篇 |
2013年 | 389篇 |
2012年 | 494篇 |
2011年 | 486篇 |
2010年 | 466篇 |
2009年 | 427篇 |
2008年 | 420篇 |
2007年 | 417篇 |
2006年 | 373篇 |
2005年 | 303篇 |
2004年 | 246篇 |
2003年 | 178篇 |
2002年 | 182篇 |
2001年 | 136篇 |
2000年 | 131篇 |
1999年 | 91篇 |
1998年 | 44篇 |
1997年 | 37篇 |
1996年 | 32篇 |
1995年 | 24篇 |
1994年 | 33篇 |
1993年 | 28篇 |
1992年 | 27篇 |
1991年 | 36篇 |
1990年 | 17篇 |
1989年 | 20篇 |
1988年 | 9篇 |
1987年 | 14篇 |
1986年 | 4篇 |
1983年 | 1篇 |
1981年 | 1篇 |
1977年 | 1篇 |
1972年 | 2篇 |
1970年 | 1篇 |
1965年 | 1篇 |
排序方式: 共有8784条查询结果,搜索用时 15 毫秒
71.
本文从主次流气动参数(相对静压降、主次流温比、主流马赫数等)和冷却结构(冲击高度、开孔率等)两方面比较分析了两种双层壁复合冷却结构及对应的单层壁冷却结构的冷却效率。试验结果表明:气动参数中相对压降对冷却效率的影响较大,结构参数中冲击高度对冷却效率的影响较小,而试验孔板开孔率对冷却效率的影响较大,增加冲击板后的双层壁复合冷却结构冷却效率大大增强。 相似文献
72.
杨春燕 《西安航空技术高等专科学校学报》2006,24(3):71-73
课程设计是教学中的重要实践环节,在促进学生对课程内容的消化和吸收,培养学生查找、利用资源,锻炼学生综合运用所学知识和技能创造性地解决实际问题等方面,具有重要的意义。以《机械制图》为例,从选题、讲授到评分,探讨了如何在课程设计中培养和提高学生的综合应用能力。 相似文献
73.
绩效管理是人力资源管理的一个核心内容,它对于提高组织管理水平,完善激励机制,树立组织价值观,实现战略目标至关重要。文章针对当前基层税务组织绩效管理存在的问题,结合现代绩效管理基本理论及其在西方公共部门的应用,从关键绩效指标体系、绩效文化、绩效考核等方面构建了基层税务组织的绩效管理系统,通过绩效管理系统的实施,不断改进和提升税务组织的总体绩效。 相似文献
74.
对求解偏微分方程问题的程序的严格验证,一直以来由于其精确解有限,较难进行,针对这种情况,本文给出了一种新的程序验证方法,虚构解方法,该方法旨在解决大型科学计算程序如何较严格地进行程序验证这一问题;该方法通过构造虚构解,修改原控制方程,然后通过对计算结果的分析处理达到对程序的精确验证;文中给出了一组通用的虚构解的选取办法,解决了虚构解方法验证过程中确定虚构解的问题;同时还给出了运用该方法对非结构二维Euler计算程序进行验证的具体例子,网格收敛分析结果表明该方法是一种有效的程序验证方法,并且具有较好的通用性。 相似文献
75.
76.
77.
针对发动机转子高速动平衡转速波动、无法保证振动信号同步整周期采样的特点,提出了一种基于转速脉冲的振动信号重构技术,大大提高了相量测量的准确度和稳定性。经试验验证,这项技术是有效、可行的。 相似文献
78.
阐述了ART1神经网络在制造单元设计过程中形成零件族的基本方法,并在基于MATLAB的软件平台上,利用其神经网络工具箱对生产过程中的实际情况进行了仿真和应用。 相似文献
79.
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
80.
基于μ综合的鲁棒飞行控制系统设计 总被引:1,自引:0,他引:1
针对飞控系统设计中存在的建模误差以及实际飞行中的外界干扰的影响,采用 μ综合控制方法,根据系统的飞行品质及设计要求,构造了纵向姿态控制系统μ综合控制设计框架,选取了不同环节的权函数,数字仿真表明,所设计的某型无人机飞控系统具有良好的性能。 相似文献