全文获取类型
收费全文 | 1427篇 |
免费 | 250篇 |
国内免费 | 322篇 |
专业分类
航空 | 1284篇 |
航天技术 | 230篇 |
综合类 | 244篇 |
航天 | 241篇 |
出版年
2024年 | 3篇 |
2023年 | 24篇 |
2022年 | 64篇 |
2021年 | 71篇 |
2020年 | 79篇 |
2019年 | 76篇 |
2018年 | 81篇 |
2017年 | 75篇 |
2016年 | 98篇 |
2015年 | 84篇 |
2014年 | 81篇 |
2013年 | 76篇 |
2012年 | 108篇 |
2011年 | 111篇 |
2010年 | 103篇 |
2009年 | 110篇 |
2008年 | 76篇 |
2007年 | 92篇 |
2006年 | 69篇 |
2005年 | 62篇 |
2004年 | 56篇 |
2003年 | 44篇 |
2002年 | 46篇 |
2001年 | 45篇 |
2000年 | 22篇 |
1999年 | 29篇 |
1998年 | 21篇 |
1997年 | 17篇 |
1996年 | 30篇 |
1995年 | 22篇 |
1994年 | 25篇 |
1993年 | 22篇 |
1992年 | 23篇 |
1991年 | 20篇 |
1990年 | 13篇 |
1989年 | 11篇 |
1988年 | 8篇 |
1987年 | 1篇 |
1984年 | 1篇 |
排序方式: 共有1999条查询结果,搜索用时 15 毫秒
11.
本文研究了微弯机翼在正弦阵风作用下的脉动升力,并导出计算公式,分析了动、静叶栅几何及气动参数对转子脉动升力及噪声级的影响。 相似文献
12.
13.
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
14.
15.
孙凯斌 《沈阳航空工业学院学报》1996,13(1):45-52
本文基于近红外制导系统噪声分析的框架模型,在分析探讨主要噪声源的基础上,给出了基本噪声立意,建立了探测器等组成部件基本噪声的功率谱分析式,设计出一种以红外探测器为抑制主体的减噪系统。通过目标、误差响应率的测定与跟踪试验获得较好的效果。 相似文献
16.
刘利秋 《沈阳航空工业学院学报》2005,22(3):58-61
时差法相关测量中信号的带宽越宽,互相关函数的峰值点的峰值优势越大,其测量的抗干扰性能越好。通过理论分析和数学仿真研究了两种宽带信号源——噪声信号和扫频信号,并利用相关分析法测量两信号问时差时的性能。结论是:噪声信号频带范围宽,带宽不受所采用信号长短的限制,测量分辨力高,但其频谱与噪声干扰频谱相似,抗干扰能力差;扫频信号的频率和带宽可人为控制,频谱特征明显,抗干扰性能好。 相似文献
17.
宋敏 《西安航空技术高等专科学校学报》2004,22(1):3-6
用正交法对斜齿圆柱齿轮传动进行参数优化设计 ,用方差分析法找出对质量影响最显著的因素 ,最后 ,由信噪比作为指标选出最佳参数组合 ,这是一种快速创新开发产品的设计方法。 相似文献
18.
19.
二维小波变换及其在医学图像处理中的应用 总被引:5,自引:0,他引:5
介绍了二维离散小波变换的一般形式,在图像分解的基础上.分析了二维小波变换在医学图像消噪和图像增强中的应用,同时给出应用实例。结果表明,应用小波分析进行医学图像处理,能够有效地改善图像质量,有利于医生对病情的诊断和治疗。 相似文献
20.