全文获取类型
收费全文 | 994篇 |
免费 | 210篇 |
国内免费 | 134篇 |
专业分类
航空 | 932篇 |
航天技术 | 118篇 |
综合类 | 120篇 |
航天 | 168篇 |
出版年
2024年 | 2篇 |
2023年 | 11篇 |
2022年 | 45篇 |
2021年 | 60篇 |
2020年 | 62篇 |
2019年 | 21篇 |
2018年 | 43篇 |
2017年 | 54篇 |
2016年 | 66篇 |
2015年 | 52篇 |
2014年 | 68篇 |
2013年 | 47篇 |
2012年 | 85篇 |
2011年 | 62篇 |
2010年 | 62篇 |
2009年 | 72篇 |
2008年 | 55篇 |
2007年 | 61篇 |
2006年 | 68篇 |
2005年 | 59篇 |
2004年 | 31篇 |
2003年 | 31篇 |
2002年 | 39篇 |
2001年 | 24篇 |
2000年 | 28篇 |
1999年 | 18篇 |
1998年 | 9篇 |
1997年 | 17篇 |
1996年 | 21篇 |
1995年 | 8篇 |
1994年 | 16篇 |
1993年 | 7篇 |
1992年 | 12篇 |
1991年 | 2篇 |
1990年 | 6篇 |
1989年 | 6篇 |
1988年 | 5篇 |
1984年 | 3篇 |
排序方式: 共有1338条查询结果,搜索用时 15 毫秒
31.
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
32.
33.
34.
35.
36.
37.
燃气涡轮发动机地面试验传感器数据确认概念与方法研究 总被引:1,自引:1,他引:1
本文介绍了燃气涡轮发动机传感器数据确认系统的研究与应用现状,详细阐述了基于发动机和试验系统物理模型的解析冗余检验相关多传感器信号有效性方法,以及基于信号序列统计与时频特征分析的单传感器通道信号有效性的确认方法,提出了传感器数据有效性确认系统的研究框架。 相似文献
38.
机械合金化+热压制备Laves相NbCr2合金及其组织性能研究 总被引:3,自引:0,他引:3
采用机械合金化 热压工艺路线来制备化学配比成分的单相Laves相NbCr2合金.研究了Cr,Nb元素粉经20h球磨后在1200℃,1250℃和1300℃不同时间热压所获得的Laves相NbCr2合金的组织和性能.结果表明:1250℃×0.5h热压获得的Laves相NbCr2合金组织均匀,晶粒尺寸达到微/纳米级,致密度达到97.1%,室温断裂韧性高于5.07MPa·m1/2.与熔铸工艺制备的单相Laves相NbCr2合金的断裂韧性1.50MPa·m1/2相比,所制备的单相Laves相NbCr2合金的室温断裂韧性大大提高,充分实现了细晶韧化的效果. 相似文献
39.
真实气体流动的相似规律 总被引:8,自引:0,他引:8
本文从具有化学反应的NS方程出发导出了真实气体流动的相似律,分别给出了高温空气非平衡流、平衡流和冻结流的相似参数。文中还讨论了航天飞机轨道器各种Mach数范围内的真实气体流动的相似参数和实验模拟问题。 相似文献
40.