全文获取类型
收费全文 | 475篇 |
免费 | 77篇 |
国内免费 | 100篇 |
专业分类
航空 | 292篇 |
航天技术 | 144篇 |
综合类 | 56篇 |
航天 | 160篇 |
出版年
2024年 | 1篇 |
2023年 | 21篇 |
2022年 | 10篇 |
2021年 | 17篇 |
2020年 | 17篇 |
2019年 | 20篇 |
2018年 | 10篇 |
2017年 | 22篇 |
2016年 | 27篇 |
2015年 | 26篇 |
2014年 | 32篇 |
2013年 | 25篇 |
2012年 | 50篇 |
2011年 | 41篇 |
2010年 | 36篇 |
2009年 | 46篇 |
2008年 | 48篇 |
2007年 | 34篇 |
2006年 | 29篇 |
2005年 | 33篇 |
2004年 | 10篇 |
2003年 | 19篇 |
2002年 | 13篇 |
2001年 | 10篇 |
2000年 | 5篇 |
1999年 | 6篇 |
1998年 | 3篇 |
1997年 | 4篇 |
1996年 | 10篇 |
1995年 | 7篇 |
1994年 | 3篇 |
1993年 | 4篇 |
1992年 | 5篇 |
1991年 | 1篇 |
1989年 | 1篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1986年 | 1篇 |
1984年 | 3篇 |
排序方式: 共有652条查询结果,搜索用时 15 毫秒
131.
Dale P. Cruikshank 《Space Science Reviews》2005,116(1-2):421-439
The diverse populations of icy bodies of the outer Solar System (OSS) give critical information on the composition and structure
of the solar nebula and the early phases of planet formation. The two principal repositories of icy bodies are the Kuiper
belt or disk, and the Oort Cloud, both of which are the source regions of the comets. Nearly 1000 individual Kuiper belt objects
have been discovered; their dynamical distribution is a clue to the early outward migration and gravitational scattering power
of Neptune. Pluto is perhaps the largest Kuiper belt object. Pluto is distinguished by its large satellite, a variable atmosphere,
and a surface composed of several ices and probable organic solid materials that give it color. Triton is probably a former
member of the Kuiper belt population, suggested by its retrograde orbit as a satellite of Neptune. Like Pluto, Triton has
a variable atmosphere, compositionally diverse icy surface, and an organic atmospheric haze. Centaur objects appear to come
from the Kuiper belt and occupy temporary orbits in the planetary zone; the compositional similarity of one well studied Centaur
(5145 Pholus) to comets is notable. New discoveries continue apace, as observational surveys reveal new objects and refined
observing techniques yield more physical information about specific bodies. 相似文献
132.
Dario Lorenzetti 《Space Science Reviews》2005,119(1-4):181-199
Observations of pre-main sequence objects (T Tauri, Herbig Ae/Be and FU Orionis stars) obtained with the instrumentation on
board the Infrared Space Observatory (ISO) are reviewed. All the observations have been mainly carried out by using the two
spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to
reconstruct the spectral energy distributions. Line emission and photometric behaviour of pre-main sequence objects have been
analyzed in the framework of the current models, discussing the agreement (or disagreement) with them and trying to derive
the questions which should be answered by the forthcoming FIR instrumentation.
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries:
France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA. 相似文献
133.
Alain Abergel Laurent Verstraete Christine Joblin René Laureijs Marc-Antoine Miville-Deschênes 《Space Science Reviews》2005,119(1-4):247-271
Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important
progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also
the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the
interstellar medium, where T
gas≲ 500 K, n
H∼ 100–105 cm−3 and the electron density is a few 10−4.
JEL codes: D24, L60, 047
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries:
France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA. 相似文献
134.
针对某型号卫星加热笼设计中的一些特殊问题,设计了一些特殊的处理方法,包括加热带双面涂黑漆的方法,加热笼结构设计中的一些特殊处理,以及支架控温装置等的设计。试验证明,这些方法在卫星真空热试验过程中取得了好的效果,可以为今后加热笼的设计开阔思路,有利于更好地完成试验任务。 相似文献
135.
FY-2C星多通道扫描辐射计及其在轨运行 总被引:3,自引:0,他引:3
介绍了风云二号(FY-2)C静止气象卫星多通道扫描辐射计的性能、组成和工作原理,以及为适应将3通道改为5通道而完成的5通道焦平面、光学系统、结构、电子学、红外探测器、辐射致冷器、光学薄膜和第二扫描结构等主要设计改进.卫星的在轨测试和运行结果表明,C星扫描辐射计在第一代自旋静止气象卫星上实现了包括中波红外的5通道同时对地观测,图像质量总体优于同类GMS5,METEOSAT-5静止气象卫星,与目前应用的GOES9三轴稳定静止气象卫星基本相当. 相似文献
136.
137.
Yu.N. Gnedin G.V. Khozov V.M. Larionov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
Observations of the X-ray binaries 4U 0115+634 and A 0535+262 performed in 1981 – 1982 revealed significant IR variabilities of these sources. 4U 0115+634 was observed twice, in the state close to X-ray activity, and in the state of low activity, thus changing from K = 7m.75 to K > 9m. A 0535+262 shows the temporal variations ranged from tens minutes to some days. The regular variations of IR brightness are suspected with teh period close to 104 s that corresponds to the period of axial rotation of neutron star in A 0535+262. The results obtained present arguments in favour of hypothesis that IR radiation is generated near the accreting neutron star and is possibly of maser nature. 相似文献
138.
红外气体分析中环境影响的补偿方法研究 总被引:6,自引:0,他引:6
环境温度、总压影响是红外气体分析中难以有效解决的主要问题之一,本文以二氧化碳气体为测量对象,采用实验手段,单片机和数据自理技术建立了环境温度、总压对红上气体分析影响的补偿数学模型和求解方法,并进行了实验验证,研究的内容为红外气体分析中影响影响的外补偿开始辟了一条新的途径,具有广阔的应用前景。 相似文献
139.
Spectral analysis and self-adjusting mechanism for oscillation phenomenon in hydrogen-oxygen continuously rotating detonation engine 总被引:2,自引:0,他引:2
The continuously rotating detonation engine(CRDE)is a new concept of engines for aircraft and spacecraft.Quasi-stable continuously rotating detonation(CRD)can be observed in an annular combustion chamber,but the sustaining,stabilizing and adjusting mechanisms are not yet clear.To learn more deeply into the CRDE,experimental studies have been carried out to investigate hydrogen-oxygen CRDE.Pressure histories are obtained during each shot,which show that stable CRD waves are generated in the combustor,when feeding pressures are higher than 0.5 MPa for fuel and oxidizer,respectively.Each shot can keep running as long as fresh gas feeding maintains.Close-up of the pressure history shows the repeatability of pressure peaks and indicates the detonation velocity in hydrogen–oxygen CRD,which proves the success of forming a stable CRD in the annular chamber.Spectrum of the pressure history matches the close-up analysis and confirms the CRD.It also shows multi-wave phenomenon and affirms the fact that in this case a single detonation wave is rotating in the annulus.Moreover,oscillation phenomenon is found in pressure peaks and a self-adjusting mechanism is proposed to explain the phenomenon. 相似文献
140.
Brunella Nisini Anlaug Amanda Kaas Ewine F. Van Dishoeck Derek Ward-Thompson 《Space Science Reviews》2005,119(1-4):159-179
We summarize the observations of the Infrared Space Observatory (ISO) concerning the earliest stages of the stellar formation.
The observations of samples of sources in different evolutionary stages are reviewed, addressing in particular how the physical
and chemical properties of the protostellar environments change from the pre-stellar cores to the protostars at the end of
their accretion phase. In addition, the mid-IR surveys in nearby star-forming regions are discussed, showing their implications
for the understanding of the stellar initial mass function.
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries:
France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA. 相似文献