全文获取类型
收费全文 | 699篇 |
免费 | 122篇 |
国内免费 | 55篇 |
专业分类
航空 | 406篇 |
航天技术 | 182篇 |
综合类 | 65篇 |
航天 | 223篇 |
出版年
2024年 | 5篇 |
2023年 | 19篇 |
2022年 | 21篇 |
2021年 | 24篇 |
2020年 | 15篇 |
2019年 | 28篇 |
2018年 | 18篇 |
2017年 | 24篇 |
2016年 | 32篇 |
2015年 | 28篇 |
2014年 | 51篇 |
2013年 | 39篇 |
2012年 | 47篇 |
2011年 | 61篇 |
2010年 | 49篇 |
2009年 | 59篇 |
2008年 | 61篇 |
2007年 | 32篇 |
2006年 | 34篇 |
2005年 | 30篇 |
2004年 | 35篇 |
2003年 | 26篇 |
2002年 | 27篇 |
2001年 | 32篇 |
2000年 | 14篇 |
1999年 | 9篇 |
1998年 | 10篇 |
1997年 | 11篇 |
1996年 | 1篇 |
1995年 | 6篇 |
1994年 | 9篇 |
1993年 | 3篇 |
1992年 | 3篇 |
1991年 | 2篇 |
1990年 | 2篇 |
1989年 | 3篇 |
1988年 | 1篇 |
1984年 | 4篇 |
1981年 | 1篇 |
排序方式: 共有876条查询结果,搜索用时 609 毫秒
211.
212.
Richard N. Grugel Houssam Toutanji 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):103-112
Melting sulfur and mixing it with an aggregate to form “concrete” is commercially well established and constitutes a material that is particularly well-suited for use in corrosive environments. Discovery of the mineral troilite (FeS) on the moon poses the question of extracting the sulfur for use as a lunar construction material. This would be an attractive alternative to conventional concrete as it does not require water. However, the viability of sulfur concrete in a lunar environment, which is characterized by lack of an atmosphere and extreme temperatures, is not well understood. Here it is assumed that the lunar ore can be mined, refined, and the raw sulfur melded with appropriate lunar regolith to form, for example, bricks. This study evaluates pure sulfur and two sets of small sulfur concrete samples that have been prepared using JSC-1 lunar stimulant and SiO2 powder as aggregate additions. Each set was subjected to extended periods in a vacuum environment to evaluate sublimation issues. Results from these experiments are presented and discussed within the context of the lunar environment. 相似文献
213.
徐剑锋 《西安航空技术高等专科学校学报》2007,25(2):78-80
从中国新闻史目前的现状出发,看出中国新闻史研究的成绩和困境。在比较分析《中国新闻事业通史》和《美国新闻史》的叙事模式的基础上,提出并论证了通过新闻史书写中主体意识的加强,来弥补历史书写中微观叙述的缺失。 相似文献
214.
C. M. Lisse M. F. A’Hearn T. L. Farnham O. Groussin K. J. Meech U. Fink D. G. Schleicher 《Space Science Reviews》2005,117(1-2):161-192
As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules
and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface
temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 102 km), it is in collisional equilibrium, at larger distances (≥104 km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply
dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics
of the coma, as well as with its variability with time, orbital position, and heliocentric distance.
The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive
measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several
gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986.
This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current
state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards
that the coma presents for the spacecraft.
An erratum to this article is available at . 相似文献
215.
Deep Impact Mission Design 总被引:1,自引:0,他引:1
William H. Blume 《Space Science Reviews》2005,117(1-2):23-42
The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed
impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment.
The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus
size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability
for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth. 相似文献
216.
Since its discovery in 1867, periodic comet 9P/Tempel 1 has been observed at 10 returns to perihelion, including all its returns
since 1967. The observations for the seven apparitions beginning in 1967 have been fit with an orbit that includes only radial
and transverse nongravitational accelerations that model the rocket-like thrusting introduced by the outgassing of the cometary
nucleus. The successful nongravitational acceleration model did not assume any change in the comet’s ability to outgas from
one apparition to the next and the outgassing was assumed to reach a maximum at perihelion. The success of this model over
the 1967–2003 interval suggests that the comet’s spin axis is currently stable. Rough calculations suggest that the collision
of the impactor released by the Deep Impact spacecraft will not provide a noticeable perturbation on the comet’s orbit nor
will any new vent that is opened as a result of the impact provide a noticeable change in the comet’s nongravitational acceleration
history. The observing geometries prior to, and during, the impact will allow extensive Earth based observations to complement
the in situ observations from the impactor and flyby spacecraft. 相似文献
217.
王香%于德志%连晓明%李庆芬 《宇航材料工艺》2006,36(4):50-53
采用自蔓延高温合成(SHS)法制备高TiC颗粒含量的TiC/Al复合材料。利用自制的实验装置研究复合材料中TiC颗粒在静止锌液中的均匀化过程。结果表明:当锌液温度低于铝的熔点时,TiC/Al复合材料置于锌液后,锌向其内部扩散,引起复合材料表层内液相线温度降低,当表层内Al-Zn合金的液相线温度等于或低于锌液温度时,Al-Zn合金便处于熔融状态,TiC颗粒随其一起从TiC/Al复合材料块上脱落,并不断地向锌液内部传输,最终均匀分布在锌液中;而当锌液温度高于铝熔点时,TiC/Al复合材料置入后,锌和铝同时进行扩散,但是当复合材料表面温度达到铝熔点时,铝开始熔化,铝的熔化导致TiC颗粒的脱落,脱落下来的TiC颗粒不断向锌液内部传输,最终均匀分布在锌液中。 相似文献
218.
219.
220.
Philipp Podsiadlowski 《Space Science Reviews》1993,66(1-4):439-453
Nearby supernovae like SN 1987A and SN 1993J provide valuable constraints on the late evolution of massive stars. For this purpose, we review evolutionary models for the progenitor of SN 1987A and confront them with five observational/theoretical tests we devised. We show that single-star models (with the possible exception of rapid-rotation models) fail at least two of these tests, while two binary models (accretion and merger models) are consistent with all available constraints. We conclude that it is most likely that the progenitor of SN 1987A had a binary companion, either at the time of the explosion or at least in the not-too-distant past, and that SN 1987A should therefore not be used to calibrate single stellar evolution theory. For SN 1993J, we infer from the presupernova photometry and the early light curve that its progenitor was a 15M
star that lost almost all of its hydrogen-rich envelope prior to the supernova. This seems to require that the progenitor underwent stable case C mass transfer. We discuss future observational tests of binary models for both supernovae. 相似文献