全文获取类型
| 收费全文 | 198篇 |
| 免费 | 1篇 |
专业分类
| 航空 | 93篇 |
| 航天技术 | 55篇 |
| 综合类 | 1篇 |
| 航天 | 50篇 |
出版年
| 2022年 | 1篇 |
| 2021年 | 4篇 |
| 2020年 | 4篇 |
| 2019年 | 5篇 |
| 2018年 | 7篇 |
| 2017年 | 3篇 |
| 2016年 | 1篇 |
| 2015年 | 3篇 |
| 2014年 | 7篇 |
| 2013年 | 9篇 |
| 2012年 | 6篇 |
| 2011年 | 15篇 |
| 2010年 | 15篇 |
| 2009年 | 15篇 |
| 2008年 | 11篇 |
| 2007年 | 6篇 |
| 2006年 | 7篇 |
| 2005年 | 3篇 |
| 2004年 | 1篇 |
| 2003年 | 6篇 |
| 2001年 | 3篇 |
| 2000年 | 3篇 |
| 1999年 | 5篇 |
| 1998年 | 2篇 |
| 1996年 | 1篇 |
| 1995年 | 1篇 |
| 1994年 | 1篇 |
| 1993年 | 9篇 |
| 1992年 | 2篇 |
| 1991年 | 1篇 |
| 1988年 | 1篇 |
| 1987年 | 2篇 |
| 1986年 | 3篇 |
| 1985年 | 9篇 |
| 1984年 | 7篇 |
| 1981年 | 5篇 |
| 1980年 | 1篇 |
| 1979年 | 1篇 |
| 1978年 | 2篇 |
| 1977年 | 1篇 |
| 1975年 | 1篇 |
| 1974年 | 2篇 |
| 1970年 | 1篇 |
| 1969年 | 1篇 |
| 1968年 | 2篇 |
| 1967年 | 2篇 |
| 1966年 | 1篇 |
排序方式： 共有199条查询结果，搜索用时 0 毫秒
191.
192.
Adolf K. Paul 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(10):51-54
Deviations from horizontal stratification in the F-region can cause significant errors in electron density profile calculations from ionograms. Such situations exist every day during sunrise and sunset. Angle of arrival measurements and studies of the variation of other F-region parameters indicate that gravity waves are frequently strong enough to produce effects of comparable magnitudes. Ray tracing model studies permit a first order estimate of the resulting errors which are largest for the peak parameters. 相似文献
193.
Paul B. Larsen 《Space Policy》2000,16(2)
This paper discusses a range of legal issues that need to be considered in planning for a space solar power system. Because objects placed in space are inherently international, the paper primarily looks at international law that affects launching, construction, operation, property rights, the environment, communication and liability. International coordination early in the planning process is urged to make space solar powers systems a reality more speedily. 相似文献
194.
James A. Blake Paul Chote Don Pollacco William Feline Grant Privett Andrew Ash Stuart Eves Arthur Greenwood Nick Harwood Thomas R. Marsh Dimitri Veras Christopher Watson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):360-370
Recent anomalies exhibited by satellites and rocket bodies have highlighted that a population of faint debris exists at geosynchronous (GEO) altitudes, where there are no natural removal mechanisms. Despite previous optical surveys probing to around 10–20 cm in size, regular monitoring of faint sources at GEO is challenging, thus our knowledge remains sparse. It is essential that we continue to explore the faint debris population using large telescopes to better understand the risk posed to active GEO satellites. To this end, we present photometric results from a survey of the GEO region carried out with the 2.54 m Isaac Newton Telescope in La Palma, Canary Islands. We probe to 21st visual magnitude (around 10 cm, assuming Lambertian spheres with an albedo of 0.1), uncovering 129 orbital tracks with GEO-like motion across the eight nights of dark-grey time comprising the survey. The faint end of our brightness distribution continues to rise until the sensitivity limit of the sensor is reached, suggesting that the modal brightness could be even fainter. We uncover a number of faint, uncatalogued objects that show photometric signatures of rapid tumbling, many of which straddle the limiting magnitude of our survey over the course of a single exposure, posing a complex issue when estimating object size. This work presents the first instalment of DebrisWatch, an ongoing collaboration between the University of Warwick and the Defence Science and Technology Laboratory (UK) investigating the faint population of GEO debris. 相似文献
195.
Conclusions Passive observation of the naturally occurring γ-ray and X-ray from the planets is potentially an important technique for determining their gross chemical composition and on the basis of natural γ-radiation determining if the planetary surface is composed of differential material. If the planet is not covered by a thick atmosphere then it is possible to map the distribution of the most abundant elements on a scale of spatial resolution that is of the order of the altitude at which the observations are made. Initial observations carried out from lunar orbit have shown that the flux levels are approximately as expected and that the lunar surface is not characterized by any widespread distribution of acidic rocks in the region observed by the Luna 10 spacecraft. 相似文献
196.
197.
货舱和行李舱所受的磨损程度仅次于机轮和刹车装置。这是因为在货物装卸过程中,货舱及行李舱受到日复一日的损坏。货舱和行李舱也是腐蚀最多的部位,而且在飞机进行大修检查前是无法察觉的。 相似文献
198.
G. Randall Gladstone S. Alan Stern Kurt D. Retherford Ronald K. Black David C. Slater Michael W. Davis Maarten H. Versteeg Kristian B. Persson Joel W. Parker David E. Kaufmann Anthony F. Egan Thomas K. Greathouse Paul D. Feldman Dana Hurley Wayne R. Pryor Amanda R. Hendrix 《Space Science Reviews》2010,150(1-4):161-181
199.
Paul Morgan Matthias Grott Brigitte Knapmeyer-Endrun Matt Golombek Pierre Delage Philippe Lognonné Sylvain Piqueux Ingrid Daubar Naomi Murdoch Constantinos Charalambous William T. Pike Nils Müller Axel Hagermann Matt Siegler Roy Lichtenheldt Nick Teanby Sharon Kedar 《Space Science Reviews》2018,214(6):104
This article discusses relevant physical properties of the regolith at the Mars InSight landing site as understood prior to landing of the spacecraft. InSight will land in the northern lowland plains of Mars, close to the equator, where the regolith is estimated to be (geq3mbox{--}5~mbox{m}) thick. These investigations of physical properties have relied on data collected from Mars orbital measurements, previously collected lander and rover data, results of studies of data and samples from Apollo lunar missions, laboratory measurements on regolith simulants, and theoretical studies. The investigations include changes in properties with depth and temperature. Mechanical properties investigated include density, grain-size distribution, cohesion, and angle of internal friction. Thermophysical properties include thermal inertia, surface emissivity and albedo, thermal conductivity and diffusivity, and specific heat. Regolith elastic properties not only include parameters that control seismic wave velocities in the immediate vicinity of the Insight lander but also coupling of the lander and other potential noise sources to the InSight broadband seismometer. The related properties include Poisson’s ratio, P- and S-wave velocities, Young’s modulus, and seismic attenuation. Finally, mass diffusivity was investigated to estimate gas movements in the regolith driven by atmospheric pressure changes. Physical properties presented here are all to some degree speculative. However, they form a basis for interpretation of the early data to be returned from the InSight mission. 相似文献