全文获取类型
收费全文 | 826篇 |
免费 | 86篇 |
国内免费 | 39篇 |
专业分类
航空 | 110篇 |
航天技术 | 437篇 |
综合类 | 9篇 |
航天 | 395篇 |
出版年
2023年 | 22篇 |
2022年 | 15篇 |
2021年 | 31篇 |
2020年 | 18篇 |
2019年 | 21篇 |
2018年 | 20篇 |
2017年 | 2篇 |
2016年 | 18篇 |
2015年 | 27篇 |
2014年 | 35篇 |
2013年 | 40篇 |
2012年 | 43篇 |
2011年 | 46篇 |
2010年 | 43篇 |
2009年 | 28篇 |
2008年 | 25篇 |
2007年 | 61篇 |
2006年 | 41篇 |
2005年 | 52篇 |
2004年 | 36篇 |
2003年 | 34篇 |
2002年 | 28篇 |
2001年 | 29篇 |
2000年 | 40篇 |
1999年 | 33篇 |
1998年 | 29篇 |
1997年 | 25篇 |
1996年 | 23篇 |
1995年 | 16篇 |
1994年 | 16篇 |
1993年 | 10篇 |
1992年 | 8篇 |
1991年 | 12篇 |
1990年 | 5篇 |
1989年 | 5篇 |
1988年 | 6篇 |
1987年 | 6篇 |
1984年 | 2篇 |
排序方式: 共有951条查询结果,搜索用时 31 毫秒
241.
Myrtille Laas-Bourez Sébastien Wailliez Florent Deleflie Alain Klotz Dominique Albanese Nathalie Saba 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The MéO (for Métrologie Optique) telescope is the Satellite and Lunar Laser Ranging (SLR) dedicated telescope of Observatoire de la Côte d’Azur (France) located at plateau de Calern. The telescope uses an altazimuth mount. The motorization of the mount has a capability of 6 deg/s allowing the follow up of Low Earth Orbits (LEO) satellites, as well as Medium Earth Orbits (MEO) and geostationary (GEO) satellites, and the Moon. The telescope has a primary mirror of 1.54 m. It uses a Nasmyth focus equipped with an EMCCD camera. The telescope field of view, defined by the equivalent focal length and the size of the camera, is currently 3.4 arcmin × 3.4 arcmin. 相似文献
242.
F.J. Montojo T. López Moratalla C. Abad 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In the project titled “Astrometric Positioning of Geostationary Satellite” (PASAGE), carried out by the Real Instituto y Observatorio de la Armada (ROA), optical observation techniques were developed to allow satellites to be located in the geostationary ring with angular accuracies of up to a few tenths of an arcsec. These techniques do not necessarily require the use of large telescopes or especially dark areas, and furthermore, because optical observation is a passive method, they could be directly applicable to the detection and monitoring of passive objects such as space debris in the geostationary ring. 相似文献
243.
Multi-point observations and modeling of subauroral polarization streams (SAPS) and double-peak subauroral ion drifts (DSAIDs): A case study 总被引:1,自引:0,他引:1
Dong Wei Yiqun Yu Aaron J. Ridley Jinbin Cao Malcolm W. Dunlop 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3522-3535
While subauroral polarization streams (SAPS) are well recognized as representatively one of the most important features of magnetosphere-ionosphere (M-I) coupling processes in the subauroral region, the double-peak subauroral ion drifts (DSAIDs) is a newly recognized ionospheric phenomenon, categorized as a subset of subauroral ion drifts (SAIDs). In this study, we investigate both SAPS and DSAIDs that appear during the storm main phase of the 17 March 2015 event through a combination of multi-point observations and numerical simulations. We find that when SAPS/DSAIDs are observed by the DMSP spacecraft near the dusk subauroral region, strong electric fields are detected minutes later by the Van Allen Probes almost in the same conjugate region near the equatorial plane. Numerical simulations are carried out not only to reveal the global context and dynamic evolution of the SAPS in both the magnetospheric and ionospheric systems, but also to aid the understanding of the effect of conductance on the DSAIDs. Our results confirm that SAPS are indeed associated with Region 2 field-aligned currents (FACs) flowing into the low conductance region. On the other hand, the DSAIDs may be related to the double-conductance-trough in the subauroral region. 相似文献
244.
245.
A. Sprague J. Warell G. Cremonese Y. Langevin J. Helbert P. Wurz I. Veselovsky S. Orsini A. Milillo 《Space Science Reviews》2007,132(2-4):399-431
Mercury’s surface is thought to be covered with highly space-weathered silicate material. The regolith is composed of material
accumulated during the time of planetary formation, and subsequently from comets, meteorites, and the Sun. Ground-based observations
indicate a heterogeneous surface composition with SiO2 content ranging from 39 to 57 wt%. Visible and near-infrared spectra, multi-spectral imaging, and modeling indicate expanses
of feldspathic, well-comminuted surface with some smooth regions that are likely to be magmatic in origin with many widely
distributed crystalline impact ejecta rays and blocky deposits. Pyroxene spectral signatures have been recorded at four locations.
Although highly space weathered, there is little evidence for the conversion of FeO to nanophase metallic iron particles (npFe0), or “iron blebs,” as at the Moon. Near- and mid-infrared spectroscopy indicate clino- and ortho-pyroxene are present at
different locations. There is some evidence for no- or low-iron alkali basalts and feldspathoids. All evidence, including
microwave studies, point to a low iron and low titanium surface. There may be a link between the surface and the exosphere
that may be diagnostic of the true crustal composition of Mercury. A structural global dichotomy exists with a huge basin
on the side not imaged by Mariner 10. This paper briefly describes the implications for this dichotomy on the magnetic field
and the 3 : 2 spin : orbit coupling. All other points made above are detailed here with an account of the observations, the
analysis of the observations, and theoretical modeling, where appropriate, that supports the stated conclusions. 相似文献
246.
最严重充电条件下航天器的瞬态充电模拟研究 总被引:2,自引:1,他引:2
运用等效电路模式理论推导出随时间变化充电问题的微分方程组,针对最严重情况构造了解决瞬态充电问题的程序,对ATS-6卫星的二种情况运用这个程序进行了计算。讨论了航天器不同材料对充放电的影响。 相似文献
247.
镜反射凹面及相互可视表面的轨道外热流计算 总被引:6,自引:0,他引:6
通过对空间表面所受外热流以及镜反射表面所具有的特性的分析,提出了采用蒙特卡罗法计算镜反射凹面及镜反射相互可视表面的轨道热流的方法,并对半球凹面和两相互垂直可视平板的轨道热流进行了计算。 相似文献
248.
G. Setti G. Zamorani 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
We review the present knowledge on the cosmological evolution of quasars, by discussing some of the recent results obtained from studies of optically selected objects. Despite the fast development of prism survey tecniques, the color selection still appears to be the best tecnique for constructing the complete samples which are necessary for statistical studies. It is shown, however, that even the best available complete samples of quasars selected on the basis of ultraviolet excess (z < 2.2) are not sufficient to univocally determine the “correct” evolutionary model. Moreover, some preliminary results suggest that the evolution law derived from quasars with mB<20 and z<2.2 can not be extrapolated to fainter magnitudes and higher redshifts. On the basis of what is known today about the optical and X-ray properties of quasars, we then discuss some of teh possible results, relevant to cosmology, which can be achieved with future coordinated optical and X-ray observations of quasars. 相似文献
249.
提出了航天器稀疏编队飞行的概念及其设计方法,阐明了它与通常的紧密编队飞行的区别及其在应用上的前景。采用了一个比Hill解更为广泛的新公式来设计稀疏编队,并列举了若干稀疏编队的阵形。当各航天器距离很近时,该公式自然退化为与Hill解相同的形式。通过与Hill解的设计相比较,表明了新公式用于稀疏编队设计的优越性。 相似文献
250.