全文获取类型
收费全文 | 3219篇 |
免费 | 831篇 |
国内免费 | 462篇 |
专业分类
航空 | 1535篇 |
航天技术 | 1169篇 |
综合类 | 168篇 |
航天 | 1640篇 |
出版年
2024年 | 34篇 |
2023年 | 120篇 |
2022年 | 133篇 |
2021年 | 178篇 |
2020年 | 140篇 |
2019年 | 140篇 |
2018年 | 165篇 |
2017年 | 118篇 |
2016年 | 146篇 |
2015年 | 166篇 |
2014年 | 275篇 |
2013年 | 195篇 |
2012年 | 259篇 |
2011年 | 280篇 |
2010年 | 210篇 |
2009年 | 216篇 |
2008年 | 203篇 |
2007年 | 224篇 |
2006年 | 167篇 |
2005年 | 167篇 |
2004年 | 108篇 |
2003年 | 111篇 |
2002年 | 91篇 |
2001年 | 111篇 |
2000年 | 72篇 |
1999年 | 62篇 |
1998年 | 64篇 |
1997年 | 56篇 |
1996年 | 40篇 |
1995年 | 47篇 |
1994年 | 38篇 |
1993年 | 32篇 |
1992年 | 29篇 |
1991年 | 24篇 |
1990年 | 36篇 |
1989年 | 13篇 |
1988年 | 18篇 |
1987年 | 14篇 |
1986年 | 2篇 |
1985年 | 1篇 |
1984年 | 6篇 |
1981年 | 1篇 |
排序方式: 共有4512条查询结果,搜索用时 640 毫秒
1.
Alexis Petit Alessandro Rossi Elisa Maria Alessi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(12):4177-4192
The Earth orbital environment is drastically changing due to an intensification of the space activities. In particular, several projects of large constellations, proposed for the next years for communications purpose like global internet access, Internet of Things, or for Earth observations, will lead to the deployment of several thousands of new satellites at an unprecedented rate. It is a crucial challenge for space traffic management, which will deal with a great number of satellite conjunctions, potentially causing a collision with damaging consequences for the constellation itself and the space environment sustainability.In this paper, we investigate the close approach frequency and the cumulative collision probability for each referenced constellation. For this purpose, we compute the orbital evolution of satellites in different constellations during the lifecycle, from the deployment to the decommissioning, and we apply the CUBE algorithm and the Foster method to assess the collision probability with the background space debris population assuming a constant uncertainty in position. We show the variation of risk defined by the close approach frequency and the cumulative collision probability as a function of the proposed configuration. In particular, satellites of the Iridium and Kuiper constellation, but also satellite of the Telesat constellation on polar orbits are the most exposed at a collision. Moreover, the decommissioning phase contribute for a major part to the final cumulative collision probability. 相似文献
2.
3.
Yi Wei Qingjun Li Fangnuan Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):393-400
A new orbit-attitude-vibration coupled dynamic model of the tethered solar power satellite (Tethered SPS) is established based on absolute nodal coordinate formulation. The Hamilton’s equation of the system is derived by introducing generalized momentum through Legendre transformation. The correctness of the proposed model is verified by an example. The dynamic characteristics of the Tethered SPS are studied using the symplectic Runge-Kutta method. Simulation results show that the orbital radius and the total energy of the system are well preserved. The attitude of the system is unstable when the mass of the bus system is small. However, the attitude stability is dependent on some other parameters of the system, which requires further studies. It is also found that the average tether force/deformation can be roughly estimated by simplifying the solar panel as a particle. The proposed model can be used to study the orbit-attitude-vibration coupled dynamics and control problems. 相似文献
4.
Nurollah Tatar Mohammad Saadatseresht Hossein Arefi Ahmad Hadavand 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(11):2787-2800
Unwanted contrast in high resolution satellite images such as shadow areas directly affects the result of further processing in urban remote sensing images. Detecting and finding the precise position of shadows is critical in different remote sensing processing chains such as change detection, image classification and digital elevation model generation from stereo images. The spectral similarity between shadow areas, water bodies, and some dark asphalt roads makes the development of robust shadow detection algorithms challenging. In addition, most of the existing methods work on pixel-level and neglect the contextual information contained in neighboring pixels. In this paper, a new object-based shadow detection framework is introduced. In the proposed method a pixel-level shadow mask is built by extending established thresholding methods with a new C4 index which enables to solve the ambiguity of shadow and water bodies. Then the pixel-based results are further processed in an object-based majority analysis to detect the final shadow objects. Four different high resolution satellite images are used to validate this new approach. The result shows the superiority of the proposed method over some state-of-the-art shadow detection method with an average of 96% in F-measure. 相似文献
5.
6.
Aprajita Verma Vassilis Charmandaris Ulrich Klaas Dieter Lutz Martin Haas 《Space Science Reviews》2005,119(1-4):355-407
Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction
of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory
(ISO) have provided a relatively unabsorbed view to the sources fuelling this active emission. The improved sensitivity, spatial
resolution and spectroscopic capability of ISO over its predecessor Infrared Astronomical Satellite (IRAS) of enabled significant
advances in the understanding of the infrared properties of active galaxies. ISO surveyed a wide range of active galaxies
which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing
a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many
nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines
as well as broad band features in the mid- and far-infrared. This was particularly useful, since it resulted in the understanding
of the power production, excitation and fuelling mechanisms in the nuclei of active galaxies including the intriguing but
so far elusive ultraluminous infrared galaxies. Detailed studies of various classes of AGN and quasars greatly improved our
understanding of the unification scenario. Far-infrared imaging and photometry revealed the presence of a new very cold dust
component in galaxies and furthered our knowledge of the far-infrared properties of faint starbursts, ULIGs and quasars. We
summarise almost nine years of key results based on ISO data spanning the full range of luminosity and type of active galaxies. 相似文献
7.
8.
介绍了卫星在热平衡试验后所发现的有效载荷的污染情况,通过对污染提取物的分析和试验设备的再次污染监测,找出了污染源,并对以后的防污染工作提供了借鉴. 相似文献
9.
从防空导弹地面电源--热电池的热设计和工艺角度出发,分析影响电池工作寿命的因素,提出延长电池工作寿命的三条途径:合理控制热电池的内部热量;提高加热片的均匀性;合理选择外保温材料。实践证明,这些途径是可行的。 相似文献
10.
Mauro Orlandini 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2742-2746
Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1. 相似文献