全文获取类型
收费全文 | 1998篇 |
免费 | 303篇 |
国内免费 | 247篇 |
专业分类
航空 | 1068篇 |
航天技术 | 1038篇 |
综合类 | 125篇 |
航天 | 317篇 |
出版年
2024年 | 5篇 |
2023年 | 49篇 |
2022年 | 54篇 |
2021年 | 94篇 |
2020年 | 106篇 |
2019年 | 98篇 |
2018年 | 93篇 |
2017年 | 69篇 |
2016年 | 82篇 |
2015年 | 89篇 |
2014年 | 157篇 |
2013年 | 131篇 |
2012年 | 129篇 |
2011年 | 167篇 |
2010年 | 126篇 |
2009年 | 161篇 |
2008年 | 142篇 |
2007年 | 102篇 |
2006年 | 67篇 |
2005年 | 107篇 |
2004年 | 48篇 |
2003年 | 42篇 |
2002年 | 44篇 |
2001年 | 46篇 |
2000年 | 42篇 |
1999年 | 36篇 |
1998年 | 41篇 |
1997年 | 37篇 |
1996年 | 18篇 |
1995年 | 24篇 |
1994年 | 41篇 |
1993年 | 17篇 |
1992年 | 24篇 |
1991年 | 22篇 |
1990年 | 16篇 |
1989年 | 9篇 |
1988年 | 11篇 |
1987年 | 1篇 |
1986年 | 1篇 |
排序方式: 共有2548条查询结果,搜索用时 218 毫秒
931.
932.
圆柱体垂直入水空泡形态试验 总被引:2,自引:2,他引:2
在不同攻角和不同速度条件下,对圆柱形运动体垂直入水空泡形态进行试验研究.对140°锥角头型圆柱体在零攻角和带攻角条件下进行垂直入水试验,分析了低速垂直入水所引起的入水空泡生成、发展和闭合流动过程以及空泡稳定性等;利用平头圆柱体进行不同速度条件下垂直入水试验,分析了入水速度对空泡闭合方式和形态的影响.研究结果表明:在试验速度范围内均能形成稳定的入水空泡,并经历生成、充分发展、空泡闭合以及最后完全脱落的过程,不同发展阶段具有不同的稳定性,其闭合方式和形态与入水速度密切相关. 相似文献
933.
934.
三轴稳定卫星平台搭载的光学有效载荷都存在午夜太阳辐射干扰问题,由此产生的热变形效应对光学系统的成像品质影响显著。采用复杂外热流近似建模技术,以及多软件耦合有限元仿真方法,以FY-4卫星的扫描辐射计为应用背景,研究了昼夜太阳辐射对星载辐射计扫描镜产生的热效应,并对不同热设计条件下的工况进行了对比分析。分析结果显示:扫描镜侧面及背面的热控涂层选取对其热变形有重要影响,但是仅仅通过热设计解决温度波动和热变形的矛盾是不够的,需要通过改进扫描镜的材料和优化光机结构加以改善。 相似文献
935.
936.
937.
H.S. Ahluwalia R.C. Ygbuhay 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The annual mean sunspot number (SSN) has a minimum value in 2008, while the monthly mean SSN has a value of zero in August 2009. The galactic cosmic ray modulation for cycle 24 began at earth orbit in January 2010. We study the onset characteristics of the new modulation cycle using data from the global network of neutron monitors. They respond to time variations in different segments of the galactic cosmic ray rigidity spectrum. The corresponding temporal variations in the interplanetary magnetic field intensity (B) and solar wind velocity (V) as well as the tilt angle of the heliospheric current sheet are also studied. There is a lag of 3 months between a large, sharp increase of the tilt angle of the heliospheric current sheet and the onset of modulation. Some neutron monitors are undergoing long-term drifts of unknown origin. 相似文献
938.
M.D. Ngobeni M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Observations made with the two Voyager spacecraft confirmed that the solar wind decelerates to form the heliospheric termination shock. Voyager 1 crossed this termination shock at ∼94 AU in 2004, while Voyager 2 crossed it in 2007 at a different heliolatitude, about 10 AU closer to the Sun. These different positions of the termination shock confirm the dynamic and cyclic nature of the shock’s position. Observations from the two Voyager spacecraft inside the heliosheath indicate significant differences between them, suggesting that apart from the dynamic nature caused by changing solar activity there also may exist a global asymmetry in the north–south (polar) dimensions of the heliosphere, in addition to the expected nose–tail asymmetry. This relates to the direction in which the heliosphere is moving in interstellar space and its orientation with respect to the interstellar magnetic field. In this paper we focus on illustrating the effects of this north–south asymmetry on modulation of galactic cosmic ray Carbon, between polar angles of 55° and 125°, using a numerical model which includes all four major modulation processes, the termination shock and the heliosheath. This asymmetry is incorporated in the model by assuming a significant dependence on heliolatitude of the thickness of the heliosheath. When comparing the computed spectra between the two polar angles, we find that at energies E < ∼1.0 GeV the effects of the assumed asymmetry on the modulated spectra are insignificant up to 60 AU from the Sun but become increasingly more significant with larger radial distances to reach a maximum inside the heliosheath. In contrast, with E > ∼1.0 GeV, these effects remain insignificant throughout the heliosphere even very close to the heliopause. Furthermore, we find that a higher local interstellar spectrum for Carbon enhances the effects of asymmetric modulation between the two polar angles at lower energies (E < ∼300 MeV). In conclusion, it is found that north–south asymmetrical effects on the modulation of cosmic ray Carbon depend strongly on the extent of the geometrical asymmetry of the heliosheath together with the assumed value of the local interstellar spectrum. 相似文献
939.
P.R. Fagundes V. Klausner J.A. Bittencourt Y. Sahai J.R. Abalde 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The occurrence of an additional F3-layer has been reported at Brazilian, Indian and Asian sectors by several investigators. In this paper, we report for the first time the seasonal variations of F3-layer carried out near the southern crest of the equatorial ionospheric anomaly (EIA) at São José dos Campos (23.2°S, 45.0°W; dip latitude 17.6°S – Brazil) as a function of solar cycle. The period from September 2000 to August 2001 is used as representative of high solar activity (HSA) and the period from January 2006 to December 2006 as representative of low solar activity (LSA). This investigation shows that during HSA there is a maximum occurrence of F3-layer during summer time and a minimum during winter time. However, during LSA, there is no seasonal variation in the F3-layer occurrence. Also, the frequency of occurrence of the F3-layer during HSA is 11 times more than during LSA. 相似文献
940.
Ji Wu Weiying Sun Jianhua Zheng Cheng Zhang Hao Liu Jingye Yan Chi Wang Chuanbing Wang Shui Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Coronal mass ejections (CMEs) represent a great concentration of mass and energy input into the lower corona. They have come to be recognized as the major driver of physical conditions change in the Sun–Earth system. Consequently, observations of CMEs are important for understanding and ultimately predicting space weather conditions. This paper discusses a proposed mission, the Solar Polar Orbit Radio Telescope (SPORT) mission, which will observe the propagation of interplanetary CMEs to distances of near 0.35 AU from the Sun. The orbit of SPORT is an elliptical solar polar orbit. The inclination angle between the orbit and ecliptic plane should be about 90°. The main payload on board SPORT will be an imaging radiometer working at the meter wavelength band (radio telescope), which can follow the propagation of interplanetary CMEs. The images that are obtained by the radio telescope embody the brightness temperature of the objectives. Due to the very large size required for the antenna aperture of the radio telescope, we adopt interferometric imaging technology to reduce it. Interferometric imaging technology is based on indirect spatial frequency domain measurements plus Fourier transformation. The SPORT spacecraft will also be equipped with a set of optical and in situ measurement instruments such as a EUV solar telescope, a solar wind ion instrument, an energetic particle detector, a magnetometer, a wave detector and a solar radio burst spectrometer. 相似文献