全文获取类型
收费全文 | 303篇 |
免费 | 69篇 |
国内免费 | 69篇 |
专业分类
航空 | 216篇 |
航天技术 | 103篇 |
综合类 | 28篇 |
航天 | 94篇 |
出版年
2024年 | 1篇 |
2023年 | 5篇 |
2022年 | 16篇 |
2021年 | 8篇 |
2020年 | 18篇 |
2019年 | 9篇 |
2018年 | 19篇 |
2017年 | 18篇 |
2016年 | 23篇 |
2015年 | 18篇 |
2014年 | 39篇 |
2013年 | 12篇 |
2012年 | 24篇 |
2011年 | 32篇 |
2010年 | 22篇 |
2009年 | 22篇 |
2008年 | 18篇 |
2007年 | 24篇 |
2006年 | 10篇 |
2005年 | 17篇 |
2004年 | 13篇 |
2003年 | 7篇 |
2002年 | 10篇 |
2001年 | 7篇 |
2000年 | 6篇 |
1999年 | 12篇 |
1998年 | 2篇 |
1997年 | 2篇 |
1996年 | 3篇 |
1995年 | 4篇 |
1994年 | 6篇 |
1993年 | 3篇 |
1992年 | 2篇 |
1991年 | 2篇 |
1990年 | 3篇 |
1989年 | 1篇 |
1988年 | 2篇 |
1984年 | 1篇 |
排序方式: 共有441条查询结果,搜索用时 15 毫秒
101.
102.
103.
We analyzed UVCS/SOHO data and compared the H I Lyα (121.6 nm) and O VI (103.2 nm, 103.7 nm) emission in the polar and equatorial
coronal holes. We found that the emission lines have similar characteristics in these two types of coronal holes. Both types
show evidence for superradially diverging boundaries. The latitudinal distribution of the O VI line ratio may indicate that
the equatorial coronal hole has O+5 outflow velocities lower than in the polar coronal holes.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
104.
R. M. Suleiman J.L. Kohl A. V. Panasyuk A. Ciaravella S.R. Cranmer L.D. Gardner R. Frazin R. Hauck P.L. Smith G. Noci 《Space Science Reviews》1999,87(1-2):327-330
The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure
spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance
is believed to become frozen.
In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity
distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been
corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic
height from 1.5 to 2.5 R⊙ and decrease with height from 3.5 to 5 R⊙.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
105.
106.
提出了某型机VHF电台通讯距离短的问题,简述了对某型机VHF电台进行地面试验、空中作用距离试飞情况。并用通讯原理,对VHF电台通讯距离短进行了理论分析,采取了整改措施。最终解决了某型飞机VHF电台通讯距离短的问题,使飞行通讯联络正常。 相似文献
107.
UV P-Cygni profiles of OB-stars in the Magellanic Clouds (observed with HST), and the galaxy (observed with IUE) are analyzed empirically using a line formation procedure similar to the one described by Lamers et al. (1987). The assumption of a constant microturbulencev
turb throughout the wind is dropped and replaced by a radially increasing turbulence parameterv
turb(v), thus improving the fit for the emission peaks substantially, and at the same time avoiding the need for a justification of extremely supersonic turbulence in the vicinity of the wind's sonic point. The Sobolev optical depth is determined interatively at fixed velocities in the wind, which removes the bias introduced by the choice of a specific parameterization function. Where it was possible and necessary a full photospheric spectrum was used to illuminate the wind line. The terminal velocitiesv
are are found to be largest in the Galaxy, smallest in the Small Magellanic Cloud, and intermediate or similar to galactic in the Large Cloud. 相似文献
108.
研究一种用于近程弹道式地-地弹的导引法,它是借用空-空弹常值目标方位角导引法的概念,把它改变成按弹道设计需要而变化的目标方位角导引法,去攻击地面固定目标,它有减小气动阻力,提高命中相对精度的优点,称它为变目标方位角导引法。 相似文献
109.
针对仅有相对距离测量信息的近圆轨道航天器近程交会问题,首次提出一种基于传感器偏离航天器质心安装杆臂效应的解析初始相对定轨算法,解决了仅测距定轨存在镜像解的模糊性问题。首先给出了仅测距定轨模糊性的数学解释,然后基于Clohessy-Wiltshire动力学模型和传感器偏心安装的杆臂效应推导了仅测距信息情况下的初始相对轨道解析解,并给出系统能够去模糊的传感器安装条件。最后通过无误差仿真验证了所提算法的有效性,通过误差情况下的Monte Carlo仿真分析了算法的定轨性能。仿真结果表明所提算法有效,在满足传感器偏心安装条件下能够实现较为精确的初始相对定轨。 相似文献
110.