全文获取类型
收费全文 | 165篇 |
免费 | 13篇 |
国内免费 | 7篇 |
专业分类
航空 | 70篇 |
航天技术 | 75篇 |
综合类 | 6篇 |
航天 | 34篇 |
出版年
2024年 | 1篇 |
2023年 | 2篇 |
2021年 | 1篇 |
2020年 | 5篇 |
2019年 | 4篇 |
2018年 | 1篇 |
2017年 | 3篇 |
2016年 | 3篇 |
2015年 | 3篇 |
2014年 | 17篇 |
2013年 | 10篇 |
2012年 | 13篇 |
2011年 | 10篇 |
2010年 | 7篇 |
2009年 | 10篇 |
2008年 | 14篇 |
2007年 | 9篇 |
2006年 | 6篇 |
2005年 | 4篇 |
2004年 | 7篇 |
2003年 | 6篇 |
2002年 | 3篇 |
2001年 | 3篇 |
2000年 | 1篇 |
1999年 | 11篇 |
1998年 | 5篇 |
1997年 | 1篇 |
1995年 | 4篇 |
1994年 | 13篇 |
1993年 | 4篇 |
1992年 | 1篇 |
1991年 | 2篇 |
1988年 | 1篇 |
排序方式: 共有185条查询结果,搜索用时 46 毫秒
171.
172.
介绍了用紫外分光光度法测定复合固体推进剂中的叔丁基二茂铁含量。该方法简便、快速,精密度和准确度较好。推进剂中其它二茂铁衍生物也可用此方法测定. 相似文献
173.
The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) has observed the extended solar corona between 1 and 10 R· for more
than two years. We review spectroscopic and polarimetric measurements made in coronal holes, equatorial streamers, and coronal
mass ejections, as well as selected non-solar targets. UVCS/SOHO has provided a great amount of empirical information about
the physical processes that heat and accelerate the solar wind, and about detailed coronal structure and evolution.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
174.
Raymond Simons David Thilker Luciana Bianchi Ted Wyder 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The Galaxy Evolution Exporer (GALEX) has performed unprecedented imaging surveys of the Magellanic Clouds (MC) and their surrounding areas including the Magellanic Bridge (MB) in near-UV (NUV, 1771-2831 Å) and far-UV (FUV, 1344-1786 Å) bands at 5″ resolution. Substantially more area was covered in the NUV than FUV, particularly in the bright central regions, because of the GALEX FUV detector failure. The 5σ depth of the NUV imaging varies between 20.8 and 22.7 (ABmag). Such imaging provides the first sensitive view of the entire content of hot stars in the Magellanic System, revealing the presence of young populations even in sites with extremely low star-formation rate surface density like the MB, owing to high sensitivity of the UV data to hot stars and the dark sky at these wavelengths. 相似文献
175.
176.
177.
为揭示跨声速阶段仪器舱附近脉动压力的空间相关特性,以某旋成体模型为研究对象,基于风洞试验获取了仪器舱附近脉动压力载荷分布规律,计算了测点间的脉动压力空间相关系数。通过曲线拟合与归一化处理,获得了模型仪器舱脉动压力空间相关特性曲线,并研究了攻角、马赫数与雷诺数对空间相关性的影响。结果表明,该模型仪器舱脉动压力空间相关特性具有波动与衰减的特点,随着流动复杂程度的增加,其相关性逐渐降低。同时,在跨声速范围内,该模型仪器舱脉动压力空间相关特性对马赫数以及较高的雷诺数比较敏感。对脉动压力空间相关特性的研究,为飞行器结构响应分析以及载荷环境预示提供了支撑。 相似文献
178.
Hitoshi Irie Hironobu Iwabuchi Katsuyuki Noguchi Yasuko Kasai Kazuyuki Kita Hajime Akimoto 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
To investigate the feasibility of new satellite observations, including air quality (AQ) observations from geostationary (GEO) orbit, it is essential to link the measurement precision (ε) with sensor specifications in advance. The present study attempts to formulate the linkage between ε and specifications of a UV/visible sensor (signal-to-noise ratio (SNR), full width at half maximum (FWHM) of the slit function, and sampling ratio (SR)) on a GEO satellite. A sophisticated radiative transfer model (JACOSPAR) is used to calculate synthetic radiance spectra that would be measured by a UV/visible sensor observing the atmosphere over Tokyo (35.7°N, 139.7°E) from GEO orbit at 120°E longitude. The spectra, modified according to given sensor specifications, are analyzed by the differential optical absorption spectroscopy technique to estimate the ε for slant column densities of O3 and NO2. We find clear relationships: for example, the ε of the O3 slant column density (molecules cm−2) and SNR at 330 nm are linked by the equation log(ε) = −1.06 · log(SNR) + 20.71 in the UV region, and the ε of the NO2 slant column density and SNR at 450 nm are linked by log(ε) = −0.98 · log(SNR) + 18.00, at a FWHM = 0.6 nm (for the Gaussian slit function) and SR = 4. The relationships are mostly independent of other specifications (e.g., horizontal and temporal resolutions), as they affect ε primarily through SNR, providing constraints in determining the optimal SNR (and alternatively FWHM and SR) for similar UV/visible sensors dedicated for AQ studies. 相似文献
179.
180.
空间辐射环境是导致光电倍增管性能衰变甚至失效的主要原因, 由于空间辐射环境的复杂性以及飞行器在空间活动的轨道、设计寿命和光电倍增管的类型不同, 光电倍增管需要的抗辐射屏蔽要求不同. 以太阳同步轨道高能粒子辐射环境为例, 对真空紫外光电倍增管进行了辐射屏蔽的Monte-Carlo计算, 在此基础上提出了运行于该轨道上的真空紫外光电倍增管的高能粒子屏蔽优化组合. 模拟计算表明, 采用Al-W-Al三层结构的屏蔽组合形式, 其中Al层厚2mm, W厚 0.5mm,可将辐射剂量从原本的9.98× 106rad (Si)降低到 8.41× 102rad (Si), 能较好地满足实际使用要求. 相似文献