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 93 毫秒
131.
M.A. Barstow S.L. Casewell J.B. Holberg M.P. Kowalski 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The Extreme Ultraviolet wavelength range was one of the final windows to be opened up to astronomy. Nevertheless, it provides very important diagnostic tools for a range of astronomical objects, although the opacity of the interstellar medium restricts the majority of observations to sources in our own galaxy. This review gives a historical overview of EUV astronomy, describes current instrumental capabilities and examines the prospects for future facilities on small and medium-class satellite platforms. 相似文献
132.
J.B. Hutchings L. Bianchi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We use the combined photometric GALEX + SDSS database to look for populations of luminous blue star-forming galaxies. These were initially identified from such a sample at redshifts near 0.4, using SDSS spectra. We make use of the NUV, g, and i colour index previously defined in our previous paper, to separate stars and QSOs, to locate more of these unusual galaxies, to fainter limits. They are found in significant numbers in two different regions of the related colour-magnitude plot. Within these regions, we use the ensemble 7-colour photometry (FUV, NUV, u, g, r, i, z) to postulate the populations of blue star-forming galaxies at redshifts near 0.4 and 1.0, from a full photometric sample of over half a million. 相似文献
133.
研究了掺杂稀土离子Ce^3+的碱土氟化物发光体LiXAlF6:Ce^3+(X=Ca^2+,Sr^2+或Ba^2+),XBaAlF6:Ce^3+(X=Li6+,Na^+或K^+)及LiBaXF6:Ce^3+(X=Al^3+,Ga^3+或In^3+)的紫外发光特性。实验发现,在LiXAlF6=Ce^3+中,随着X元素原子序数的增大,Ce^3+的发光峰就向短波方向移动。首次研究了在XBaAlF6:Ce^3+与LiBaXF6:Ce^3+中的X元素的一价与三价离子对Ce^3+发光的影响,发现这些一价与三价离子的原子序数的变化并不影响Ce^3+的发射光谱的峰值,它们只在晶格中起着填隙和电荷补偿作用,这有利于Ce^3+的发光,使发光强度有所增强。这些紫外发光可用来增强X射线影像板中所包含的储存辐射的发光体BaFBr:Eu“的发光,使X射线影像板的显像增强。 相似文献
134.
135.
The PRISMA payload optomechanical design, a high performance instrument for a new hyperspectral mission 总被引:2,自引:0,他引:2
Demetrio Labate Massimo Ceccherini Andrea Cisbani Vittorio De Cosmo Claudio Galeazzi Lorenzo Giunti Mauro Melozzi Stefano Pieraccini Moreno Stagi 《Acta Astronautica》2009,65(9-10):1429-1436
PRISMA (PRecursore IperSpettrale della Missione Applicativa) hyperspectral instrument is an advanced hyperspectral sensor including a panchromatic camera at medium resolution. The instrument is the focus of the new Earth observation mission that a consortium of Italian companies has started developing under contract of Italian Space Agency. Key features of the instrument are the very high requirement for signal-to-noise and the high quality of data that have to be provided. To meet these demanding figures the optical system has been based on a high transmittance optical system, including a single mirror telescope and two prism spectrometers based on an innovative concept to minimize number of optical elements, while high performance detectors have been chosen for the photon detection. To provide the required data quality for the entire mission lifetime an accurate calibration unit (radiometric and spectral) will be included in the instrument optomechanical assembly. The thermo-mechanical design of the instrument is based on innovative concepts, considering that the use of prism spectrometers implies a tight control of temperature variations to guarantee the stability of all instrument features once in orbit. The presented paper describes the concepts and design principle of the optomechanical assembly of the instrument, at the present status of development. 相似文献
136.
137.
金属氧化物薄膜具有良好的光学,电学特性,因此是卫星表面热控材料防静电积累的重要材料之一。实验研究发现这些金属氧化物薄膜还是具有优良的防原子氧和抗空间辐照环境的能力,而且这种能力与成膜方法及工艺过程直接相关。经模拟原子氧环境的氧等离子体作用后,溅射镀氧化锡样品的质损明显小于蒸镀氧化铟锡薄膜的质损,而氧化铟锡薄膜的质损又小于未镀薄膜试样质损。 相似文献
138.
基于有机材料出气污染过程分析,并结合辐射化学有关理论,建立材料在紫外辐照后的分子污染模型;在ASTM E1559标准测试方法的基础上,以硅橡胶材料为污染源开展试验,测试其经过不同紫外辐照时间后的出气污染沉积量,并对辐照后材料表面的微观特性进行测试分析。根据沉积量测试结果对模型待定参数进行拟合,并结合微观测试结果,分析得到紫外辐照导致硅橡胶分子链中Si-O键以及Si-C键断裂,且部分小分子物质提前挥发,从而使得出气成分中小分子污染物含量下降,大分子污染物含量上升,并最终导致总污染量在前期有所下降,在后期显著增加。 相似文献
139.
140.
Ultraviolet spectra of a quiescent prominence observed with theHigh Resolution Telescope and Spectrograph (HRTS) are analyzed. Different techniques lead to greatly different spatial scales for the prominence structures. The UV spectra show strong variations in intensity and Doppler shift on scales larger than 1700 km. Spectroscopic diagnostics employing line intensity ratios indicate the existence of scales between 400 m to some hundred kilometers. We attempt to interpret various aspects of the prominence intensities and velocities with a multiple thread model. 相似文献