全文获取类型
收费全文 | 340篇 |
免费 | 57篇 |
国内免费 | 18篇 |
专业分类
航空 | 100篇 |
航天技术 | 166篇 |
综合类 | 10篇 |
航天 | 139篇 |
出版年
2023年 | 8篇 |
2022年 | 17篇 |
2021年 | 17篇 |
2020年 | 19篇 |
2019年 | 15篇 |
2018年 | 10篇 |
2017年 | 4篇 |
2016年 | 6篇 |
2015年 | 10篇 |
2014年 | 16篇 |
2013年 | 11篇 |
2012年 | 20篇 |
2011年 | 30篇 |
2010年 | 23篇 |
2009年 | 19篇 |
2008年 | 17篇 |
2007年 | 32篇 |
2006年 | 16篇 |
2005年 | 8篇 |
2004年 | 15篇 |
2003年 | 10篇 |
2002年 | 7篇 |
2001年 | 13篇 |
2000年 | 9篇 |
1999年 | 15篇 |
1998年 | 9篇 |
1997年 | 5篇 |
1996年 | 7篇 |
1995年 | 5篇 |
1994年 | 6篇 |
1993年 | 1篇 |
1992年 | 8篇 |
1991年 | 2篇 |
1990年 | 3篇 |
1989年 | 1篇 |
1987年 | 1篇 |
排序方式: 共有415条查询结果,搜索用时 15 毫秒
171.
R.L.C. Starling E.M. Puchnarewicz E. Romero-Colmenero K.O. Mason 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2588-2593
We present a series of monitoring observations of the ultrasoft broad-line Seyfert galaxy RE J2248-511 with XMM-Newton. Previous X-ray observations showed a transition from a very soft state to a harder state five years later. We find that the ultrasoft X-ray excess has re-emerged, yet there is no change in the hard power-law. Reflection models with a reflection fraction of 15, and Comptonisation models with two components of different temperatures and optical depths (kT1 = 83 keV, T1 = 30 eV, τ1 = 0.8; KT2 = 3.5 keV, T2 = 60 eV, τ2 = 2.8) can be fit to the spectrum, but cannot be constrained. The best representation of the spectrum is a model consisting of two blackbodies (kT1 = 0.09 ± 0.01 keV, kT2 = 0.21 ± 0.03 keV) plus a power-law (Γ = 1.8 ± 0.08). We also present simultaneous optical and infrared data showing that the optical spectral slope also changes dramatically on timescales of years. If the optical to X-ray flux comes primarily from a Comptonised accretion disk we obtain estimates for the black hole mass , accretion rate and inclination cos(i) 0.8 of the disk. 相似文献
172.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(1):624-644
The integration of geosynchronous orbit (GSO) satellites in Global Navigation Satellite Systems (GNSS) is mostly discussed to enable a regional enhancement for tracking. But how do GSO satellites affect the orbit determination of the rest of the constellation? How accurately can these orbits be determined in a future GNSS tracking scenario with optical links? In this simulation study we analyze the benefit of GSO satellites as an expansion of a MEO (Medium Earth Orbit) satellite constellation – we selected the Galileo satellite constellation – for MEO Precise Orbit Determination (POD). We address not only the impact on POD of MEO satellites but also the possibility to precisely determine the GSO satellites – geostationary orbits (GEO) and inclined geosynchronous orbits (IGSO) – in such an expanded MEO constellation. In addition to GNSS microwave observations, we analyze the influence of different optical links between the participating entities: Optical two-way Inter-Satellite Links (OISL) and ground-space oriented Optical Two-Way Links (OTWL). These optical measurements together with the GNSS microwave observations give a remarkable benefit for the POD capability. In the case of GNSS and OTWL, we simulate the measurements with regard to a network of 16 ground stations. We pay great attention to the simulation of systematic effects of all measurement techniques. We discuss the influence on the systematic errors as well as the formal orbit uncertainties. A MEO constellation expanded with GSO satellites as well as the use of optical links together with GNSS observations not only improves the MEO satellite orbits but also the GSOs to a great extent. 相似文献
173.
Peter W. A. Roming Thomas E. Kennedy Keith O. Mason John A. Nousek Lindy Ahr Richard E. Bingham Patrick S. Broos Mary J. Carter Barry K. Hancock Howard E. Huckle S D. Hunsberger Hajime Kawakami Ronnie Killough T Scott Koch Michael K. Mclelland Kelly Smith Philip J. Smith Juan Carlos Soto Patricia T. Boyd Alice A. Breeveld Stephen T. Holland Mariya Ivanushkina Michael S. Pryzby Martin D. Still Joseph Stock 《Space Science Reviews》2005,120(3-4):95-142
The Ultra-Violet/Optical Telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (∼1 min) UV and optical photons from the afterglow of gamma-ray
bursts in the 170–600 nm band as well as long term observations of these afterglows. This is accomplished through the use
of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey–Chrétien design with micro-channel plate intensified
charged-coupled device detectors that record the arrival time of individual photons and provide sub-arcsecond positioning
of sources. We discuss some of the science to be pursued by the UVOT and the overall design of the instrument. 相似文献
174.
175.
扫描角监控器是CBERS_1卫星红外多光谱扫描仪(IRMSS)中的重要部件。文章主要介绍了扫描角监控器的工作原理、主要技术指标以及研制过程中的技术状态、技术难点、关键技术和质量保证。最后对国内外相关的技术项目及经济社会效益情况做了简要对比和分析 相似文献
176.
图像处理作为成像链路的重要组成部分,是系统优化设计不得不考虑的一个环节,其中调制传递函数补尝(MTFC)是当今研究的热点,在遥感成像系统优化设计中发挥着重要作用。如果综合应用地面MTFC的能力,对遥感器进行优化设计,则可以大大减轻遥感器的研制难度、节约成本和缩短研制周期。该文对MTFC在光学遥感成像系统优化设计中的应用进行了一些探讨。 相似文献
177.
178.
多光谱多镜头CCD相机的光学配准 总被引:3,自引:0,他引:3
文章分析了多光谱多镜头CCD相机光学配准的重要性 ,以及影响多光谱多镜头CCD相机的光学配准的各种技术因素 相似文献
179.
180.
提出了一种新的立体影像解析方法。在卫星轨道特性和相机交会角已知的条件下,根据对同一地物的摄影时间差提取高度信息,进而确定其三维空间位置。建立了不考虑/考虑地球自转的地物高度测定,以及位置确定模型,给出了地物空间位置计算的流程。讨论了地物高度的测量误差和对卫星平台性能的基本要求。新方法用摄影时间差的测量取代传统方法影像像点坐标的测量,更简捷和准确,更适合数字图像,具有重要应用价值。 相似文献