全文获取类型
收费全文 | 907篇 |
免费 | 141篇 |
国内免费 | 146篇 |
专业分类
航空 | 724篇 |
航天技术 | 300篇 |
综合类 | 59篇 |
航天 | 111篇 |
出版年
2024年 | 4篇 |
2023年 | 41篇 |
2022年 | 27篇 |
2021年 | 50篇 |
2020年 | 62篇 |
2019年 | 39篇 |
2018年 | 42篇 |
2017年 | 48篇 |
2016年 | 50篇 |
2015年 | 32篇 |
2014年 | 65篇 |
2013年 | 36篇 |
2012年 | 47篇 |
2011年 | 48篇 |
2010年 | 34篇 |
2009年 | 62篇 |
2008年 | 79篇 |
2007年 | 81篇 |
2006年 | 46篇 |
2005年 | 45篇 |
2004年 | 30篇 |
2003年 | 23篇 |
2002年 | 8篇 |
2001年 | 43篇 |
2000年 | 10篇 |
1999年 | 8篇 |
1998年 | 19篇 |
1997年 | 2篇 |
1996年 | 14篇 |
1995年 | 14篇 |
1994年 | 62篇 |
1993年 | 15篇 |
1992年 | 1篇 |
1990年 | 1篇 |
1989年 | 2篇 |
1984年 | 4篇 |
排序方式: 共有1194条查询结果,搜索用时 31 毫秒
51.
高空高速无人飞行器热控制系统设计 总被引:1,自引:0,他引:1
针对飞行时间短、速度和高度变化快、表面温度波动大的无人飞行器UAV(Unmanned Aerial Vehicles)热控制系统设计难题,提出了一种可解决实际工程问题的热分析计算方法.即把热天工况、冷天工况和标准天工况作为设计/试验工况;采用参考温度法、高超音速工程预测法或计算流体动力学CFD(Computational Fluid Dynamics)数值模拟法,确定了飞行器表面温度分布,并把其作为后续热分析数学模型的外边界条件;分析结构热容量对瞬态热载荷的影响,建立与之相应的边值问题方程,并采用有限差分法求解;根据高空高速飞行特点及瞬态热载荷值,确定仪器设备舱调温系统方案. 相似文献
52.
用矢通量分裂法求解N-S方程和Euler方程,对超音通流风扇叶栅流场进行了数值模拟,由计算结果给出的物理图象表明,叶栅通道内没有强激波,亦未出现分离回流,全叶栅流场均为超音速,说明计算的两种叶型符合设计要求,其性能有待实验检验。 相似文献
53.
T. Sbarrato L. Foschini G. Ghisellini F. Tavecchio 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The γ-ray emission of blazar jets shows a pronounced variability and this feature provides limits to the size and to the speed of the emitting region. We study the γ-ray variability of bright blazars using data from the first 18 months of activity of the Large Area Telescope on the Fermi Gamma-Ray Space Telescope. From the daily light-curves of the blazars characterized by a remarkable activity, we firstly determine the minimum variability time-scale, giving an upper limit for the size of the emitting region of the sources, assumed to be spheroidal blobs in relativistic motion. These regions must be smaller than ∼10−3 parsec. Another interesting time-scale is the duration of the outbursts. We conclude that they cannot correspond to radiation produced by a single blob moving relativistically along the jet, but they are either the signature of emission from a standing shock extracting energy from a modulated jet, or the superposition of a number of flares occurring on a shorter time-scale. We also derive lower limits on the bulk Lorentz factor needed to make the emitting region transparent for gamma-rays interacting through photon–photon collisions. 相似文献
54.
55.
L. Zampieri C. Germanà C. Barbieri G. Naletto A. Čadež I. Capraro A. Di Paola C. Facchinetti T. Occhipinti D. Ponikvar E. Verroi P. Zoccarato 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We are developing fast photon-counter instruments to study the rapid variability of astrophysical sources by time tagging photon arrival times with unprecedented accuracy, making use of a Rubidium clock and GPS receiver. The first realization of such optical photon-counters, dubbed AquEYE (the Asiago Quantum Eye), was mounted in 2008 at the 182 cm Copernicus Observatory in Asiago. AquEYE observed the Crab pulsar several times and collected data of extraordinary quality that allowed us to perform accurate optical timing of the Crab pulsar and to study the pulse shape stability on a timescale from days to years with an excellent definition. Our results reinforce the evidence for decadal stability of the inclination angle between the spin and magnetic axis of the Crab pulsar. Future realizations of our instrument will make use of the Galileo Global Navigation Satellite System (GNSS) time signal. 相似文献
56.
Silvia Zane Roberto Turolla Luciano Nobili Nanda Rea 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In this paper, we discuss our first attempts to model the broadband persistent emission of magnetars within a self-consistent, physical scenario. We present the predictions of a synthetic model that we calculated with a new Monte Carlo 3D radiative code. The basic idea is that soft thermal photons (e.g. emitted by the star surface) can experience resonant cyclotron upscattering by a population of relativistic electrons treated in the twisted magnetosphere. Our code is specifically tailored to work in the ultra-magnetized regime; polarization and QED effects are consistently accounted for, as well different configurations for the magnetosphere. We discuss the predicted spectral properties in the 0.1–1000 keV range, the polarization properties, and we present the model application to a sample of magnetars soft X-ray spectra. 相似文献
57.
针对四旋翼无人机路径跟踪问题,设计了一种基于变量集结预测控制的控制器。首先以四旋翼无人机状态空间模型为基础建立预测模型;接着设计控制器时采用分段集结的策略把控制量集结成三段优化序列以减少优化计算量,并降低优化保守性,为了进一步加强系统稳定性,控制器引入终端代价函数和终端约束;最后用四旋翼无人机的动力学模型作为被控对象进行仿真验证,结果表明:该控制器能使四旋翼无人机在三轴方向均能实现一个良好的路径跟踪效果。与传统方法相比,这种基于变量集结的预测控制策略能够减小在线优化量,更适合四旋翼无人机飞控芯片的应用。 相似文献
58.
Anne Hutter Felix Spanier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We consider a relativistically moving blob consisting of an isotropic electron distribution that Compton-scatters photons from an external isotropic radiation field. We compute the resulting beaming pattern, i.e. the distribution of the scattered photons, in the blob frame as well as in the observer’s frame by using the full Klein–Nishina cross section and the exact incident photon distribution. In the Thomson regime the comparison of our approach with Dermer (1995) results in concurrent characteristics but different absolute number of the scattered photons by a factor of fcorr = 3.09. Additionally, our calculation yields a slightly lower boost factor which varies the more from the corresponding value in Dermer (1995) the higher the spectral index p of the electron distribution gets. 相似文献
59.
60.