全文获取类型
收费全文 | 1573篇 |
免费 | 304篇 |
国内免费 | 235篇 |
专业分类
航空 | 1121篇 |
航天技术 | 382篇 |
综合类 | 198篇 |
航天 | 411篇 |
出版年
2024年 | 5篇 |
2023年 | 20篇 |
2022年 | 54篇 |
2021年 | 56篇 |
2020年 | 61篇 |
2019年 | 47篇 |
2018年 | 46篇 |
2017年 | 45篇 |
2016年 | 52篇 |
2015年 | 73篇 |
2014年 | 91篇 |
2013年 | 84篇 |
2012年 | 100篇 |
2011年 | 119篇 |
2010年 | 104篇 |
2009年 | 99篇 |
2008年 | 85篇 |
2007年 | 87篇 |
2006年 | 82篇 |
2005年 | 91篇 |
2004年 | 55篇 |
2003年 | 43篇 |
2002年 | 46篇 |
2001年 | 49篇 |
2000年 | 38篇 |
1999年 | 59篇 |
1998年 | 48篇 |
1997年 | 30篇 |
1996年 | 40篇 |
1995年 | 38篇 |
1994年 | 39篇 |
1993年 | 44篇 |
1992年 | 38篇 |
1991年 | 42篇 |
1990年 | 18篇 |
1989年 | 28篇 |
1988年 | 22篇 |
1987年 | 7篇 |
1986年 | 8篇 |
1985年 | 2篇 |
1984年 | 2篇 |
1983年 | 4篇 |
1982年 | 3篇 |
1981年 | 4篇 |
1980年 | 1篇 |
1978年 | 1篇 |
1975年 | 1篇 |
1974年 | 1篇 |
排序方式: 共有2112条查询结果,搜索用时 31 毫秒
281.
提高长线传输数字波形质量的技术措施 总被引:2,自引:0,他引:2
从两方面论述数字编码波形在长线上传输的影响因素及其改善措施。通过分析并经实验表明,长线的分布电容影响通常居诸因素之首位。改进长线驱动电路,在一定程度上,可改善其传输波形之质量。另外,可利用长线传输波形的同时,还传输供总线接口电路需要的电源能量,满足总线浮空隔离的要求,有效地抑制了共模干扰。此项技术适用于远距多路串行总线的数据采集系统。 相似文献
282.
CAD技术及其在卫星工程中的应用 总被引:1,自引:0,他引:1
CAD 技术作为一种高效率、高质量、高精度的设计技术,正在包括航天技术在内的多个领域中广泛应用,发挥其效益。尤其是在机械(MCAD)与电子(ECAD)两方面的应用,更是令人瞩目。本文就CAD 技术的范畸、功能、组成、主要技术等并结合卫星研制的具体应用前景,作一介绍,目的在于推动CAD技术的开展,并为CAD/CAM 一体化做好思想准备。 相似文献
283.
284.
Recently, unmanned aerial vehicles (UAVs) acting as relay platforms have attracted considerable attention due to the advantages of extending coverage and improving connectivity for long-range communications. Specifically, in the scenario where the access point (AP) is mobile, a UAV needs to find an efficient path to guarantee the connectivity of the relay link. Motivated by this fact, this paper proposes an optimal design for beamforming (BF) and UAV path planning. First of all, we study a dual-hop amplify-and-forward (AF) wireless relay network, in which a UAV is used as relay between a mobile AP and a fixed base station (BS). In the network, both of the AP and the BS are equipped with multiple antennas, whereas the UAV has a single antenna. Then, we obtain the output signal~to-noise ratio (SNR) of the dual-hop relay network. Based on the criterion of maximizing the output SNR, we develop an optimal design to obtain the solution of the optimal BF weight vector and the UAV heading angle. Next, we derive the closed-form outage probability (OP) expression to investigate the performance of the dual-hop relay network conveniently. Finally, computer simulations show that the proposed approach can obtain nearly optimal flying path and OP performance, indicating the effectiveness of the proposed algorithm. Furthermore, we find that increasing the antenna number at the BS or the maximal heading angle can significantly improve the performance of the considered relay network. 相似文献
285.
为了揭示跨声速大膨胀比涡轮损失的主要特点和两种不同尾缘冷却方式对损失的影响,以典型大膨胀比跨声速涡轮和跨声速叶栅为研究对象开展了数值研究。研究发现大膨胀比跨声速涡轮的主要损失是叶型损失,占到总损失的65%左右,尾缘激波损失是叶型损失的主要来源。尾缘全劈缝冷气入射通过提高尾缘基压区基压来减少尾缘膨胀波对气流的加速程度,从而降低最高马赫数和激波损失,尾缘压力面劈缝冷气入射通过改变叶片尾缘压力面激波波系结构,使原来的一道激波变成两道或者两道以上的弱激波,从而减少激波损失。两种尾缘冷气方式都有利于降低大膨胀比跨声速涡轮激波损失,但压力面劈缝冷气入射方式效果更为明显。 相似文献
286.
J. B. Blake B. H. Mauk D. N. Baker P. Carranza J. H. Clemmons J. Craft W. R. Crain A. Crew Y. Dotan J. F. Fennell R. H. Friedel L. M. Friesen F. Fuentes R. Galvan C. Ibscher A. Jaynes N. Katz M. Lalic A. Y. Lin D. M. Mabry T. Nguyen C. Pancratz M. Redding G. D. Reeves S. Smith H. E. Spence J. Westlake 《Space Science Reviews》2016,199(1-4):309-329
287.
介绍了一种非接触式激光检测系统,可用于检测液晶曝光中液晶模板与基板之间的间隙,给出了该种系统的测量原理、硬件系统、信号处理方法、测量结果、分辨力和误差分析,并指出了这种测量系统的应用。 相似文献
288.
采用积木式方法构建试验金字塔是目前已经被广泛接受的用来完成大型飞机结构强度验证的基本手段。本文概述了积木式方法和试验金字塔的发展历程和趋势,介绍了不同型号的美军机在研制过程中所建立的强度验证试验金字塔的统计结果,并且从试验层级、对象、目的和类型等四个方面比较了试验内容的数量与经费占比,由此来说明基础层级试验验证工作在强度验证试验金字塔中重要性和经济性。通过对虚拟试验在强度验证工作中的发展趋势、应用和限制的介绍,为顺利完成相关的全尺寸部件和整机的强度验证提供可靠的保障手段。 相似文献
289.
Yong Lin 《Space Science Reviews》2011,158(2-4):237-266
Thanks to gradually improving observational capabilities, both from space and ground-based observatories, it is now generally accepted that thin threads (width ??200 km) constitute the building blocks of solar filaments and prominences. At ultra-small scales, high quality image sequences show a non-static picture of filaments and reveal that their oscillatory behavior is an important dynamic feature of these structures. Filament seismology sheds light on the internal magnetic structures of filaments and their interactions with surrounding solar regions. Understanding the overall magnetic topology of solar filaments and prominences including their small-scale thread-like structures is essential in interpretation and understanding of their oscillations. For this reason we aim here to present an update of the dynamic and spatial structures of prominences and filaments as inferred from high resolution observations in the past decennia. Some constraints in high resolution observations are addressed. Our review focuses mainly on the observational aspects and aims to summarize recent oscillation studies of individual filament threads and groups of threads. Finally, some theoretical interpretations of oscillations of filament threads and the inferred physical conditions of filament plasma are also discussed. 相似文献
290.
R. P. Lin 《Space Science Reviews》2011,159(1-4):421-445
RHESSI measurements relevant to the fundamental processes of energy release and particle acceleration in flares are summarized. RHESSI??s precise measurements of hard X-ray continuum spectra enable model-independent deconvolution to obtain the parent electron spectrum. Taking into account the effects of albedo, these show that the low energy cut-off to the electron power-law spectrum is typically ?tens of keV, confirming that the accelerated electrons contain a large fraction of the energy released in flares. RHESSI has detected a high coronal hard X-ray source that is filled with accelerated electrons whose energy density is comparable to the magnetic-field energy density. This suggests an efficient conversion of energy, previously stored in the magnetic field, into the bulk acceleration of electrons. A new, collisionless (Hall) magnetic reconnection process has been identified through theory and simulations, and directly observed in space and in the laboratory; it should occur in the solar corona as well, with a reconnection rate fast enough for the energy release in flares. The reconnection process could result in the formation of multiple elongated magnetic islands, that then collapse to bulk-accelerate the electrons, rapidly enough to produce the observed hard X-ray emissions. RHESSI??s pioneering ??-ray line imaging of energetic ions, revealing footpoints straddling a flare loop arcade, has provided strong evidence that ion acceleration is also related to magnetic reconnection. Flare particle acceleration is shown to have a close relationship to impulsive Solar Energetic Particle (SEP) events observed in the interplanetary medium, and also to both fast coronal mass ejections and gradual SEP events. New instrumentation to provide the high sensitivity and wide dynamic range hard X-ray and ??-ray measurements, plus energetic neutral atom (ENA) imaging of SEPs above ??2 R??, will enable the next great leap forward in understanding particle acceleration and energy release is large solar eruptions??solar flares and associated fast coronal mass ejections (CMEs). 相似文献