全文获取类型
收费全文 | 82677篇 |
免费 | 15703篇 |
国内免费 | 11300篇 |
专业分类
航空 | 60948篇 |
航天技术 | 18409篇 |
综合类 | 7844篇 |
航天 | 22479篇 |
出版年
2024年 | 320篇 |
2023年 | 1121篇 |
2022年 | 3038篇 |
2021年 | 3586篇 |
2020年 | 3406篇 |
2019年 | 2954篇 |
2018年 | 3264篇 |
2017年 | 3687篇 |
2016年 | 2689篇 |
2015年 | 3451篇 |
2014年 | 4501篇 |
2013年 | 4731篇 |
2012年 | 5388篇 |
2011年 | 6100篇 |
2010年 | 6073篇 |
2009年 | 6360篇 |
2008年 | 6136篇 |
2007年 | 5489篇 |
2006年 | 5057篇 |
2005年 | 4096篇 |
2004年 | 2977篇 |
2003年 | 2432篇 |
2002年 | 2154篇 |
2001年 | 2336篇 |
2000年 | 2008篇 |
1999年 | 2030篇 |
1998年 | 1524篇 |
1997年 | 1120篇 |
1996年 | 1174篇 |
1995年 | 1260篇 |
1994年 | 1299篇 |
1993年 | 681篇 |
1992年 | 677篇 |
1991年 | 401篇 |
1990年 | 360篇 |
1989年 | 496篇 |
1988年 | 291篇 |
1987年 | 387篇 |
1986年 | 274篇 |
1985年 | 511篇 |
1984年 | 425篇 |
1983年 | 338篇 |
1982年 | 341篇 |
1981年 | 481篇 |
1980年 | 203篇 |
1979年 | 163篇 |
1978年 | 175篇 |
1975年 | 162篇 |
1974年 | 162篇 |
1972年 | 156篇 |
排序方式: 共有10000条查询结果,搜索用时 359 毫秒
111.
Satoko Uchida Mitsuyo Masukawa Shigeki Kamigaichi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2002,30(4):797-802
National Space Development Agency of Japan (NASDA) has developed aquatic animal experiment facilities for NASA Space Shuttle use. Vestibular Function Experiment Unit (VFEU) was firstly designed and developed for physiological research using carp in Spacelab-J (SL-J, STS-47) mission. It was modified as Aquatic Animal Experiment Unit (AAEU) to accommodate small aquatic animals, such as medaka and newt, for second International Microgravity Laboratory (IML-2, STS-65) mission. Then, VFEU was improved to accommodate marine fish and to perform neurobiological experiment for Neurolab (STS-90) and STS-95 missions. We have also developed and used water purification system which was adapted to each facility. Based on these experiences of Space Shuttle missions, we are studying to develop advanced aquatic animal experiment facility for both Space Shuttle and International Space Station (ISS). 相似文献
112.
L O Bjorn S Widell T Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2002,30(6):1557-1562
Plants have evolved under the influence of UV-B radiation and have acquired systems for monitoring it and investing appropriate resources for protection against it, i.e., filters, quenchers of radicals and reactive oxygen species, and repair systems. An hypothesis for how plants monitor radiation has been presented. 相似文献
113.
This study introduces a field oriented controlled (FOC) induction machine based flywheel energy storage (FES) system fed from a 20 kHz high frequency (HF) ac link and pulse density modulated (PDM) Converter. The feasibility of FES system is investigated both in software and hardware and is demonstrated successfully in both cases. The investigated system offers a good potential as a temporary energy storage system for various applications from automobile industry to aerospace applications. 相似文献
114.
115.
116.
A review of common switching techniques for dc/dc power conversion is presented. The evolution of the forward converter is discussed, leading naturally to the introduction of the double forward converter. Technical details for a series of radiation-hardened converters are then provided. This series was designed for space power management and distribution (PMAD) applications. The successful development of the PMAD converter demonstrated the viability of high voltage bus. 相似文献
117.
杠杆式力标准机自动控制系统 总被引:4,自引:1,他引:3
介绍单片机用于杠杆式力标准机控制、实现检定过程自动化的设计方法,重点介绍硬件结构和软件编制。 相似文献
118.
In a previous paper (Tappin et al., 1999) we used cross-correlation analysis of high-cadence observations with the LASCO coronagraphs to trace the acceleration
of the solar wind at low latitudes. In this paper we present a similar analysis carried out over the North pole of the Sun.
The observations which were made in March 2000 with the C3 coronagraph show low bulk flow speeds (comparable to or lower than
those seen at the equator in early 1998). We observe the acceleration continuing to the edge of the C3 field of view at about
30 R
⊙. We also observe, as at low latitude, a high-speed tail but now reaching out well beyond 2000 km s−1. We do not see a clear signature of a fast polar bulk flow. We therefore conclude that at this phase of the solar cycle,
any fast bulk flow occupies only a small part of the line of sight and is therefore overwhelmed by the denser slow solar wind
in these observations. We also show that the fast component is consistent with observed solar wind speeds at 1 AU.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
119.
晶体管h参数微变等效电路是电子技术中求解低频、小信号放大电路常用的分析方法.本文通过具体分析,将模拟放大电路进行了新的分类,并且明确而系统地给出运用微变等效电路求解各类模拟放大电路动态指标Av、ri和γ0公式、解题难点及规律. 相似文献
120.
Magnetic turbulence at the magnetopause, a key problem for understanding the solar wind/ magnetosphere exchanges 总被引:1,自引:0,他引:1
According to ideal MHD, the magnetopause boundary should split the terrestrial environment in two disconnected domains: outside, the solar wind (including its shocked part, the magnetosheath), and inside, the magnetosphere. This view is at variance with the experimental data, which show that the magnetopause is not tight and that a net transfer of matter exists from the solar wind to the magnetosphere; it implies that the frozen-in condition must break down on the magnetopause, either over the whole boundary or at some points. In the absence of ordinary collisions, only short scale phenomena (temporal and/or spatial) can be invoked to explain this breakdown, and the best candidates in this respect appear to be the ULF magnetic fluctuations which show very strong amplitudes in the vicinity of the magnetopause boundary. It has been shown that these fluctuations are likely to originate in the magnetosheath, probably downstream of the quasi-parallel shock region, and that they can get amplified by a propagation effect when crossing the magnetopause. When studying the propagation across the magnetopause boundary, several effects are to be taken into account simultaneously to get reliable results: the magnetopause density gradient, the temperature effects, and the magnetic field rotation can be introduced while remaining in the framework of ideal MHD. In these conditions, the magnetopause amplification has been interpreted in term of Alfvén and slow resonances occurring in the layer. When, in addition, one takes the ion inertia effects into account, by the way of the Hall-MHD equations, the result appears drastically different: no resonance occurs, but a strong Alfvén wave can be trapped in the boundary between the point where it is converted from the incident wave and the point where it stops propagating back, i.e., the point where k
\|=0, which can exist thanks to the magnetic field rotation. This effect can bring about a new interpretation to the magnetopause transfers, since the Hall effect can allow reconnection near this particular point. The plasma transfer through the magnetopause could then be interpreted in terms of a reconnection mechanism directly driven by the magnetosheath turbulence, which is permanent, rather than due to any local instability of the boundary, for instance of the tearing type, which should be subject to an instability threshold and thus, as far as it exists, more sporadic. 相似文献