全文获取类型
收费全文 | 8895篇 |
免费 | 9175篇 |
国内免费 | 1473篇 |
专业分类
航空 | 17002篇 |
航天技术 | 882篇 |
综合类 | 119篇 |
航天 | 1540篇 |
出版年
2024年 | 84篇 |
2023年 | 183篇 |
2022年 | 262篇 |
2021年 | 301篇 |
2020年 | 423篇 |
2019年 | 1130篇 |
2018年 | 1312篇 |
2017年 | 1230篇 |
2016年 | 1274篇 |
2015年 | 1190篇 |
2014年 | 1030篇 |
2013年 | 1029篇 |
2012年 | 968篇 |
2011年 | 889篇 |
2010年 | 899篇 |
2009年 | 926篇 |
2008年 | 809篇 |
2007年 | 658篇 |
2006年 | 507篇 |
2005年 | 331篇 |
2004年 | 323篇 |
2003年 | 277篇 |
2002年 | 319篇 |
2001年 | 267篇 |
2000年 | 239篇 |
1999年 | 275篇 |
1998年 | 232篇 |
1997年 | 208篇 |
1996年 | 158篇 |
1995年 | 135篇 |
1994年 | 139篇 |
1993年 | 193篇 |
1992年 | 137篇 |
1991年 | 314篇 |
1990年 | 263篇 |
1989年 | 294篇 |
1988年 | 208篇 |
1987年 | 83篇 |
1986年 | 33篇 |
1985年 | 1篇 |
1983年 | 5篇 |
1981年 | 3篇 |
1972年 | 1篇 |
1962年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
11.
A sulfur-based survival strategy for putative phototrophic life in the venusian atmosphere 总被引:1,自引:0,他引:1
Several observations indicate that the cloud deck of the venusian atmosphere may provide a plausible refuge for microbial life. Having originated in a hot proto-ocean or been brought in by meteorites from Earth (or Mars), early life on Venus could have adapted to a dry, acidic atmospheric niche as the warming planet lost its oceans. The greatest obstacle for the survival of any organism in this niche may be high doses of ultraviolet (UV) radiation. Here we make the argument that such an organism may utilize sulfur allotropes present in the venusian atmosphere, particularly S(8), as a UV sunscreen, as an energy-converting pigment, or as a means for converting UV light to lower frequencies that can be used for photosynthesis. Thus, life could exist today in the clouds of Venus. 相似文献
12.
13.
The primary objective of the Laser Interferometer Space Antenna (LISA) mission is to detect and observe gravitational waves from massive black holes and galactic binaries in the frequency range 10−4 to 10−1 Hz. This low-frequency range is inaccessible to ground-based interferometers because of the unshieldable background of local gravitational noise and because ground-based interferometers are limited in length to a few km. LISA is an ESA cornerstone mission and recently had a system study (Ref. 1) carried out by a consortium led by Astrium, which confirmed the basic configuration for the payload with only minor changes, and provided detailed concepts for the spacecraft and mission design. The study confirmed the need for a drag-free technology demonstration mission to develop the inertial sensors for LISA, before embarking on the build of the flight sensors. With a technology demonstration flight in 2005, it would be possible to carry out LISA as a joint ESA-NASA mission with a launch by 2010 subject to the funding programmatics. The baseline for LISA is three disc-like spacecraft each of which consist of a science module which carries the laser interferometer payload (two in each science module) and a propulsion module containing an ion drive and the hydrazine thrusters of the AOCS. The propulsion module is used for the transfer from earth escape trajectory provided by the Delta II launch to the operational orbit. Once there the propulsion module is jettisoned to reduce disturbances on the payload. Detailed analysis of thermal and gravitational disturbances, a model of the drag-free control and of the interferometer operation confirm that the strain sensitivity of the interferometer will be achieved. 相似文献
14.
15.
Deever DB Young RS Wang S Bradshaw BA Miles J Pettis CR Witten ML 《Acta Astronautica》2002,50(7):445-452
Head-down tilt models have been used as ground-based simulations of microgravity. Our previous animal research has demonstrated that there are significant changes in fluid distribution within 2 h after placement in a 45 degrees head-down tilt (45HDT) position and these changes in fluid distribution were still present after 14 days of 45HDT. Consequently, we investigated changes in fluid distribution during recovery from 16 days of 45HDT. Changes in radioactive tracer distribution and organ/body weight ratio were examined in rats randomly assigned to a 45HDT or prone control group. The 45HDT rats were suspended for 16 days and then allowed to recover at the prone position 0, 77, 101, or 125 h post-suspension. Animals were injected with technetium-labeled diethylenetriamine pentaacetate (99mTcDTPA, MW=492 amu, physical half-life of 6.02 h) and then killed 30 min post-injection. Lungs, heart, liver, spleen, kidneys, and brain were harvested, weighed, and measured for radioactive counts. Statistical analyses included two-way analysis of variance (ANOVA) that compared 45HDT versus controls at the four experimental time points. The organ weight divided by the body weight ratio for the brain, heart, kidneys and liver in the 45HDT rats was significantly different than the control rats, regardless of time (treatment). There was no difference between the different time points (time). The average 99mTcDTPA count divided by the organ weight ratio values for the heart, liver, and spleen were significantly higher in the 45HDT group than the control group. The average counts for the heart and spleen were significantly higher at 77, 101, and 125 h than at time zero. We conclude that the major organs have different recovery patterns after 45HDT for 16 days in the rat. 相似文献
16.
针对固体火箭发动机药柱存在裂纹的情况,对运动激波在狭缝中绕射传播的非定常流场进行了计算,得到了清晰的流场变化图谱,从流场图中可分辨出激波在狭缝中的传播过程。对不同深宽比的狭缝进行研究,发现流场结构存在明显差别,在深宽比较小时狭缝内压力波振荡较小,当深宽比超过一定值时狭缝内的压力波产生剧烈振荡。研究结果表明,该方法可很好地描述激波在狭缝中的传播过程。 相似文献
17.
Africano John Schildknecht Thomas Matney Mark Kervin Paul Stansbery Eugene Flury Walter 《Space Debris》2000,2(4):357-369
Since more than 10 years there is evidence that small-size space debris is accumulating in the geosynchronous orbit (GEO), probably as the result of breakups. Two break-ups have been reported in GEO. The 1978 break-up of an EKRAN 2 satellite, SSN 10365, was identified in 1992, and in 1992 a Titan 3C Transtage, SSN 3432, break-up produced at least twenty observable pieces. Subsequently several nations performed optical surveys of the GEO region in the form of independent observation campaigns. Such surveys suffer from the fact that the field of view of optical telescopes is small compared with the total area covered by the GEO ring. As a consequence only a small volume of the orbital element-magnitude-space is covered by each individual survey. Results from these surveys are thus affected by observational biases and therefore difficult to compare. This paper describes the development of a common search strategy to overcome these limitations. The strategy optimizes the sampling for objects in orbits similar to the orbits of the known GEO population but does not exclude the detection of objects with other orbital planes. A properly designed common search strategy clearly eases the comparison of results from different groups and the extrapolation from the sparse (biased) samples to the entire GEO environment. 相似文献
18.
基于RBF网络的惯导系统初始对准 总被引:18,自引:2,他引:18
建立了惯导系统(INS)初始对准的线性和非线性误差模型。分析了径向基函数(RBF)网络的结构和工作原理。研究了RBF网代替初始对准中的卡尔曼滤波器的实现方法。通过仿真表明,用神经网络进行初始对准,既可获得与卡尔曼滤波相同的对准精度,又提高了系统的实时性。 相似文献
19.
Major X-33 flight hardware has been delivered, and assembly of the vehicle is well underway in anticipation of its flight test program commencing in the summer of 1999. Attention has now turned to the operational VentureStarTM, the first single-stage-to-orbit (SSTO) reusable launch vehicle. Activities are grouped under two broad categories: (1) vehicle development and (2) market/business planning, each of which is discussed. The mission concept is presented for direct payload delivery to the International Space Station and to low Earth orbit, as well as payload delivery with an upper stage to Geosynchronous Transfer Orbit (GTO) and other high energy orbits. System requirements include flight segment and ground segment. Vehicle system sizing and design status is provided including the application of X-33 traceability and lessons learned. Technology applications to the VentureStarTM are described including the structure, propellant tanks, thermal protection system, aerodynamics, subsystems, payload bay and propulsion. Developing a market driven low cost launch services system for the 21st Century requires traditional and non-traditional ways of being able to forecast the evolution of the potential market. The challenge is balancing both the technical and financial assumptions of the market. This involves the need to provide a capability to meet market segments that in some cases are very speculative, while at the same time providing the financial community with a credible revenue stream. Furthermore, the market derived requirements need to be assessed so as not to impose unnecessary requirements on the vehicle design that add unreasonable cost to the development of the system, yet provides the right capabilities for new markets that could be triggered by dramatically lower space transportation prices. 相似文献
20.
介绍一种以大规模集成电路为核心组成的通用计数器的设计。该通用计数器具有输出标准信号、测量频率、测量周期、累加计数和自校等多种功能。 相似文献