全文获取类型
收费全文 | 6117篇 |
免费 | 651篇 |
国内免费 | 486篇 |
专业分类
航空 | 3365篇 |
航天技术 | 1901篇 |
综合类 | 440篇 |
航天 | 1548篇 |
出版年
2023年 | 47篇 |
2022年 | 107篇 |
2021年 | 167篇 |
2020年 | 130篇 |
2019年 | 133篇 |
2018年 | 239篇 |
2017年 | 185篇 |
2016年 | 161篇 |
2015年 | 168篇 |
2014年 | 243篇 |
2013年 | 254篇 |
2012年 | 267篇 |
2011年 | 322篇 |
2010年 | 335篇 |
2009年 | 380篇 |
2008年 | 386篇 |
2007年 | 274篇 |
2006年 | 220篇 |
2005年 | 216篇 |
2004年 | 164篇 |
2003年 | 203篇 |
2002年 | 217篇 |
2001年 | 194篇 |
2000年 | 159篇 |
1999年 | 159篇 |
1998年 | 145篇 |
1997年 | 129篇 |
1996年 | 123篇 |
1995年 | 156篇 |
1994年 | 138篇 |
1993年 | 90篇 |
1992年 | 116篇 |
1991年 | 69篇 |
1990年 | 56篇 |
1989年 | 85篇 |
1988年 | 42篇 |
1987年 | 38篇 |
1986年 | 38篇 |
1985年 | 111篇 |
1984年 | 79篇 |
1983年 | 68篇 |
1982年 | 83篇 |
1981年 | 103篇 |
1980年 | 31篇 |
1979年 | 41篇 |
1978年 | 28篇 |
1977年 | 18篇 |
1974年 | 17篇 |
1973年 | 16篇 |
1972年 | 15篇 |
排序方式: 共有7254条查询结果,搜索用时 894 毫秒
111.
112.
113.
航天器振动试验中的动力吸振现象 总被引:1,自引:0,他引:1
振动环境试验是考验航天器中各分机力学品质的重要试验,分机适应力学环境的能力在设计阶段必须充分考虑。目前分机的力学环境条件往往是在考虑了一定的安全系数后,以分机安装处界面的加速度包络曲线给出的。然而一般来说,分机振动试验过程中的边界条件与分机实际工作状态的边界条件是不同的。具体地说就是在振动试验过程中分机通过试验转接托架与振动台面相连,实际工作状态是分机安装在安装件(卫星各舱板)上。由于试验转接托架与安装件的动力学特性不一样,根据多自由度弹簧质量阻尼系统的动力吸振原理,可以推出试验状态分机在固有频率处存在过试验现象。为了减少过试验对分机带来的危害,新的试验方法研究(加速度响应限幅控制、阻抗特性模拟法、限力技术等)已成为国内外航天工作者研究的热点。文章详细阐述了振动试验中动力吸振的机理及过试验产生的缘由。 相似文献
114.
Smirnova N. V. Lyakhov A. N. Setzer Yu. I. Osepian A. P. Meng C.-I. Smith R. Stenbaek-Nielsen H. C. 《Cosmic Research》2004,42(3):210-218
Spatial distributions of the electron density in the latitude range 60°–90° N were calculated on the basis of a physical model of the E and lower Fregions of the high-latitude ionosphere using statistical models of auroral proton and electron precipitation. It is shown that precipitating protons can play the key role in the ionization of the Eregion in the dusk and midnight sectors of the auroral oval. However, quantitative estimates of the contribution of protons to the ionization depend on the used statistical models of electron precipitation. Comparison of the electron density profiles calculated for two incoherent scatter radars, EISCAT (Tromsö) and ESR (Svalbard), for simultaneous precipitation of electrons and protons and for electron precipitation only show that the influence of protons is the most significant in the dusk sector over the EISCAT radar and in the midnight sector over the ESR radar. The results presented indicate the need to take protons into account when radar data are used to derive precipitating electron spectra. 相似文献
115.
根据固体火箭发动机内弹道计算模型,分析了使用大扩张比喷管地面静止试验性能与真空性能之间的联系,建立了由地面性能换算成真空性能的方法,计算出的真空推力、真空比冲等数据与实际相符。 相似文献
116.
K R Sridhar J E Finn M H Kliss 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2000,25(2):249-255
The atmosphere of Mars has many of the ingredients that can be used to support human exploration missions. It can be "mined" and processed to produce oxygen, buffer gas, and water, resulting in significant savings on mission costs. The use of local materials, called ISRU (for in-situ resource utilization), is clearly an essential strategy for a long-term human presence on Mars from the standpoints of self-sufficiency, safety, and cost. Currently a substantial effort is underway by NASA to develop technologies and designs of chemical plants to make propellants from the Martian atmosphere. Consumables for life support, such as oxygen and water, will probably benefit greatly from this ISRU technology development for propellant production. However, the buffer gas needed to dilute oxygen for breathing is not a product of a propellant production plant. The buffer gas needs on each human Mars mission will probably be in the order of metric tons, primarily due to losses during airlock activity. Buffer gas can be separated, compressed, and purified from the Mars atmosphere. This paper discusses the buffer gas needs for a human mission to Mars and consider architectures for the generation of buffer gas including an option that integrates it to the propellant production plant. 相似文献
117.
Chao-Song Huang J.C. Foster K. Yumoto J.L. Chau O. Veliz 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2407-2412
It is well known that the solar wind can significantly affect high-latitude ionospheric dynamics. However, the effects of the solar wind on the middle- and low-latitude ionosphere are much less studied. In this paper, we report observations that large perturbations in the middle- and low-latitude ionosphere are well correlated with solar wind variations. In one event, a significant (20–30%) decrease of the midlatitude ionospheric electron density over a large latitudinal range was related to a sudden drop in the solar wind pressure and a northward turning of the interplanetary magnetic field, and the density decrease became larger at lower latitudes. In another event, periodic perturbations in the dayside equatorial ionospheric E × B drift and electrojet were closely associated with variations in the interplanetary electric field. Since the solar wind is always changing with time, it can be a very important and common source of ionospheric perturbations at middle- and low-latitudes. The relationship between solar wind variations and significant ionospheric perturbations has important applications in space weather. 相似文献
118.
K O'Brien H H Sauer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,32(1):73-80
High-energy solar particles, produced in association with solar flares and coronal mass ejections, occasionally bombard the earth's atmosphere. resulting in radiation intensities additional to the background cosmic radiation. Access of these particles to the earth's vicinity during times of geomagnetic disturbances are not adequately described by using static geomagnetic field models. These solar fluxes are also often distributed non uniformly in space, so that fluxes measured by satellites obtained at great distances from the earth and which sample large volumes of space around the earth cannot be used to predict fluxes locally at the earth's surface. We present here a method which uses the ground-level neutron monitor counting rates as adjoint sources of the flux in the atmosphere immediately above them to obtain solar-particle effective dose rates as a function of position over the earth's surface. We have applied this approach to the large September 29-30, 1989 ground-level event (designated GLE 42) to obtain the magnitude and distribution of the solar-particle effective dose rate from an atypically large event. The results of these calculations clearly show the effect of the softer particle spectra associated with solar particle events, as compared with galactic cosmic rays, results in a greater sensitivity to the geomagnetic field, and, unlike cosmic rays, the near-absence of a "knee" near 60 degrees geomagnetic latitude. 相似文献
119.
董雷 《中国空间科学技术》1996,16(3):58-62
叙述了资源卫星动量轮的一般结构和开环测试原理。详细介绍了应用IEEE488总线构成的动量轮开环性能自动测试系统。说明了这个自动测试系统的系统构成以及测试项目、测试流程和获得的测试结果。并据此提出这个系统在卫星研制工作中具有推广价值。 相似文献
120.
K. Tsuruda I. Nakatani T. Yamamoto 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1996,17(12):21-29
PLANET-B is the Japanese Mars orbiter program. The primary objective of the program is to study the Martian aeronomy, putting emphasis on the interaction of the Martian upper atmosphere with the solar wind. The launch of the spacecraft is scheduled for August, 1998. The periapsis altitude and the apoapsis are 150 km and 15 Mars radii, respectively. The dry weight of the orbiter is 186 kg including 14 science instruments. Advanced technologies are employed in the design of the spacecraft in order to overcome the weight limitation. This paper describes the scientific objectives of the PLANET-B program and outline of the spacecraft system. 相似文献