全文获取类型
收费全文 | 24941篇 |
免费 | 1441篇 |
国内免费 | 1561篇 |
专业分类
航空 | 14616篇 |
航天技术 | 6953篇 |
综合类 | 1185篇 |
航天 | 5189篇 |
出版年
2022年 | 246篇 |
2021年 | 409篇 |
2020年 | 284篇 |
2019年 | 297篇 |
2018年 | 407篇 |
2017年 | 272篇 |
2016年 | 376篇 |
2015年 | 371篇 |
2014年 | 794篇 |
2013年 | 939篇 |
2012年 | 895篇 |
2011年 | 1080篇 |
2010年 | 840篇 |
2009年 | 1197篇 |
2008年 | 1178篇 |
2007年 | 746篇 |
2006年 | 762篇 |
2005年 | 692篇 |
2004年 | 712篇 |
2003年 | 817篇 |
2002年 | 801篇 |
2001年 | 919篇 |
2000年 | 611篇 |
1999年 | 729篇 |
1998年 | 658篇 |
1997年 | 513篇 |
1996年 | 554篇 |
1995年 | 599篇 |
1994年 | 590篇 |
1993年 | 511篇 |
1992年 | 470篇 |
1991年 | 477篇 |
1990年 | 423篇 |
1989年 | 586篇 |
1988年 | 269篇 |
1987年 | 290篇 |
1986年 | 257篇 |
1985年 | 642篇 |
1984年 | 522篇 |
1983年 | 415篇 |
1982年 | 490篇 |
1981年 | 612篇 |
1980年 | 247篇 |
1979年 | 193篇 |
1978年 | 189篇 |
1976年 | 155篇 |
1975年 | 189篇 |
1974年 | 180篇 |
1973年 | 161篇 |
1972年 | 189篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
1.
针对复杂动态环境下无人飞行器的动态障碍规避问题,基于合理假设建立了无人飞行器和动态障碍的运动学模型,并综合考虑无人飞行器飞行过程中的终端约束、控制输入约束、安全避障约束等,以能量最少为性能指标构建动态避障问题数学描述。之后,针对终端约束和控制输入约束,依据优化模型预测静态规划算法(OMPSP)生成初始轨迹;针对动态避障问题的不等式约束,引入松弛变量并结合滑模变结构控制方法设计松弛变量动力学,实现对一个、多个或同时多个动态障碍的安全规避;最后,依据有限时间微分动态规划(RHDDP)算法进行轨迹优化,获得满足上述各种约束并能规避动态障碍的近似最优轨迹。 相似文献
2.
Houman Hakima M. Reza Emami 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(7):2151-2171
This paper presents the mission design for a CubeSat-based active debris removal approach intended for transferring sizable debris objects from low-Earth orbit to a deorbit altitude of 100 km. The mission consists of a mothership spacecraft that carries and deploys several debris-removing nanosatellites, called Deorbiter CubeSats. Each Deorbiter is designed based on the utilization of an eight-unit CubeSat form factor and commercially-available components with significant flight heritage. The mothership spacecraft delivers Deorbiter CubeSats to the vicinity of a predetermined target debris, through performing a long-range rendezvous maneuver. Through a formation flying maneuver, the mothership then performs in-situ measurements of debris shape and orbital state. Upon release from the mothership, each Deorbiter CubeSat proceeds to performing a rendezvous and attachment maneuver with a debris object. Once attached to the debris, the CubeSat performs a detumbling maneuver, by which the residual angular momentum of the CubeSat-debris system is dumped using Deorbiter’s onboard reaction wheels. After stabilizing the attitude motion of the combined Deorbiter-debris system, the CubeSat proceeds to performing a deorbiting maneuver, i.e., reducing system’s altitude so much so that the bodies disintegrate and burn up due to atmospheric drag, typically at around 100 km above the Earth surface. The attitude and orbital maneuvers that are planned for the mission are described, both for the mothership and Deorbiter CubeSat. The performance of each spacecraft during their operations is investigated, using the actual performance specifications of the onboard components. The viability of the proposed debris removal approach is discussed in light of the results. 相似文献
3.
4.
5.
Arman Seuylemezian Manuela Buonanno Lisa Guan David J. Brenner David Welch 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):496-503
This work aims to investigate far-UVC light at 222 nm as a new microbial reduction tool for planetary protection purposes which could potentially be integrated into the spacecraft assembly process. The major advantage of far-UVC (222 nm) compared to traditional germicidal UVC (254 nm) is the potential for application throughout the spacecraft assembly process in the presence of humans without adverse health effects due to the limited penetration of far-UVC light into biological materials. Testing the efficacy of 222-nm light at inactivating hardy bacterial cells and spores isolated from spacecraft and associated surfaces is a necessary step to evaluate this technology. We assessed survival of Bacillus pumilus SAFR-032 and Acinetobacter radioresistens 50v1 exposed to 222-nm light on proxy spacecraft surfaces simulated by drying the bacteria on aluminum coupons. The survival fraction of both bacteria followed a single stage decay function up to 60 mJ/cm2, revealing similar susceptibility of both species to 222-nm light, which was independent of the exposure rate. Irradiation with far-UVC light at 222 nm is an effective method to decontaminate the proxy spacecraft materials tested in this study. 相似文献
6.
随着软件的应用规模越来越大,软件系统一旦出现故障,很可能会造成人员伤亡或财产等重大损失,因此对软件可信性进行评估尤为重要.在安全攸关如航空航天等领域,作为可信关键属性之一的安全性影响着整个软件系统的可信评估.特别当一个组件受到安全攻击或缺陷出现时,可信性会下降,会影响到与它可信关联的组件可信性,从而影响到整个系统的可信性.遵循这一思路,设计了软件系统组件可信性发生改变后对其它组件可信性影响度量公式,进一步给出当一组件可信性发生变化,整个软件系统各组件可信性度量发生变化的度量模型.本文以某“航天电源管理设备”为例,证明了本文所建立的组件可信依赖关系度量模型的合理性和有效性. 相似文献
7.
Ethan. R. Burnett Hanspeter Schaub 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(11):3381-3395
This paper explores methods for approximating and analyzing the dynamics of highly perturbed spacecraft formations with an emphasis on computationally efficient approaches. This facilitates on-board computation or rapid preliminary mission design analysis. Perturbed formation dynamics are often approximated as linear time-varying (LTV) systems, for which Floquet theory can be used to analyze the degree of system instability. Furthermore, the angular momentum of the relative orbital state can be computed with the approximate dynamics to provide additional insight. A general methodology is developed first and then applied to the problem of unstable formation dynamics in asteroid orbits. Here the dominant perturbative effects due to low-order gravitational harmonics and solar radiation pressure are modeled. Numerical simulations validate the approach and illustrate the approximation accuracy achieved. 相似文献
8.
Yi Wei Qingjun Li Fangnuan Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):393-400
A new orbit-attitude-vibration coupled dynamic model of the tethered solar power satellite (Tethered SPS) is established based on absolute nodal coordinate formulation. The Hamilton’s equation of the system is derived by introducing generalized momentum through Legendre transformation. The correctness of the proposed model is verified by an example. The dynamic characteristics of the Tethered SPS are studied using the symplectic Runge-Kutta method. Simulation results show that the orbital radius and the total energy of the system are well preserved. The attitude of the system is unstable when the mass of the bus system is small. However, the attitude stability is dependent on some other parameters of the system, which requires further studies. It is also found that the average tether force/deformation can be roughly estimated by simplifying the solar panel as a particle. The proposed model can be used to study the orbit-attitude-vibration coupled dynamics and control problems. 相似文献
9.
Kugusheva A. D. Kalegaev V. V. Vlasova N. A. Petrov K. A. Bazilevskaya G. A. Makhmutov V. S. 《Cosmic Research》2021,59(6):446-455
Cosmic Research - The results of an analysis of the space–time characteristics and dynamics of precipitations of magnetospheric electrons with energies in the range from 0.1 to 0.7 MeV are... 相似文献
10.
Michael A. Earl Philip W. Somers Konstantin Kabin Donald Bédard Gregg A. Wade 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(8):2135-2146
For the first time, the spin axis orientation of an inactive box-wing geosynchronous satellite has been estimated from ground-based optical photometric observations of Echostar-2’s specular reflections. Recent photometric light curves obtained of Echostar-2 over four years suggest that unusually bright and brief specular reflections were occurring twice within an observed spin period. These bright and brief specular reflections suggested two satellite surfaces with surface normals separated by approximately 180°. The geometry between the satellite, the Sun, and the observing location at the time of each of the brightest observed reflections, was used to estimate Echostar-2’s equatorial spin axis orientation coordinates. When considering prograde and retrograde rotation, Echostar-2’s spin axis orientation was estimated to have been located within 30° of either equatorial coordinate pole. Echostar-2’s spin axis was observed to have moved approximately 180° in right ascension, within a time span of six months, suggesting a roughly one year spin axis precession period about the satellite’s angular momentum vector. 相似文献