全文获取类型
收费全文 | 327篇 |
免费 | 34篇 |
国内免费 | 37篇 |
专业分类
航空 | 206篇 |
航天技术 | 75篇 |
综合类 | 30篇 |
航天 | 87篇 |
出版年
2022年 | 3篇 |
2021年 | 13篇 |
2020年 | 7篇 |
2019年 | 6篇 |
2018年 | 6篇 |
2017年 | 9篇 |
2016年 | 8篇 |
2015年 | 9篇 |
2014年 | 19篇 |
2013年 | 14篇 |
2012年 | 6篇 |
2011年 | 22篇 |
2010年 | 5篇 |
2009年 | 13篇 |
2008年 | 9篇 |
2007年 | 6篇 |
2006年 | 7篇 |
2005年 | 19篇 |
2004年 | 15篇 |
2003年 | 34篇 |
2002年 | 41篇 |
2001年 | 12篇 |
2000年 | 7篇 |
1999年 | 9篇 |
1997年 | 4篇 |
1996年 | 10篇 |
1995年 | 9篇 |
1994年 | 7篇 |
1993年 | 10篇 |
1991年 | 2篇 |
1989年 | 6篇 |
1986年 | 3篇 |
1985年 | 3篇 |
1984年 | 3篇 |
1981年 | 3篇 |
1980年 | 3篇 |
1978年 | 3篇 |
1976年 | 1篇 |
1975年 | 4篇 |
1974年 | 1篇 |
1973年 | 1篇 |
1972年 | 6篇 |
1971年 | 1篇 |
1970年 | 3篇 |
1969年 | 1篇 |
1968年 | 1篇 |
1967年 | 4篇 |
1966年 | 2篇 |
1963年 | 2篇 |
1962年 | 1篇 |
排序方式: 共有398条查询结果,搜索用时 17 毫秒
51.
热流限制下的最优气动力辅助变轨 总被引:4,自引:0,他引:4
以变轨能量消耗最小为优化目标,应用极大值原理研究了飞行过程受热流限制和升力系统约束下的气动力辅助共面变轨问题,飞行过程成分第一自由弧段,约束弧段,第二自由弧段三个部分,讨论了升力系数的最优表达式,分析了飞行过程中两种约束的相互作用,给出了约束弧起始位置的角点条件和终端的横截条件下,对不同的初值选取方法讨论了三种计算策略,并给出了数值算例。 相似文献
52.
针对机会阵雷达方向图综合的不确定问题,提出了一种基于模糊机会约束规划的方向图综合规划模型。该模型基于可信性理论,综合考虑天线单元分布的随机性以及激励状态的不确定性,将参与方向图综合时激励打开的天线数目看做一个梯形模糊变量,用以描述综合时的复杂不确定环境。随后,将规划模型转化为清晰等价形式,再结合遗传算法和灰关联综合评价法则设计了一种混合智能优化算法,用于求解该模型。以一维任意非均匀线阵为例,对主瓣宽度和最大副瓣电平进行了优化。仿真表明:优化后结果的可信性高于置信水平,验证了该算法的有效性。 相似文献
53.
Carle M. Pieters Lucy A. McFadden Thomas Prettyman M. Cristina De Sanctis Thomas B. McCord Takahiro Hiroi Rachel Klima Jian-Yang Li Ralf Jaumann 《Space Science Reviews》2011,163(1-4):117-139
The instruments on the Dawn spacecraft are exceptionally well suited to characterize and map the surface composition of Vesta in an integrated manner. These include a framing camera with multispectral capabilities, a high spectral resolution near-infrared imaging spectrometer, and a gamma-ray and neutron spectrometer. Three examples of issues addressed at Vesta are: (1) What is the composition of Vesta??s interior and differentiation state as exposed by the Great South Crater? (2) How has space weathering affected Vesta, both globally and at a local scale? and (3) Are volatiles or hydrated material present on Vesta??s surface? We predict that Dawn finds many surprises, such as an olivine-bearing mantle exposed near the south-pole, a weakly or un-weathered surface that has been relatively recently resurfaced, and a very thin layer of surficial volatiles derived from interaction with the solar wind. 相似文献
54.
M Casolino V Bidoli E De Grandis M P De Pascale G Furano A Morselli L Narici P Picozza E Reali R Sparvoli A Galper M Korotkov Y Ozerov A Popov G Mazzenga M Ricci G Castellini S Avdeev M Boezio W Bonvicini A Vacchi N Zampa P Spillantini P Carlson C Fuglesang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,31(1):135-140
In this work we present preliminary results of nuclear composition measurements on board space station MIR obtained with SILEYE-2 particle telescope. SILEYE-2 was placed on MIR in 1997 and has been working since then. It consists of an array of 6 active silicon strip detectors which allow nuclear and energetic identification of cosmic rays in the energy range between approximately 30 and 200 MeV/n. The device is attached to an helmet and connected to an eye mask which shields the cosmonaut eyes from light and allow studies of the Light Flashes (LF) phenomenon. In addition to the study of the causes of LF, the device is used to perform real time long term radiation environment monitoring inside the MIR, performing measurements in solar quiet and active days. 相似文献
55.
Massimo Materassi Lucilla Alfonsi Giorgiana De Franceschi Vincenzo Romano Cathryn Mitchell Paolo Spalla 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The study of amplitude scintillation on GPS radio links is usually done after detrending the time series of the transmitted power so to define scintillations as the chaotic fluctuation around a unitary value. In a sense, the choice of how to detrend the time series is part of the definition of scintillation. 相似文献
56.
Giuseppe Consolini Paola De Michelis Matthieu Kretzschmar 《Space Science Reviews》2006,122(1-4):293-299
Recent studies evidenced that the magnetotail dynamics looks like the one of an avalanching system. This fact has been related
with a near criticality dynamics and modelled by singular diffusion and transport equations. Here, we discuss some features
of the Earth’s magnetotail dynamics using a thermodynamic approach. In detail we discuss the role played by fluctuations in
singular diffusion and relaxation processes from a non-equilibrium thermodynamics point of view. Moreover, the emergence of
non-Gaussian statistics is discussed in the framework of the thermodynamics of composite systems. 相似文献
57.
H. Van De Stadt 《Space Science Reviews》1975,17(5):673-676
58.
59.
In part I (De Greve and Packet) we have investigated the occurrence of reversed phases of mass-transfer during Case A evolution in close binaries. If the initial period of a system is shorter than 1–2 days (Early Case A) the reversed phase starts before core hydrogen exhaustion of the gainer (part I). This type of evolution is characterized by at least two phases of slow mass-transfer.We have computed the evolution of four Early Case A systems with initial masses of the loser equal to 3 Mo and 5 Mo. These four systems start mass-exchange when Xc of the primary has decreased to 0.525 (75% of its initial value). They all experience two phases of slow mass-transfer.We find that both phases have about the same duration for all systems. The mass ratios are clearly distinct, being closer to unity during the first phase. In the Hertzsprung-Russell, mass-radius and mass-luminosity diagrams both components remain close to the main-sequence band during slow mass-transfer. Evolution as an Algol is ended when both components overflow their outer critical surface after a second reversal of the mass-transfer.Observed Algol systems evolving in Early Case A are scarce. A search thruogh the catalogue by Giuricin et al. gives us the following candidates: X Tri, SX Aur and V Pup. Based on their mass ratios, SX Aur can tentatively be assigned to the first phase of slow mass transfer and X Tri to the second phase. For V Pup (which is more massive) this choice can not be made with certainty. 相似文献
60.
L. D. De Feiter 《Space Science Reviews》1972,13(4-6):827-842
Recent observations of the energetic particles produced in solar flares indicate that the production of electrons, with energies up to about 100 keV, is a fairly common feature of small flares. In those flares the acceleration of protons and other nuclei does not extend beyond about 1 MeV.The X-ray emission often exhibits two distinct components of which the first one is produced by non-thermal, the second by thermal electrons through bremsstrahlung collisions with the ambient ions. Along with these X rays, radio emission, in the microwave region, is observed. This radio emission is usually interpreted as due to gyrosynchrotron radiation from the same electrons.In this review a discussion is presented of the processes occurring in solar flares with special reference to the acceleration and radiation processes. 相似文献