全文获取类型
收费全文 | 908篇 |
免费 | 88篇 |
国内免费 | 182篇 |
专业分类
航空 | 609篇 |
航天技术 | 327篇 |
综合类 | 111篇 |
航天 | 131篇 |
出版年
2024年 | 1篇 |
2023年 | 36篇 |
2022年 | 8篇 |
2021年 | 21篇 |
2020年 | 27篇 |
2019年 | 43篇 |
2018年 | 31篇 |
2017年 | 31篇 |
2016年 | 34篇 |
2015年 | 31篇 |
2014年 | 83篇 |
2013年 | 26篇 |
2012年 | 46篇 |
2011年 | 52篇 |
2010年 | 39篇 |
2009年 | 44篇 |
2008年 | 87篇 |
2007年 | 71篇 |
2006年 | 46篇 |
2005年 | 45篇 |
2004年 | 34篇 |
2003年 | 32篇 |
2002年 | 16篇 |
2001年 | 46篇 |
2000年 | 17篇 |
1999年 | 19篇 |
1998年 | 23篇 |
1997年 | 16篇 |
1996年 | 25篇 |
1995年 | 21篇 |
1994年 | 67篇 |
1993年 | 22篇 |
1992年 | 5篇 |
1991年 | 7篇 |
1990年 | 4篇 |
1989年 | 8篇 |
1988年 | 5篇 |
1987年 | 1篇 |
1984年 | 8篇 |
排序方式: 共有1178条查询结果,搜索用时 15 毫秒
171.
Yann Alibert Christoph Mordasini Olivier Mousis Willy Benz 《Space Science Reviews》2005,116(1-2):77-95
We present models of giant planet formation, taking into account migration and disk viscous evolution. We show that migration
can significantly reduce the formation timescale bringing it in good agreement with typical observed disk lifetimes. We then
present a model that produces a planet whose current location, core mass and total mass are comparable with the one of Jupiter.
For this model, we calculate the enrichments in volatiles and compare them with the one measured by the Galileo probe. We
show that our models can reproduce both the measured atmosphere enrichments and the constraints derived by Guillot et al. (2004), if we assume the accretion of planetesimals with ices/rocks ratio equal to 4, and that a substantial amount of CO2 was present in vapor phase in the solar nebula, in agreement with ISM measurements. 相似文献
172.
Werner Schmutz 《Space Science Reviews》1993,66(1-4):253-261
A standard non-LTE Wolf-Rayet star atmosphere model is compared with an identical model but including line-blanketing. The structures of the two models are presented in detail and the implications of blanketed models for spectroscopic analyses are discussed. 相似文献
173.
论述了企业应变能力的结构,内容及各层次间应变的特征,以应变能力在各责任单位之间的传递过程作了描述,用传递矩阵方法研究了应变能力在企业四个层次上的目标与保证关系,建立了一套实用的评价、诊断的定量指标体系。 相似文献
174.
杨惠 《中国民航学院学报》1994,(4)
自汉朝以来,以儒家法律思想为主的封建正统法律思想在中国法律史上一直处于独尊独尚的地位。然而,清廷统治的最后十年,一场史无前例的变法修律,却首开吸收西方资产阶级法律思想入律之先河,第一次对封建正统法律思想的根本原则,基本内容等进行了突破、改易。尽管这些突破是有限的,但它足以表明晚清修律终于结束了两千多年来封建正统法律思想的垄断统治,终于使中国古代法律冲破了旧的樊篱,迈上了近现代型的历史轨道,为新的法律思想的发展完善开拓出了广阔的空间。 相似文献
175.
以微机、LH-SC16A型A/D板、SC50型D/A板以及TMS320C30A型DSP板为基础,建立了时域结构响应主动控制的主从机并行处理系统。这一系统具有多通道快速运算能力,可提高控制系统的控制律,更新速率,改善控制系统的跟踪能力。 相似文献
176.
“自准”赝像及识别 总被引:1,自引:0,他引:1
金重 《中国民航学院学报》1996,(6):68-71
置平面镜于凸透镜后,则凸透镜前焦平面上的物成像于该物平面上,即“自准”成像.满足其它条件也能成像于物平面.分析不同条件下像的形成及其特点,并给出识别自准成像的判据. 相似文献
177.
郝红武 《西安航空技术高等专科学校学报》2005,23(3):31-32
通过对强度理论、杆件拉伸概念及公式的分析研究,引入实验元件的几何刚度和弹性稳定性系数的概念,推导出实验元件的拉伸位移变化率的公式,并以此进行实验元件的破坏预估及结构模型修正。 相似文献
178.
气动伺服弹性研究的进展与挑战 总被引:4,自引:1,他引:3
飞机、导弹等飞行器的气动伺服弹性(ASE)问题源于空气动力、结构弹性以及控制系统之间的复杂耦合。随着飞行器朝着结构更轻、速度更快、性能更好的目标发展,该问题日益突出,直接影响飞行安全与性能。经过六十余年的研究,国内外在ASE分析、综合与试验方面取得了卓有成效的进展。近十余年来,若干新问题因非常规构型飞行器设计的发展而暴露出来,对ASE研究施加巨大挑战,值得重点分析。鉴于此,讨论了ASE分析中的刚弹耦合、非线性、推力矢量以及系统辨识等问题,对ASE综合中的阵风减缓、颤振主动控制和ASE优化问题加以阐述,强调了ASE试验中需要重视的技术,简要介绍了近十余年国外代表性的ASE试验项目案例,指出了一些ASE研究的新动向,并对国内的ASE研究给出了建议。 相似文献
179.
Understanding properties of solar energetic particle (SEP) events associated with coronal mass ejections has been identified
as a key problem in solar-terrestrial physics. Although recent CME shock acceleration models are highly promising, detailed
agreement between theoretical predictions and observations has remained elusive. Recent observations from ACE have shown substantial
enrichments in the abundances of 3He and He+ ions which are extremely rare in the thermal solar wind plasma. Consequently, these ions act as tracers of their source material,
i.e.,
3He ions are flare suprathermals and He+ ions are interstellar pickup ions. The average heavy ion composition also exhibits unsystematic differences when compared
with the solar wind values, but correlates significantly with the ambient suprathermal material abundances. Taken together
these results provide compelling evidence that CME-driven shocks draw their source material from the ubiquitous but largely
unexplored suprathermal tail rather than from the more abundant solar wind peak. However, the suprathermal energy regime has
many more contributors and exhibits much larger variability than the solar wind, and as such needs to be investigated more
thoroughly. Answers to fundamental new questions regarding the preferred injection of the suprathermal ions, the spatial and
temporal dependence of the various sources, and the causes of their variability and their effects on the SEP properties are
needed to improve agreement between the simulations and observations. 相似文献
180.
The current status of the theory of a new astrophysical phenomenon, aradiation-driven diskon, is outlined.The cyclotron radiation pressure around sufficiently hot, strongly magnetized white dwarfs and neutron stars is shown to be able to drive a wind from the photosphere and support a plasma envelope in the closed part of the magnetosphere. The magnetohydrostatic configuration of an optically thin, radiatively supported plasma envelope is determined. It consists of an equatorial disk in the region where the cyclotron radiation force exceeds the local force of gravity and a closed shell near the equilibrium surface where the radiation pressure equals gravity. The effects of finite optical depth on the behaviour of the magnetospheric plasma and the influence of the envelope on the observed radiation are discussed.Classes of magnetic degenerate stars are pointed out in which radiation-driven diskons may be found. The best candidates are two individual stars, the strongly magnetized white dwarfs GD 229 and PG 1031+234. Both exhibit broad and deep depressions in the ultraviolet which are explained as a result of cyclotron scattering by an optically thick radiation-driven envelope in the inhomogeneous magnetic field of the star. We predict a temporal and spectral variability of these features due to non-stationary plasma motions in the envelope. 相似文献