全文获取类型
收费全文 | 8386篇 |
免费 | 318篇 |
国内免费 | 254篇 |
专业分类
航空 | 4167篇 |
航天技术 | 2773篇 |
综合类 | 218篇 |
航天 | 1800篇 |
出版年
2022年 | 74篇 |
2021年 | 129篇 |
2020年 | 65篇 |
2019年 | 92篇 |
2018年 | 203篇 |
2017年 | 152篇 |
2016年 | 162篇 |
2015年 | 120篇 |
2014年 | 268篇 |
2013年 | 302篇 |
2012年 | 310篇 |
2011年 | 441篇 |
2010年 | 332篇 |
2009年 | 426篇 |
2008年 | 443篇 |
2007年 | 306篇 |
2006年 | 238篇 |
2005年 | 275篇 |
2004年 | 237篇 |
2003年 | 248篇 |
2002年 | 190篇 |
2001年 | 267篇 |
2000年 | 164篇 |
1999年 | 221篇 |
1998年 | 238篇 |
1997年 | 138篇 |
1996年 | 211篇 |
1995年 | 240篇 |
1994年 | 228篇 |
1993年 | 163篇 |
1992年 | 187篇 |
1991年 | 89篇 |
1990年 | 66篇 |
1989年 | 166篇 |
1988年 | 81篇 |
1987年 | 63篇 |
1986年 | 70篇 |
1985年 | 185篇 |
1984年 | 146篇 |
1983年 | 111篇 |
1982年 | 116篇 |
1981年 | 217篇 |
1980年 | 50篇 |
1979年 | 45篇 |
1978年 | 50篇 |
1977年 | 42篇 |
1975年 | 51篇 |
1974年 | 39篇 |
1971年 | 35篇 |
1970年 | 37篇 |
排序方式: 共有8958条查询结果,搜索用时 15 毫秒
421.
422.
A.K. Sharma D.P. Nade S.S. Nikte P.T. Patil R.N. Ghodpage R.S. Vhatkar M.V. Rokade S. Gurubaran 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
This paper reports the nightglow observations of OI 630.0 nm emissions, made by using all sky imager operating at low latitude station Kolhapur (16.8°N, 74.2°E and dip lat. 10.6°N) during high sunspot number years of 24th solar cycle. The images are analyzed to study the nocturnal, seasonal and solar activity dependence occurrence of plasma bubbles. We observed EPBs in images regularly during a limited period 19:30 to 02:30 LT and reach maximum probability of occurrence at 22:30 LT. The observation pattern of EPBs shows nearly no occurrence during the month of May and it maximizes during the period October–April. The equinox and solstice seasonal variations in the occurrence of plasma bubbles show nearly equal and large differences, respectively, between years of 2010–11 and 2011–12. 相似文献
423.
S.I. Oronsaye L.A. McKinnell J.B. Habarulema 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
A new version of global empirical model for the ionospheric propagation factor, M(3000)F2 prediction is presented. Artificial neural network (ANN) technique was employed by considering the relevant geophysical input parameters which are known to influence the M(3000)F2 parameter. This new version is an update to the previous neural network based M(3000)F2 global model developed by Oyeyemi et al. (2007), and aims to address the inadequacy of the International Reference Ionosphere (IRI) M(3000)F2 model (the International Radio Consultative Committee (CCIR) M(3000)F2 model). The M(3000)F2 has been found to be relatively inaccurate in representing the diurnal structure of the low latitude region and the equatorial ionosphere. In particular, the existing hmF2 IRI model is unable to reproduce the sharp post-sunset drop in M(3000)F2 values, which correspond to a sharp post-sunset peak in the peak height of the F2 layer, hmF2. Data from 80 ionospheric stations globally, including a good number of stations in the low latitude region were considered for this work. M(3000)F2 hourly values from 1987 to 2008, spanning all periods of low and high solar activity were used for model development and verification process. The ability of the new model to predict the M(3000)F2 parameter especially in the low latitude and equatorial regions, which is known to be problematic for the existing IRI model is demonstrated. 相似文献
424.
A. Shalchi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We discuss the random walk of magnetic field lines in astrophysical plasmas. Based on the standard theory of field line diffusion we show that there are two asymptotic limits. In these limits field line wandering is universal because in both regimes the field line diffusion coefficient depends only on fundamental length scales and absolute magnetic field strengths. As examples we discuss the field line diffusion coefficient for different prominent turbulence models namely the slab model, the two-dimensional model, and the Goldreich–Sridhar model. We show that the field line diffusion coefficient for the latter model agrees with the results obtained for slab and two-dimensional turbulence in limiting cases. We also discuss the transport of energetic particles perpendicular with respect to the mean magnetic field. Based on the unified nonlinear transport theory we consider again asymptotic limits. It is shown that one can identify four different regimes in which the transport is again universal. In all four cases perpendicular transport only depends on fundamental length scales of turbulence, magnetic field values, and the parallel diffusion coefficient. 相似文献
425.
A.O. Olawepo J.O. Adeniyi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Ionosonde data from two equatorial stations in the African sector have been used to study the signatures of four strong geomagnetic storms on the height – electron density profiles of the equatorial ionosphere with the objective of investigating the effects and extent of the effects on the three layers of the equatorial ionosphere. The results showed that strong geomagnetic storms produced effects of varying degrees on the three layers of the ionosphere. Effect of strong geomagnetic storms on the lower layers of the equatorial ionosphere can be significant when compared with effect at the F2-layer. Fluctuations in the height of ionization within the E-layer were as much as 0% to +20.7% compared to −12.5% to +8.3% for the F2-layer. The 2007 version of the International Reference Ionosphere, IRI-07 storm-time model reproduced responses at the E-layer but overestimated the observed storm profiles for the F1- and F2-layers. 相似文献
426.
E.S. Seo T. Anderson D. Angelaszek S.J. Baek J. Baylon M. Buénerd M. Copley S. Coutu L. Derome B. Fields M. Gupta J.H. Han I.J. Howley H.G. Huh Y.S. Hwang H.J. Hyun I.S. Jeong D.H. Kah K.H. Kang D.Y. Kim H.J. Kim K.C. Kim M.H. Kim K. Kwashnak J. Lee M.H. Lee J.T. Link L. Lutz A. Malinin A. Menchaca-Rocha J.W. Mitchell S. Nutter O. Ofoha H. Park I.H. Park J.M. Park P. Patterson J.R. Smith J. Wu Y.S. Yoon 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The Cosmic Ray Energetics And Mass (CREAM) instrument is configured with a suite of particle detectors to measure TeV cosmic-ray elemental spectra from protons to iron nuclei over a wide energy range. The goal is to extend direct measurements of cosmic-ray composition to the highest energies practical, and thereby have enough overlap with ground based indirect measurements to answer questions on cosmic-ray origin, acceleration and propagation. The balloon-borne CREAM was flown successfully for about 161 days in six flights over Antarctica to measure elemental spectra of Z = 1–26 nuclei over the energy range 1010 to >1014 eV. Transforming the balloon instrument into ISS-CREAM involves identification and replacement of components that would be at risk in the International Space Station (ISS) environment, in addition to assessing safety and mission assurance concerns. The transformation process includes rigorous testing of components to reduce risks and increase survivability on the launch vehicle and operations on the ISS without negatively impacting the heritage of the successful CREAM design. The project status, including results from the ongoing analysis of existing data and, particularly, plans to increase the exposure factor by another order of magnitude utilizing the International Space Station are presented. 相似文献
427.
Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm
Iu.V. Cherniak I.E. Zakharenkova D. Dzubanov A. Krankowski 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30–45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere. 相似文献
428.
借鉴复合材料结构建模中的均匀化处理方法建立了压电网络板机电耦合动力学方程并对其进行求解,获得了耦合系统的频率特征方程;通过求解频率特征方程发现压电网络板的固有模态以耦合模态对的形式存在;在此基础上对耦合系统的频率特性进行了分析,表明耦合模态对的特征频率值随着电感的变化会出现频率转向现象.进一步通过对系统在频率转向区能量转换规律的研究,揭示了压电网络板中频率转向的意义.最后,分析了压电网络板设计参数对频率转向区特性的影响,为压电网络板的合理设计提供了理论参考. 相似文献
429.
利用四边固支板横向自由振动的精确解作为模态坐标,在模态空间求解了四边固支压电网络板的机电耦合动力学方程.基于对压电网络板在模拟单点激励下谐响应行为的计算分析,得到了控制其各阶共振的压电网络电路元件最优电学参数.电感电阻并联型四边固支压电网络板与四边简支压电网络板不同,其具有多个局部最优电学参数.通过分析这些最优参数对其他阶共振的影响,发现四边固支压电网络板具有多阶共振抑制效果,与电阻相比,该效果对电感更加敏感.电感电阻并联型四边固支压电网络板可以实现比电阻型四边固支压电网络板更好的单模态振动抑制效果,但同时其多模态振动抑制效果会降低. 相似文献
430.