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991.
E.V. Chubaryan R.M. Avakyan G.G. Harutyunyan A.S. Piloyan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(11):1359-1365
Recent astronomical observations of supernovae and cosmic microwave background indicate that the universe is accelerating. Scalar–tensor theories of gravity give rise to suitable cosmological models where a late-time accelerated expansion is naturally realized. In an alternative proposal the cosmic acceleration is generated by means of a scalar field (quintessence), in a way similar to the early-time inflation. In this paper, we consider two classes of cosmological models with scalar fields. The first one corresponds to the Jordan–Brans–Dicke tensor–scalar theory with a cosmological scalar and the second one contains a conformally coupled scalar field with quartic potential. In both type of models the cosmological dynamics is described and the deceleration parameter is evaluated. The values of the parameters are specified for which a late-time accelerated expansion is realized. 相似文献
992.
Ezequiel Echer Bruce T. Tsurutani Fernando L. Guarnieri 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
During the first half of November 2004, many solar flares and coronal mass ejections (CMEs) were associated with solar active region (AR) 10696. This paper attempts to identify the solar and interplanetary origins of two superstorms which occurred on 8 and 10 November with peak intensities of Dst = −373 nT and −289 nT, respectively. Southward interplanetary magnetic fields within a magnetic cloud (MC), and a sheath + MC were the causes of these two superstorms, respectively. Two different CME propagation models [Gopalswamy, N., Yashiro, S., Kaiser, M.L. et al. Predicting the 1-AU arrival times of coronal mass ejections. J. Geophys. Res. 106, 29207–29219, 2001; Gopalswamy, N.S., Lara, A., Manoharan, P.K. et al. An empirical model to predict the 1-AU arrival of interplanetary shocks. Adv. Space Res. 36, 2289–2294, 2005] were employed to attempt to identify the solar sources. It is found that the models identify several potential CMEs as possible sources for each of the superstorms. The two Gopalswamy et al. models give the possible sources for the first superstorm as CMEs on 2330 UT 4 November 2004 or on 1454 UT 5 November 2004. For the second superstorm, the possible solar source was a CME that on 0754 UT 5 November 2004 or one that occurred on 1206 UT 5 November 2004. We note that other propagation models sometimes agree and other times disagree with the above results. It is concluded that during high solar/interplanetary activity intervals such as this one, the exact solar source is difficult to identify. More refined propagation models are needed. 相似文献
993.
C. Taricco N. Bhandari P. Colombetti N. Verma 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(2):275-279
Measurements of 44Ti activity in meteorites show that the galactic cosmic ray (GCR) intensity has been declining in the interplanetary space during the past three centuries and has a component of cyclic variation, with periodicity of about 87 years [Taricco, C., Bhandari, N., Cane, D., et al. Galactic cosmic ray flux decline and periodicities in the interplanetary space during the last 3 centuries revealed by 44Ti in meteorites. J. Geophys. Res. 111, A08102, 2006.]. In order to verify these results, we have measured 44Ti activity in Allegan meteorite which fell in 1899 and in some other meteorites with better precision. The measurements confirm low cosmic ray flux and consequently high solar activity near the middle of 19th century. 相似文献
994.
对比研究了用于加速度表标定的重力场,离心机与电模拟的三种方法,给出了在国内目前没有大g值精密离心机条件下,如何解决大量程加速度表的系数标定问题。 相似文献
995.
W.Q. Gan Y.P. Li L.I. Miroshnichenko 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):908-913
The footpoint motions of flare hard X-ray (HXR) sources are directly related to the reconnection scenario of a solar flare. In this work, we tried to extract the information of footpoint motions for a number of flares observed with RHESSI. We found that the RHESSI flare results of the footpoint motions strongly support the classification proposed from the observations of YOHKOH/HXT. Furthermore, it is found that a flare can consist of two types of footpoint motions. We discussed the connections of the footpoint motions with the two-dimensional reconnection models. 相似文献
996.
K. Haijima K.G. Tanaka M. Fujimoto I. Shinohara 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1643-1648
Recent two-dimensional (2-D) particle-in-cell (PIC) simulations have shown that there is a critical thickness of a current sheet, above which no significant saturation amplitude of the 2-D tearing (TI) mode can be expected. Here, we have introduced the initial electron temperature anisotropy (αe0 = Te⊥/Te|| > 1), which is known to raise significantly the linear growth rates, and inspected if αe0 > 1 can change the saturation level of the TI in a super-critical current sheet. Varying αe0 and D (D: the current sheet half-thickness) systematically, we have found that while αe0 boosts up the linear growth rate in both sub- and super-critical current sheets, macroscopic effects are obtained only in sub-critical current sheets, that is, energy transfer from the fastest growing short wavelength modes to longer wavelength modes are available only in the sub-critical regime. Since the critical thickness is a fraction of the ion inertial length, the tearing mode assisted by the electron temperature anisotropy alone, despite its significant boost in the linear growth rate, cannot be the agent for reconnection triggering in a current sheet of ion-scale thickness. 相似文献
997.
Basem Elsaka Juergen Kusche Karl-Heinz Ilk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Temporal and mean gravity field models derived from the twin-satellite, leader–follower mission GRACE have provided a new type of information for Earth sciences. In this contribution, we study the potential of various alternative satellite formations for gravity field determination in the post-GRACE era in a simulation environment. In particular, the effects of spherical harmonic truncation and of temporal aliasing in the processing of gravity products from such future formations are investigated. 相似文献
998.
双旋流器单头部模型燃烧室冷态流场试验 总被引:10,自引:3,他引:7
利用PIV(Particle image velocimetry)技术对双轴向反旋旋流器、单头部、矩形模型燃烧室内的冷态流场进行了试验研究.分析了燃烧室的纵向截面、横向截面上的流场结构以及旋流器参数对回流区尺寸的影响.研究结果表明:双旋流燃烧室的流场为不规则的结构,中心轴上下两个涡不对称,各主燃孔气流穿透深度也不相同,流场中存在流向涡;减小一级旋流器流通面积、旋流数,或增大二级旋流器的旋流数,可增大回流区的尺寸,而增大二级旋流器流通面积,回流区的尺寸会减小. 相似文献
999.
针对电渣熔铸钢锭各部位温差大,易产生热应力及测量困难,本文采用大型有限元分析软件ANSYS对电渣熔铸过程中不同渣池深度时的钢锭应力场进行了模拟研究,研究结果表明不同渣池深度时的钢锭表面沿轴向自顶而下等效应力和轴向应力分布均基本遵循对数函数关系。模拟结果与实际相吻合,运用此模型可预报钢锭应力场状况,指导实际生产。 相似文献
1000.
空间微重力磁悬浮平台激励器研究 总被引:3,自引:0,他引:3
为满足空间实验室的科学实验载荷对微重力环境水平的要求,需要保证空间微重力实验载荷平台的振动隔离性能,即需要平台激励器能在控制系统的作用下适时地产生抑制平台扰动的激励力.本文提出了平台激励器的初步指标,从磁悬浮基本原理出发设计出多种结构形式,在此结构基础上完成有限元磁路仿真和激励器的线圈设计,并对各种结构形式进行比较,根据比较结果总结出各结构形式的优缺点,为激励器的具体设计提供了依据. 相似文献