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991.
Wei Fengsi Feng Xueshang Guo Jian-shan Fan Quanlin Wu Jian 《Space Science Reviews》2003,107(1-2):327-334
Recent progress in space weather research are briefly presented here from three aspects: establishment or improvement in observation
systems, such as extra-soft X-ray detector and γ-ray detector onboard the spacecraft ‘Shen Zhou 2’, new solar radio broad-band
spectrometer, magnetometer-chain, ionosonde and digisonde–chain, laser-lidar system and VHF radar; partial topic progresses
included in CMEs, multi-streamer structures, evolution of interplanetary magnetic field B
z component, regional properties of traveling ionospheric disturbances, a fully-nonlinear global dynamical model for the middle
and upper atmosphere, and a combined prediction method for geomagnetic disturbances; and space weather activity, such as ‘Meridian
Project’ — a national major scientific project, ‘International Space Weather Meridian Circle Program’ — a suggestion of internationalization
of ‘Meridian Project’, ‘Space Weather Research Plan’ — a major research plan from National Natural Science Foundation of China
(NNSFC) and other space weather activities.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
992.
993.
文章介绍了IEEE802.3 CRC-32的一种VHDL语言程序实现。对CRC的重要性进行了简要的介绍,重点讨论了CRC的算法分析、CRC-32的VHDL语言程序实现。 相似文献
994.
脉冲雷达在高仰角跟踪过程中存在不容忽视的动态滞后误差,该类误差的存在严重影响到雷达数据处理和弹/轨道精密确定。目前外测数据处理领域采用的基于误差电压和定向灵敏度的动态滞后误差修正模型,修正效果不理想。本文提出了一种用数值法修正雷达高仰角动态滞后误差的方法,并用任务实测数据进行了模型验证,结果显示这种方法能有效地降低动态滞后引起的误差。 相似文献
995.
平均绝对差图象匹配系统的定位精度 总被引:2,自引:1,他引:1
本文证明了两个基本定理。在假定图象信号和附加噪声是相互独立的零均值齐次高斯随机场、且二次可微的条件下,解决了平均绝对差图象匹配系统的定位精度的分析和计算问题。用实例说明了精度分析和计算的方法,分析了影响定位精度的因素和参数。为匹配性能的定量分析提供了理论依据和方法。 相似文献
996.
W.N. Brandt C. Vignali D.P. Schneider D.M. Alexander S.F. Anderson F.E. Bauer X. Fan G.P. Garmire S. Kaspi G.T. Richards 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2478-2485
X-ray studies of high-redshift (z > 4) active galaxies have advanced substantially over the past few years, largely due to results from the new generation of X-ray observatories. As of this writing X-ray emission has been detected from nearly 60 high-redshift active galaxies. This paper reviews the observational results and their implications for models of the first massive black holes, and it discusses future prospects for the field. 相似文献
997.
998.
Øieroset Marit Mitchell David L. Phan Tai D. Lin Robert P. Crider Dana H. Acuña Mario H. 《Space Science Reviews》2004,111(1-2):185-202
Using magnetometer and electron observations from the Mars Global Surveyor (MGS) and the Wind spacecraft we show that the region of magnetic field pile-up and density decrease located between the Martian ionosphere and bow shock exhibit strong similarities with the plasma depletion layer (PDL) observed upstream of the Earth's magnetopause in the absence of magnetic reconnection when the magnetopause is a solid obstacle in the solar wind. A PDL is formed upstream of the terrestrial magnetopause when the magnetic field piles up against the obstacle and particles in the pile-up region are squeezed away from the high magnetic pressure region along the field lines as the flux tubes convect toward the magnetopause. We here discuss the possibility that at least part of the region of magnetic field pile-up and density depletion upstream of Mars may be formed by the same physical processes which generate the PDL upstream of the Earth's magnetopause. More complete ion, electron, and neutral measurements are needed to conclusively determine the relative importance of the plasma depletion process versus exospheric processes. 相似文献
999.
The characteristics of inverted-V electron precipitation fluxes deduced predominantly from observations by the Atmosphere Explorer satellites are reviewed. The energy and pitch angle distributions are presented and shown to be generally in agreement with acceleration by a parallel electrostatic potential. Characteristics of secondary electrons are examined, and effects of beam plasma instabilities on these electrons are discussed. The properties of the monoenergetic component are compared with theoretical models of creating parallel DC electric fields, and found to favor the anomalous resistivity model. The article also discusses relations of inverted-V events with other auroral phenomena including auroras, electrostatic shocks, convective electric field reversals, field-aligned currents and wave emissions. The principal conclusions are: (1) plasma sheet electrons are continuously accelerated to form inverted-V structures in the pre-midnight hemisphere independent of substorm phase, (2) the acceleration processes are probably related to large scale electrostatic wave turbulence observed at altitudes of a few thousand kilometers, (3) narrow bursts of intense electron precipitation fluxes are found to be imbedded within some inverted-V's. It is argued that the narrow bursts of intense electron precipitation have the proper characteristics to cause discrete auroral arcs in the atmosphere. We suggest that these narrow bursts are accelerated by an electrostatic shock at higher altitude and capable of producing discrete auroral arcs below the observing satellite. 相似文献
1000.
Detonation waves induced by a confined wedge 总被引:2,自引:0,他引:2
An auto-ignition detonation phenomenon can be initiated by a wedge confined in a channel. A new, self-sustaining, normal detonation wave engine concept is proposed. The detonation processes were numerically modeled with a simplified two-dimensional wedged channel flow that was deemed to emulate a real three-dimensional configuration. The results showed that within certain ranges of incoming flow Mach number or wedge angle, detonation could be self ignited in the channel. The study furthermore investigated the detonation waves based on three different detonation initiation positions. Different configurations of the detonation waves were observed and analyzed. The performance of the different detonation wave configurations was estimated and compared. 相似文献