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181.
质子耀斑活动区的再现规律 总被引:3,自引:2,他引:1
质子耀斑活动区再现规律的研究结果表明,日面上存在着经度方向漂移式的“活火山”,即质子活动复活体,“活火山”定期地复活,并爆发质子耀斑。其复活长周期为8-11.6年,与活动周11年周期基本一致;短周期为1.26年,与活动周峰年时间宽度一致。在22周峰年中,日面南北半球上各有一个强质子活动复活体,它们爆发值流量≥100pfu和≥1000pfu的质子耀斑各占周期同类耀斑总数的70.7%和83.3%。 相似文献
182.
本文主要阐述了实验的重要性和实验教学的重要地位,实验教学观念转变及实验室如何建设发展,实验室的建设发展对高等院校教学与科研的重要作用,对高等院校的知名度和经济效益,吸引人才等方面起到的推动作用。 相似文献
183.
184.
卫生捕获太阳的新方法 总被引:2,自引:1,他引:2
对卫星入轨后捕获太阳的方法进行了研究,并对一种有效的控制规律进行了分析计算,最后对卫星的运动过程进行了仿真验证。 相似文献
185.
江泽民同志提出的“三个代表”的重要思想,是站在世纪之交的时代高度,总揽全局,对我党近80年历史经验和50年执政经验的总结,提出了加强执政党自身建设的新思路,创造性地发展了马克思主义党建理论与学说,具有鲜明的时代特点。本文就“三个代表”思想所体现的时代特点进行了初步的探讨,论证了其内在逻辑上的统一性,指出了“三个代表”思想必将成为新世纪党建理论的强大思想武器和伟大旗帜。 相似文献
186.
开环全保偏光纤陀螺结构简单,有使用价值;进入90年代国外研究成功熔接型保偏光纤耦合器以后,这种陀螺更受重视,向实用方向发展,对研究全保偏光纤陀螺中的几个关键问题,光路中元器件的特性;保偏光纤的对轴熔接技术,零漂和噪声做了分析,实验结果表明,零漂达到1.24°/h。 相似文献
187.
D. Beliu-Ionescu A.-C. Donea C. Lindsey P. Cally G. Mari 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,40(12):1921-1925
Some flares are known to drive seismic transients into the solar interior. The effects of these seismic transients are seen in helioseismic observations of the Sun’s surface thousands of km from their sources in the hour succeeding the impulsive phase of the flare. Energetic particles impinging from the corona into the chromosphere are known to drive strong, downward-propagating shocks in active region chromospheres during the impulsive phases of flares. H observations have served as an important diagnostic of these shocks, showing intense emission with characteristic transient redshifts. In most flares no detectable transients penetrate beneath the active region photosphere. In those that do, there is a strong correlation between compact white-light emission and the signature of seismic emission. This study introduces the first known H observations of acoustically active flares, centered in the core of the line. The morphology of line-core emission H in the impulsive phase of the flare is similar to that of co-spatial line-core emission in NaD1, encompassing the site of seismic emission but more extended. The latter shows a compact red shift in the region of seismic emission, but a similar feature is known to appear in a conjugate magnetic footpoint from which no seismic emission emanates. Radiative MHD modelling based on the profiles of chromospheric line emission during the impulsive phases of flares can contribute significantly to our understanding of the mechanics of flare acoustic emission penetrating into the solar interior and the conditions under which it occurs. 相似文献
188.
T.S. Kiss N. Gyenge R. Erdélyi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(2):611-616
Jets, whatever small (e.g. spicules) or large (e.g. macrospicules) their size, may play a key role in momentum and energy transport from photosphere to chromosphere and at least to the low corona. Here, we investigate the properties of abundant, large-scale dynamic jets observable in the solar atmosphere: the macrospicules (MS). These jets are observationally more distinct phenomena than their little, and perhaps more ubiquitous, cousins, the spicules. Investigation of long-term variation of the properties of macrospicules may help to a better understanding of their underlying physics of generation and role in coronal heating. Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory, a new dataset, with several hundreds of macrospicules, was constructed encompassing a period of observations over six years. Here, we analyse the measured properties and relations between these properties of macrospicules as function of time during the observed time interval. We found that cross-correlations of several of these macrospicule properties display a strong oscillatory pattern. Next, wavelet analysis is used to provide more detailed information about the temporal behaviour of the various properties of MS. For coronal hole macrospicules, a significant peak is found at around 2-year period. This peak also exists partially or is shifted to longer period, in the case of quiet Sun macrospicules. These observed findings may be rooted in the underlying mechanism generating the solar magnetic field, i.e. the global solar dynamo. 相似文献
189.
Hiroya Yamaguchi Midori Ozawa Takao Ohnishi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We report the discovery of recombining plasmas in three supernova remnants (SNRs) with the Suzaku X-ray astronomy satellite. During SNR’s evolution, the expanding supernova ejecta and the ambient matter are compressed and heated by the reverse and forward shocks to form an X-ray emitting hot plasma. Since ionization proceeds slowly compared to shock heating, most young or middle-aged SNRs have ionizing (underionized) plasmas. Owing to high sensitivity of Suzaku, however, we have detected radiative recombination continua (RRCs) from the SNRs IC 443, W49B, and G359.1–0.5. The presence of the strong RRC is the definitive evidence that the plasma is recombining (overionized). As a possible origin of the overionization, an interaction between the ejecta and dense circumstellar matter is proposed; the highly ionized gas was made at the initial phase of the SNR evolution in dense regions, and subsequent rapid adiabatic expansion caused sudden cooling of the electrons. The analysis on the full X-ray band spectrum of IC 443, which is newly presented in this paper, provides a consistent picture with this scenario. We also comment on the implications from the fact that all the SNRs having recombining plasmas are correlated with the mixed-morphology class. 相似文献
190.
S. Veretenenko M. Ogurtsov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
In this work we studied the spatial and temporal structure of long-term effects of solar activity (SA) and galactic cosmic ray (GCR) variations on the lower atmosphere circulation as well as possible reasons for the peculiarities of this structure. The study revealed a strong latitudinal and regional dependence of SA/GCR effects on pressure variations in the lower troposphere which seems to be determined by specific features of baric systems formed in different regions. The temporal structure of SA/GCR effects on the troposphere circulation at high and middle latitudes is characterized by a roughly 60-year periodicity which is apparently due to the epochs of the large-scale atmospheric circulation. It is suggested that a possible mechanism of long-term effects of solar activity and cosmic ray variations on the troposphere circulation involves changes in the evolution of the polar vortex in the stratosphere of high latitudes, as well as planetary frontal zones. 相似文献