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971.
B.M. Pilkerton M.R. Collier T.E. Moore 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2152-2156
We report results of a statistical study correlating ionized solar wind (ISW) fluxes observed by ACE during late 2000 and throughout 2001 with neutral solar wind (NSW) fluxes observed by IMAGE/LENA over the same period. The average correlation coefficient between the neutral and ionized solar wind is 0.66 with correlations greater than 0.80 occurring about 29% of the time. Correlations appear to be driven by high solar wind flux variability, similar to results obtained by in situ multi-spacecraft correlation studies. In this study, however, IMAGE remains inside the magnetosphere on over 95% of its orbits. As a function of day of year, or equivalently ecliptic longitude, the slope of the relationship between the neutral solar wind flux and the ionized solar wind flux shows an enhancement near the upstream direction, but the symmetry point appears shifted toward higher ecliptic longitudes than the interstellar neutral (ISN) flow direction by about 20°. The estimated peak interstellar neutral upstream density inside of 1 AU is about 7 × 10−3 cm−3. 相似文献
972.
采用时间累计法对基本维修作业建立数学模型,解决了表格式工时定额数据多、误差大、使用不便和管理复杂等问题。而且,通过设计和建立数学模型数据库系统,为计算机辅助制定工时定额创造了条件。以基本维修作业为研究对象,系统地分析了基本维修作业划分和量化的方法及步骤,包括模型确定的方法和系数求解公式,并对基于累计法的基本维修作业数学模型进行了深入的研究,从而得到了工时定额评估的一般方法。 相似文献
973.
This brief report summarized the latest advances of the interplanetary physics research in China during the period of 2004-2005, made independently by Chinese space physicists and through international collaboration. The report covers all aspects of the interplanetary physics, including theoretical studies, numerical simulation and data analysis. 相似文献
974.
程玉民 《华北航天工业学院学报》2000,10(1):28-30
作业成本计算(Activity—Based Costing,简称ABC)是西方国家于八十年代末开始研究、九十年代以来在先进制造企业首先应用起来的一种全新的企业管理理论和方法。本文从作业成本计算冲破了传统成本计算的思维模式,为企业的经营管理提供了更加准确监控信息的角度,对作业成本计算的基本原理进行了粗浅的探讨。随着计算机在管理中的广泛应用,作业成本计算必将成为一种新的现代管理方法受到企业管理者的青睐。 相似文献
975.
Yang Su W.Q. GanY.P. Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):988-991
Based on the light curves and images of RHESSI flares, we tried to make a preliminary classification of solar flares. Three basic types of flares seem to be existed: accordantly gradual flares, accordantly impulsive flares, and early impulsive flares. The proportion for each type is given. The possible physical meaning related to different types is discussed. 相似文献
976.
M. Fujimoto W. Baumjohann K. Kabin R. Nakamura J. A. Slavin N. Terada L. Zelenyi 《Space Science Reviews》2007,132(2-4):529-550
The small intrinsic magnetic field of Mercury together with its proximity to the Sun makes the Hermean magnetosphere unique in the context of comparative magnetosphere study. The basic framework of the Hermean magnetosphere is believed to be the same as that of Earth. However, there exist various differences which cause new and exciting effects not present at Earth to appear. These new effects may force a substantial correction of our naïve predictions concerning the magnetosphere of Mercury. Here, we outline the predictions based on our experience at Earth and what effects can drastically change this picture. The basic structure of the magnetosphere is likely to be understood by scaling the Earth’s case but its dynamic aspect is likely modified significantly by the smallness of the Hermean magnetosphere and the substantial presence of heavy ions coming from the planet’s surface. 相似文献
977.
V. V. Izmodenov 《Space Science Reviews》2007,130(1-4):377-387
Interstellar atoms penetrate deep into the heliosphere after passing through the heliospheric interface—the region of the
interaction of the solar wind with the interstellar medium. The heliospheric interface serves as a filter for the interstellar
atoms of hydrogen and oxygen, and, to a lesser extent, nitrogen, due to their coupling with interstellar and heliospheric
plasmas by charge exchange and electron impact ionization. The filtration has great importance for the determination of local
interstellar abundances of these elements, which becomes now possible due to measurements of interstellar pickup by Ulysses
and ACE, and anomalous cosmic rays by Voyagers, Ulysses, ACE, SAMPEX and Wind. The filtration of the different elements depends
on the level of their coupling with the plasma in the interaction region. The recent studies of the filtration of the interstellar
atoms in the heliospheric interface region is reviewed in this paper. The dependence of the filtration on the local interstellar
proton and H atom number densities is discussed and the roles of the charge exchange and electron impact ionization on the
filtration are evaluated. The influence of electron temperature in the inner heliosheath on the filtration process is discussed
as well. Using the filtration coefficients obtained from the modeling and SWICS/Ulysses pickup ion measurements, the local
interstellar abundances of the considered elements are determined. 相似文献
978.
Observations in the solar wind have revealed important insights into how energetic particles are accelerated in astrophysical
plasmas. In circumstances where stochastic acceleration is expected, a suprathermal tail on the distribution function is formed
with a common spectral shape: the spectrum is a power law in particle speed with a spectral index of −5. Recent theories for
this phenomenon, in which thermodynamic constraints are applied to explain the common spectral shape, are reviewed. As an
example of potential extensions of this theoretical work, consideration is given to the acceleration of Anomalous Cosmic Rays
in the heliosheath. 相似文献
979.
G. Murtaza S. IqbalM.A. Ameen A. Iqbal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
We have used the technique of expansion in Empirical Orthogonal Functions (EOFs) to develop regional models of the critical frequencies of E and F2 layers (foE, foF2), peak height (hmF2), and semi-thickness of F2 layer (YmF2) over Pakistan. In the present study levels of solar activity specified by Smoothed Sunspot Number (R) from 10 to 200 are taken into account. The magnetic dip angle for the model ranges from 30° to 60°. We have compared the regional model and the International Reference Ionosphere (IRI) with measurements of three ionosondes in Pakistan. The model parameters foE and foF2 are found overall comparable to the observed hourly median values during daytime at Karachi (geographic latitude = 24.95°N, longitude = 67.13°E, magnetic inclination = 37°), Multan (30.18°N, 71.48°E, 45°) and Islamabad (33.75°N, 73.13°E, 51.5°) during the years 1988, 1996 and 2000. For hmF2 the computed values by regional and IRI model for the year 1995 are found close to each other. However, for YmF2the results are better during daytime as compared to nighttime. 相似文献
980.