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51.
Sandrine D’Hoedt Benoît Noyelles Julien DufeyAnne Lemaitre 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Mercury is the target of two space missions: MESSENGER, which carried out its first and second flybys of Mercury on January 14, 2008 and October 6, 2008, and the ESA/JAXA space mission BepiColombo, scheduled to arrive at Mercury in 2020. The preparation of these missions requires a good knowledge of the rotation of Mercury. 相似文献
52.
53.
以某型卫星测试转台俯仰机构为研究对象,在ADAMS中建立了虚拟样机,得到了在翻转过程中丝杠轴向力曲线,并将仿真结果与理论计算结果及试验结果进行比较,验证了虚拟样机建模的合理性;研究结果为同类物理样机设计中滚珠丝杠的选用校核,台体框架的设计校核以及机电联合仿真提供有利数据支撑。 相似文献
54.
Bruno Sicardy 《Space Science Reviews》2005,116(1-2):457-470
Planetary rings are found around all four giant planets of our solar system. These collisional and highly flattened disks
exhibit a whole wealth of physical processes involving dust grains up to meter-sized boulders. These processes, together with
ring composition, can help understand better the formation and evolution of proto-satellite and proto-planetary disks in the
early solar system. The present chapter reviews some fundamental aspects of ring dynamics and composition. The forthcoming
exploration of the Saturn system by the Cassini mission will bring both high resolution and time-dependent information on Saturn’s rings. 相似文献
55.
M. Stepanova E. Antonova O. Troshichev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2423-2427
One minute resolution Polar Cap (PC) index was used for the analysis of magnetospheric dynamics. The 1995–2000 time series analysis revealed that the power spectrum of the PC-index fluctuations is a power law in a wide range of frequencies. However, the obtained exponents differ for low and high frequency regions. The probability distribution functions of the PC-index fluctuations show a strong non-gaussian shape, depending on the time of increment. This indicates that the PC-index exhibits intermittency, previously detected in solar wind and auroral electrojet index fluctuations. The PC-index probability distribution functions were fitted by the functional form proposed by Castaing et al. [Velocity probability density functions of high Reynolds number turbulence. Physica D. 46, 177–200, 1990] to describe intermittency phenomena in ordinary turbulent fluid flows. The agreement between the fitting parameters obtained for the PC index and those reported before for solar wind magnetic field fluctuations is within 30%; which is noticeably less than the difference between the same parameters of solar wind and the AE-index fluctuations. This fact indicates that the PC index reflects the solar wind influence on the high-latitude magnetosphere, especially during the summer. 相似文献
56.
Wiesław M. Macek 《Space Science Reviews》2006,122(1-4):329-337
The question of multifractality is of great importance because it allows us to investigate interplanetary hydromagnetic turbulence.
The multifractal spectrum has been investigated with Voyager (magnetic field) data in the outer heliosphere and with Helios
(plasma) data in the inner heliosphere. We use the Grassberger and Procaccia method that allows calculation of the generalized
dimensions of the solar wind attractor in the phase space directly from the cleaned experimental signal. We analyze time series
of plasma parameters of the low-speed streams of the solar wind measured in situ by Helios in the inner heliosphere. The resulting spectrum of dimensions shows a multifractal structure of the solar wind
attractor. In order to quantify that multifractality, we use a simple analytical model of the dynamical system. Namely, we
consider the generalized self-similar baker’s map with two parameters describing uniform compression and natural invariant
measure on the attractor of the system. The action of this map exhibits stretching and folding properties leading to sensitive
dependence on initial conditions. The obtained solar wind singularity spectrum is consistent with that for the multifractal
measure on the weighted baker’s map. 相似文献
57.
Giuseppe Consolini Paola De Michelis Matthieu Kretzschmar 《Space Science Reviews》2006,122(1-4):293-299
Recent studies evidenced that the magnetotail dynamics looks like the one of an avalanching system. This fact has been related
with a near criticality dynamics and modelled by singular diffusion and transport equations. Here, we discuss some features
of the Earth’s magnetotail dynamics using a thermodynamic approach. In detail we discuss the role played by fluctuations in
singular diffusion and relaxation processes from a non-equilibrium thermodynamics point of view. Moreover, the emergence of
non-Gaussian statistics is discussed in the framework of the thermodynamics of composite systems. 相似文献
58.
利用动量矩定理推导出带伸展弹性板航天器的姿态动力学方程,在弹性板等速伸展的情况下,导出板的振动与伸展运动耦合微分方程,航天器姿态运动与板的伸展运动、振动耦合微分方程,通过龙格-库搭积分法得出了数值解,结果表明:弹性板等速伸展时,其振动的振幅随板长度的增长而增大,航天器姿态角速度随板长度的增长而减少。弹性板等速率越大,板振动的振幅越大。 相似文献
59.
M. Roos-Serote 《Space Science Reviews》2005,116(1-2):201-210
Titan’ atmosphere shows some similarities with that of the Earth, in terms of composition and surface pressure. Also, its
seasonal cycle is similar, as Titan’ obliquity is about 27°(23°,5 for the Earth), although it is about 30 times as long.
Titan’ haze exhibits an albedo contrast (NSA for North-South Asymmetry) that is changing seasonally. From the analysis of
Voyager and Hubble Space Telescope data, we learned that at short visible wavelengths, the albedo of the winter hemisphere
is lower by 10-20% than that of the summer hemisphere. This asymmetry peaks at 450 nm and reaches maximum amplitude around
Titan’ equinoxes. It reverses in about five years, faster than a season which spans seven years. At longer wavelengths, longward
of 700 nm, the asymmetry is inverted. The NSA reversal process in the red and in the UV seems to lead the reversal in the
blue by 1 or 2 years. No valid explanation exists for this lag, at least in the red.
The results from a recent model which couples atmospheric dynamics, haze microphysics and transport, as well as photochemistry,
show that the NSA and its seasonal changes can be explained by
an accumulation of haze particles at the winter pole. This is due to the pole-to-pole Hadley circulation pattern that is present
during most of Titan’ year and rapidly disrupts at the time of the equinoxes. This model can also explain the observed cooler
stratospheric temperatures and higher abundances of heavy hydrocarbons and nitriles in the winter polar region. In addition,
it provides a mechanism for the formation of a detached haze layer around 300–400 km altitude, as well as the existence of
a polar hood.
Thus, it appears that the latitudinal contrasts we observe on Titan are conveniently tracing for us the dynamical behavior
of its atmosphere. 相似文献
60.
本文对JJ-7飞机的横航向晴空大气紊流响应及乘座品质进行了计算.计算结果表明,JJ-7飞机的横航向大气紊流响应值不大,乘座品质基本上满足要求,可以为飞行员接受. 相似文献