全文获取类型
收费全文 | 602篇 |
免费 | 84篇 |
国内免费 | 123篇 |
专业分类
航空 | 399篇 |
航天技术 | 234篇 |
综合类 | 75篇 |
航天 | 101篇 |
出版年
2024年 | 1篇 |
2023年 | 4篇 |
2022年 | 11篇 |
2021年 | 16篇 |
2020年 | 25篇 |
2019年 | 32篇 |
2018年 | 57篇 |
2017年 | 39篇 |
2016年 | 27篇 |
2015年 | 20篇 |
2014年 | 32篇 |
2013年 | 24篇 |
2012年 | 33篇 |
2011年 | 34篇 |
2010年 | 35篇 |
2009年 | 50篇 |
2008年 | 49篇 |
2007年 | 37篇 |
2006年 | 52篇 |
2005年 | 40篇 |
2004年 | 24篇 |
2003年 | 31篇 |
2002年 | 11篇 |
2001年 | 7篇 |
2000年 | 15篇 |
1999年 | 10篇 |
1998年 | 11篇 |
1997年 | 11篇 |
1996年 | 10篇 |
1995年 | 11篇 |
1994年 | 20篇 |
1993年 | 9篇 |
1992年 | 6篇 |
1991年 | 4篇 |
1990年 | 6篇 |
1989年 | 3篇 |
1984年 | 2篇 |
排序方式: 共有809条查询结果,搜索用时 500 毫秒
251.
The forecast of the terrestrial ring current as a major contributor to the stormtime Dst index and a predictor of geomagnetic storms is of central interest to ‘space weather’ programs. We thus discuss the dynamical
coupling of the solar wind to the Earth's magnetosphere during several geomagnetic storms using our ring current-atmosphere
interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution of H+, O+, and He+ ion distribution functions considering time-dependent inflow from the magnetotail, adiabatic drifts, and outflow from the
dayside magnetopause. Losses due to charge exchange, Coulomb collisions, and scattering by EMIC waves are included as well.
As initial and boundary conditions we use complementary data sets from spacecraft located at key regions in the inner magnetosphere,
Polar and the geosynchronous LANL satellites. We present recent model simulations of the stormtime ring current energization
due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring
current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric ring current. Near
minimum Dst there is a factor of ∼ 10 variation in the intensity of the dominant ring current ion specie with magnetic local time, its
energy density reaching maximum in the premidnight to postmidnight region. We find that the O+ content of the ring current increases after interplanetary shocks and reaches largest values near Dst minimum; ∼ 60% of the total ring current energy was carried by O+ during the main phase of the 15 July 2000 storm. The effects of magnetospheric convection and losses due to collisions and
wave-particle interactions on the global ring current energy balance are calculated during different storm phases and intercompared.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
252.
Cool giant and supergiant stars generally present low velocity winds with high mass-loss rates. Several models have been proposed
to explain the acceleration process of these winds. Although dust is known to be present in these objects, the radiation pressure
on these particles is uneffective in reproducing the observed physical parameters of the wind. The most promising acceleration
mechanism cited in the literature is the transference of momentum and energy from Alfvén waves to the gas. Usually, these
models consider the wind to be isothermal. We present a stellar wind model in which the Alfvén waves are used as the main
acceleration mechanism, and determine the temperature profile by solving the energy equation taking into account both the
radiative losses and the wave heating. We also determine, self-consistently, the magnetic field geometry as the result of
the competition between the magnetic field and the thermal pressure gradient. As the main result, we show that the magnetic
geometry presents a super-radial index in the region where the gas pressure is increasing. However, this super-radial index
is greater than that observed for the solar corona. 相似文献
253.
通过分析高频磁场作用下熔体连续处理时夹杂的去除效率表明,熔体连续处理条件下的夹杂去除效率比熔体静止时的略低,而夹杂与熔体之间的密度差对电磁分离时的去除效率影响不大。提高去除效率的有效途径是增大磁感应强度或降低分离器管径,但减小管径的同时需要提高磁场频率,以保持α/δ的值在2附近才可以取得最佳的分离效果。 相似文献
254.
255.
José Luis Ballester 《Space Science Reviews》2006,122(1-4):129-135
Prominence seismology is a rapidly developing topic which seeks to infer the internal structure and properties of solar prominences
from the study of its oscillations. Two-dimensional high-resolution observations suggest that filaments can be considered
as made by small scale fibrils, having a cool region, stacked one after another in the vertical and horizontal directions.
An extense observational background about oscillations in filaments has been gathered during the last 20 years and these observations
point out that fibrils or groups of fibrils can oscillate independently. From the theoretical point of view, small amplitude
oscillations in single and multifibril configurations have been studied as a first step to explain observational features. 相似文献
256.
A. A. Van Ballegooijen 《Space Science Reviews》1994,68(1-4):299-307
The interaction of a stellar magnetosphere with a thin accretion disk is considered. Specifically, I consider a model in which (1) the accretion disk is magnetically linked to the star over a large range of radii and (2) the magnetic diffusivity of the disk is sufficiently small that there is little slippage of field lines within the disk on the rotation time scale. In this case the magnetic energy built up as a result of differential rotation between the star and the disk is released in quasi-periodic reconnection events occuring in the magnetosphere (Aly and Kuijpers 1990). The radial transport of magnetic flux in such an accretion disk is considered. It is show that the magnetic flux distribution is stationary on the accretion time scale, provided the time average of the radial component of the field just above the disk vanishes. A simple model of the time-dependent structure of the magnetosphere is presented. It is shown that energy release in the magnetosphere must take place for (differential) rotation angles less than about 3 radians. The magnetic flux distribution in the disk depends on the precise value of the rotation angle. 相似文献
257.
分别从磁化理论和数理统计两个方面分析了影响耐蚀软磁合金1J116磁性能的因素。对某钢厂不同生产时期的生产质量水平通过理论计算进行了评估;研究了化学元素C不同含量对材料磁性能的影响;通过计算得到了提高磁性能的有效C含量范围。 相似文献
258.
稀薄效应对可倾瓦动压气体轴承性能的影响 总被引:2,自引:2,他引:0
以微型三可倾瓦动压气体轴承为研究对象,采用连续模型、一阶滑移模型和WU新滑移模型速度边界条件,建立考虑稀薄效应的滑移修正雷诺方程。结合牛顿迭代法和有限差分法求解修正雷诺方程,计算考虑稀薄效应的三可倾瓦动压气体轴承各瓦块压力分布和承载力。计算结果表明:三可倾瓦动压气体轴承偏心率越大,转速越大,压缩系数越大,轴承承载力越大;考虑稀薄效应后,计算出的可倾瓦动压气体轴承承载力明显下降,且随着克努森数的增大,WU新滑移模型计算得到的承载力明显低于一阶滑移模型。 相似文献
259.
260.
目前用于探测定位的舰船磁场模型中应用最为广泛的是磁偶极子模型,但是对于磁偶极子模型的适用观测距离缺乏定量研究。文章利用椭球体模型近似表达实际磁场,通过椭球体模型与磁偶极子模型的仿真比较,对磁偶极子模型的适用观测距离进行定量研究,得出磁偶极子模型的适用条件。 相似文献