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排序方式: 共有9473条查询结果,搜索用时 31 毫秒
971.
972.
Terrestrial technology is now, and increasingly, sensitive to space weather. Most space weather is caused by solar storms
and the resulting changes to the Earth's radiation environment and the magnetosphere. The Sun as the driver of space weather
is under intense observation but remains to be adequately modelled. Recent spacecraft measurements are greatly improving models
of solar activity, the interaction of the solar wind with the magnetosphere, and models of the radiation belts. In-situ data
updates the basic magnetospheric model to provide specific details of high-energy electron flux at satellite orbits. Shock
wave effects at the magnetopause can also be coarsely predicted. However, the specific geomagnetic effects at ground level
depend on the calculation of magnetic and electric fields and further improvements are needed. New work on physical models
is showing promise of raising geomagnetic and ionospheric predictability above the synoptic climatological level.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
973.
Kamide Y. Kihn E.A. Ridley A.J. Cliver E.W. Kadowaki Y. 《Space Science Reviews》2003,107(1-2):307-316
We report the recent progress in our joint program of real-time mapping of ionospheric electric fields and currents and field-aligned
currents through the Geospace Environment Data Analysis System (GEDAS) at the Solar-Terrestrial Environment Laboratory and
similar computer systems in the world. Data from individual ground magnetometers as well as from the solar wind are collected
by these systems and are used as input for the KRM and AMIE magnetogram-inversion algorithms, which calculate the two-dimensional
distribution of the ionospheric parameters. One of the goals of this program is to specify the solar-terrestrial environment
in terms of ionospheric processes, providing the scientific community with more than what geomagnetic activity indices and
statistical models provide.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
974.
Alexeev Igor I. Belenkaya Elena S. Bobrovnikov Sergey Yu. Kalegaev Vladimir V. 《Space Science Reviews》2003,107(1-2):7-26
A magnetohydrodynamic model of the solar wind flow is constructed using a kinematic approach. It is shown that a phenomenological
conductivity of the solar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component
normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the
solar wind electric field. A simple analytical solution for the problem of the solar wind flow past the magnetosphere is presented.
In this approach the magnetopause and the Earth's bow shock are approximated by the paraboloids of revolution. Superposition
of the effects of the bulk solar wind plasma motion and the magnetic field diffusion results in an incomplete screening of
the IMF by the magnetopause. It is shown that the normal to the magnetopause component of the solar wind magnetic field and
the tangential component of the electric field penetrated into the magnetosphere are determined by the quarter square of the
magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe
the magnetosphere in the course of the severe magnetic storm. The conditions under which the magnetospheric magnetic flux
structure is unstable and can drive the magnetospheric substorm are discussed. The model calculations are compared with the
observational data for September 24–26, 1998 magnetic storm (Dst
min=−205 nT) and substorm occurred at 02:30 UT on January 10, 1997.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
975.
为检测某火控系统的性能,采用统计量分析和AR模型预测相结合来对火控系统实时解算的数据进行分析的一种方法。根据分析结果可以看出,距离误差和航向误差是两种不同类型的误差,距离误差主要是由随机的量测误差构成的,而航向误差主要是系统误差。 相似文献
976.
基于联系数系统态势排序的目标威胁综合评估 总被引:2,自引:1,他引:2
董文洪 《海军航空工程学院学报》2005,20(6):681-684
对防空导弹将要拦截的目标进行威胁程度评估,通常是先分析影响目标威胁程度的因素,并赋予各因素权重,计算各因素在某时刻的状态值并规范化,再通过加权求和综合合成; 根据合成结果对多个目标的威胁程度作出排序,求出威胁程度最大的目标。文章阐明了采用以上的加权求和计算有时会失效,指出失效的主要原因来自加权求和模型自身,可改用基于联系数系统态势排序的目标威胁综合评估解决这一问题。 相似文献
977.
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979.
980.