全文获取类型
收费全文 | 840篇 |
免费 | 175篇 |
国内免费 | 251篇 |
专业分类
航空 | 473篇 |
航天技术 | 274篇 |
综合类 | 55篇 |
航天 | 464篇 |
出版年
2024年 | 10篇 |
2023年 | 34篇 |
2022年 | 24篇 |
2021年 | 53篇 |
2020年 | 56篇 |
2019年 | 41篇 |
2018年 | 55篇 |
2017年 | 45篇 |
2016年 | 56篇 |
2015年 | 52篇 |
2014年 | 76篇 |
2013年 | 47篇 |
2012年 | 75篇 |
2011年 | 60篇 |
2010年 | 66篇 |
2009年 | 50篇 |
2008年 | 36篇 |
2007年 | 64篇 |
2006年 | 94篇 |
2005年 | 50篇 |
2004年 | 24篇 |
2003年 | 29篇 |
2002年 | 21篇 |
2001年 | 7篇 |
2000年 | 13篇 |
1999年 | 32篇 |
1998年 | 19篇 |
1997年 | 9篇 |
1996年 | 14篇 |
1995年 | 20篇 |
1994年 | 14篇 |
1993年 | 3篇 |
1992年 | 3篇 |
1991年 | 3篇 |
1990年 | 4篇 |
1989年 | 2篇 |
1987年 | 2篇 |
1986年 | 3篇 |
排序方式: 共有1266条查询结果,搜索用时 15 毫秒
41.
Y. Futaana S. Barabash A. Grigoriev D. Winningham R. Frahm M. Yamauchi R. Lundin 《Space Science Reviews》2006,126(1-4):315-332
As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case
of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board
the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian
exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485
of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed
by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was
most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can
be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation
region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went
out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic
flux variations of the ENA flux at the spacecraft location. 相似文献
42.
43.
44.
45.
轴流风扇/压气机管道周向声模态的测量 总被引:2,自引:1,他引:2
利用管道内部周向均匀分布的麦克风阵列对某单级风扇在高背景噪声和较大硬壁反射条件下的管道周向声模态进行了实验测量.利用与参考信号互相关(CC)模态分解技术和传统的方均根(RMS)模态分解技术得到了主要的周向声模态振幅.通过与Tyler和Sofrin的理论分析对比,发现在高背景噪声和较大硬壁反射条件下,两种模态分解技术都能获得较为理想的模态分解结果;并且发现CC模态分解技术获得的模态振幅较低,初步分析这是由于和RMS模态分解技术相比,CC模态分解技术可以降低随机噪声对模态振幅分解结果的影响.此外,周向麦克风个数大于所要分解周向声模态阶数的4倍时,使用CC模态分解技术获得的模态振幅误差可以控制在1dB之内. 相似文献
46.
为了实现新一代发动机的噪声源识别技术,对于测试所得到的民用飞机发动机的整体噪声数据,通过部件噪声分解方法,将其分解到各个部件,并且认识当代民用飞机发动机噪声源的基本特征.开发出利用发动机整机噪声数据的噪声源识别系统,采用反卷积法将波束成型法的结果作为中间声源,从中获取所需要的声源信息,使得最终的结果更加准确.通过获取的发动机整机噪声数据,验证传声器阵列技术的可行性,并且证明了系统的可行性和有效性. 相似文献
47.
Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for
interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of
electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions
as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory
is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are
bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
48.
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
49.
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
50.