全文获取类型
收费全文 | 762篇 |
免费 | 135篇 |
国内免费 | 151篇 |
专业分类
航空 | 402篇 |
航天技术 | 248篇 |
综合类 | 76篇 |
航天 | 322篇 |
出版年
2024年 | 7篇 |
2023年 | 19篇 |
2022年 | 18篇 |
2021年 | 31篇 |
2020年 | 41篇 |
2019年 | 29篇 |
2018年 | 44篇 |
2017年 | 37篇 |
2016年 | 41篇 |
2015年 | 32篇 |
2014年 | 68篇 |
2013年 | 45篇 |
2012年 | 65篇 |
2011年 | 46篇 |
2010年 | 47篇 |
2009年 | 28篇 |
2008年 | 48篇 |
2007年 | 46篇 |
2006年 | 86篇 |
2005年 | 42篇 |
2004年 | 25篇 |
2003年 | 32篇 |
2002年 | 22篇 |
2001年 | 3篇 |
2000年 | 16篇 |
1999年 | 27篇 |
1998年 | 18篇 |
1997年 | 11篇 |
1996年 | 11篇 |
1995年 | 25篇 |
1994年 | 14篇 |
1993年 | 5篇 |
1992年 | 5篇 |
1991年 | 2篇 |
1990年 | 4篇 |
1989年 | 4篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1986年 | 2篇 |
排序方式: 共有1048条查询结果,搜索用时 296 毫秒
461.
We discuss quasi-static and dynamic models of the magnetotail response to perturbations imposed by the solar wind, focusing
particularly on the formation of thin current sheets, their structure and breakup. 相似文献
462.
Steven R. Spangler 《Space Science Reviews》2005,121(1-4):189-200
I discuss a method for determining the strength and spatial structure of the coronal magnetic field by observations of the
Faraday rotation of a radio galaxy which is in conjunction with the Sun. Given a knowledge of the plasma density in the outer
corona, and the magnetic field sector structure (both independently available), the strength of the coronal field can be determined,
as well as the magnitude of spatial variations on scales of 1000 km to several solar radii. Such knowledge is crucial for
testing computational models of the solar corona, which are prominently featured in this meeting. Results are presented from
observations with the Very Large Array radio telescope of the radio galaxy 3C228 on August 16, 2003, when the line of sight
to the source was at heliocentic distances of 7.1−6.2R
⊙. The observations are consistent with a coronal magnetic field which is proportional to the inverse square of the distance
in the range 6 ≤ r ≤ 10R
⊙, and has a value of 39 mG at 6.2R
⊙. The Faraday rotation is uniform across the source, indicating an absence of strong plasma inhomogeneity on spatial scales
up to 35,000 km. 相似文献
463.
根据北斗一号卫星天线在轨的实际飞行温度,反推出了SR107-ZK白漆的太阳吸收比αs退化曲线,并根据该曲线外推,得到了8年寿命末期的太阳吸收比αs,预测了卫星寿命末期天线反射面的最高温度。 相似文献
464.
465.
466.
R. A. Mewaldt 《Space Science Reviews》2006,124(1-4):303-316
Recent progress in measuring the composition and energy spectra of solar energetic particles (SEPs) accelerated by CME-driven
shocks is reviewed, including a comparison of the observed charge-to-mass dependence of breaks in SEP spectra with model predictions.
Also discussed is a comparison of SEP and CME kinetic energies in seventeen large SEP events, and estimates of the SEP radiation
dose that astronauts would be subject to once they venture outside the protective cover of Earth’s magnetosphere. 相似文献
467.
G. P. Chernov 《Space Science Reviews》2006,127(1-4):195-326
This review covers fairly comprehensively experimental and theoretical research on the fine structure of types zebra pattern
(ZP) and fiber bursts (FB) in solar type II + IV radio bursts. The basic attention is given to the latest experimental data.
A comparative analysis of several recent solar type IV radio outbursts with these fine structure in dynamical radio spectra
is carried out using available ground-based and satellite data (Yohkoh, SOHO, TRACE, RHESSI). New data on microwave zebra
structures and fiber bursts testifies that they are analogous to similar structures observed at meter wavelengths. The discovery
of the superfine structure, in the form of millisecond spikes is the most significant new effect in the cm range. All basic
theoretical models of the zebra pattern and fiber bursts are discussed critically. Two main models are studied for their interpretation:
(i) interactions between electrostatic plasma waves and whistlers, (ii) radio emission at double plasma resonance (DPR). The
relative significance of several possible mechanisms remains uncertain. 相似文献
468.
We present a preliminary analysis of two quiet Sun transition region areas observed with the SOHO/SUMER spectrometer, using
lines from oxygen, nitrogen and silicon. The average quiet Sun physical parameters are studied as a function of line intensity.
Systematic variations of line position and width with increasing intensity are found. A large number of small-scale active
points have been observed, and preliminary analysis of the physical properties and dynamics of these active features is presented.
A jet-like structure, found in an active point, is also investigated and its velocity along the line of sight determined.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
469.
Brian E. Wood 《Space Science Reviews》2006,126(1-4):3-14
Exposure to the solar wind can have significant long term consequences for planetary atmospheres, especially for planets such
as Mars that are not protected by global magnetospheres. Estimating the effects of solar wind exposure requires knowledge
of the history of the solar wind. Much of what we know about the Sun’s past behavior is based on inferences from observations
of young solar-like stars. Stellar analogs of the weak solar wind cannot be detected directly, but the interaction regions
between these winds and the interstellar medium have been detected and used to estimate wind properties. I here review these
observations, with emphasis on what they suggest about the history of the solar wind. 相似文献
470.
The Ulysses spacecraft has been the first to orbit the Sun over its poles and to explore the heliosphere at these high heliolatitudes.
It has now completed two fast latitude scans, one at solar minimum and one at solar maximum. Since its launch in October 1990,
this mission has led to several surprising discoveries concerning energetic particles, cosmic rays, Jovian electrons, the
solar wind, the heliospheric magnetic field and the global features of the heliosphere. This review addresses mainly the propagation
and modulation of cosmic rays and other charged particles, from both an observational and theoretical point of view, with
emphasis on what has been learned from exploring the inner heliosphere to high heliolatitudes. This is done for solar minimum
and maximum conditions. The review is concluded with a summary of the main scientific discoveries and insights gained so far
from the Ulysses mission. 相似文献