全文获取类型
收费全文 | 4717篇 |
免费 | 3篇 |
国内免费 | 9篇 |
专业分类
航空 | 2289篇 |
航天技术 | 1404篇 |
综合类 | 10篇 |
航天 | 1026篇 |
出版年
2021年 | 28篇 |
2018年 | 199篇 |
2017年 | 164篇 |
2016年 | 78篇 |
2015年 | 41篇 |
2014年 | 66篇 |
2013年 | 108篇 |
2012年 | 123篇 |
2011年 | 257篇 |
2010年 | 213篇 |
2009年 | 257篇 |
2008年 | 269篇 |
2007年 | 223篇 |
2006年 | 81篇 |
2005年 | 150篇 |
2004年 | 136篇 |
2003年 | 123篇 |
2002年 | 81篇 |
2001年 | 122篇 |
2000年 | 60篇 |
1999年 | 86篇 |
1998年 | 107篇 |
1997年 | 77篇 |
1996年 | 70篇 |
1995年 | 109篇 |
1994年 | 125篇 |
1993年 | 69篇 |
1992年 | 76篇 |
1991年 | 32篇 |
1990年 | 42篇 |
1989年 | 68篇 |
1988年 | 30篇 |
1987年 | 26篇 |
1986年 | 38篇 |
1985年 | 125篇 |
1984年 | 111篇 |
1983年 | 91篇 |
1982年 | 77篇 |
1981年 | 155篇 |
1980年 | 31篇 |
1979年 | 34篇 |
1978年 | 37篇 |
1977年 | 34篇 |
1976年 | 29篇 |
1975年 | 34篇 |
1974年 | 29篇 |
1973年 | 31篇 |
1972年 | 41篇 |
1971年 | 22篇 |
1970年 | 22篇 |
排序方式: 共有4729条查询结果,搜索用时 15 毫秒
311.
We study the solar cycle, radial, and latitudinal dependence of the characteristics of magnetic field irregularities in the
Heliosphere. The frequency of magnetic field discontinuities is determined, using high time resolution magnetic field observations
by Ulysses, covering the time interval from 1992 to 2000. The quasi-linear scattering mean free path of particles is also calculated.
These investigations aim at understanding/exploring transport properties of energetic charged particles in the Heliosphere.
We find that the travel time of solar wind plasma from the Sun to the observer is the key parameter of the process, by controling
the decay of the irregularities.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
312.
Ergun R.E. Carlson C.W. Mozer F.S. Delory G.T. Temerin M. McFadden J.P. Pankow D. Abiad R. Harvey P. Wilkes R. Primbsch H. Elphic R. Strangeway R. Pfaff R. Cattell C.A. 《Space Science Reviews》2001,98(1-2):67-91
We describe the electric field sensors and electric and magnetic field signal processing on the FAST (Fast Auroral SnapshoT) satellite. The FAST satellite was designed to make high time resolution observations of particles and electromagnetic fields in the auroral zone to study small-scale plasma interactions in the auroral acceleration region. The DC and AC electric fields are measured with three-axis dipole antennas with 56 m, 8 m, and 5 m baselines. A three-axis flux-gate magnetometer measures the DC magnetic field and a three-axis search coil measures the AC magnetic field. A central signal processing system receives all signals from the electric and magnetic field sensors. Spectral coverage is from DC to 4 MHz. There are several types of processed data. Survey data are continuous over the auroral zone and have full-orbit coverage for fluxgate magnetometer data. Burst data include a few minutes of a selected region of the auroral zone at the highest time resolution. A subset of the burst data, high speed burst memory data, are waveform data at 2×106 sample s–1. Electric field and magnetic field data are primarily waveforms and power spectral density as a function of frequency and time. There are also various types of focused data processing, including cross-spectral analysis, fine-frequency plasma wave tracking, high-frequency polarity measurement, and wave-particle correlations. 相似文献
313.
von Steiger R. Zurbuchen T.H. Geiss J. Gloeckler G. Fisk L.A. Schwadron N.A. 《Space Science Reviews》2001,97(1-4):123-127
The source region of solar wind plasma is observed to be directly reflected in the compositional pattern of both elemental
and charge state compositions. Slow solar wind associated with streamers shows higher freeze-in temperatures and larger FIP
enhancements than coronal hole associated wind. Also, the variability of virtually all compositional parameters is much higher
for slow solar wind compared to coronal hole associated wind. We show that these compositional patterns persist even though
stream-stream interactions complicate the identification based on in situ plasma parameters.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
314.
气固紊流剪切流中颗粒弥散的拉格朗日模拟 总被引:1,自引:0,他引:1
本文提出了一种对于气固两相紊流剪切流中圆形固体颗粒弥散的拉格朗日拟计算方法,其中考虑了颗粒间的磁撞对流体相和颗料相的影响,应用该方法对一气固紊流剪切流场进行了模拟计算,并对有、无颗粒间磁撞情况下的模拟计算结果与Lavieville用大涡模拟方法的研究结果进行了比较,并进行了讨论。 相似文献
315.
316.
317.
L. Ofman M. Romoli G. Noci G. Poletto J. L. Kohl R. A. Howard C. St. Cyr C. E. Deforest 《Space Science Reviews》1999,87(1-2):287-290
In recent UVCS/SOHO White Light Channel (WLC) observations we found quasi-periodic variations in the polarized brightness
(pB) in the polar coronal holes at heliocentric distances of 1.9 to 2.45 solar radii. The motivation for the observation is
the 2.5D MHD model of solar wind acceleration by nonlinear waves, that predicts compressive fluctuations in coronal holes.
In February 1998 we performed new observations using the UVCS/WLC in the coronal hole and obtained additional data. The new
data corroborate our earlier findings with higher statistical significance. The new longer observations show that the power
spectrum peaks in the 10–12 minute range. These timescales agree with EIT observations of brightness fluctuations in polar
plumes. We performed preliminary LASCO/C2 observations in an effort to further establish the coronal origin of the fluctuations.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
318.
319.
The problem treated here is the analysis of a class of nonlinear sampled-data systems with a Gaussian input signal. The nonlinear element is a symmetrical limiter (memoryless device) that feeds the linear element. Preceding the limiter is a sampler and zero-order hold unit for data reconstruction. The analysis is predicated on finding an equivalent gain for the nonlinear element such that the mean-square error is a minimum. The nonlinearity is thus replaced by a linear component and the system is then analyzed by conventional techniques. It is also shown that for appropriate sampling rates the sampled-data system is equivalent to a continuous system due to the action of the sampler-hold combination. All calculations pertaining to the limiter input signal require the use of a transfer function that is interior to the feedback loop. However, in developing this transfer function, the overall system is considered so that the system output may be evaluated after the value of equivalent gain has been found. 相似文献
320.