全文获取类型
收费全文 | 33838篇 |
免费 | 2867篇 |
国内免费 | 4764篇 |
专业分类
测绘学 | 2546篇 |
大气科学 | 3132篇 |
地球物理 | 3813篇 |
地质学 | 8068篇 |
海洋学 | 3121篇 |
天文学 | 17067篇 |
综合类 | 1388篇 |
自然地理 | 2334篇 |
出版年
2024年 | 158篇 |
2023年 | 349篇 |
2022年 | 662篇 |
2021年 | 678篇 |
2020年 | 852篇 |
2019年 | 1012篇 |
2018年 | 709篇 |
2017年 | 826篇 |
2016年 | 827篇 |
2015年 | 1031篇 |
2014年 | 993篇 |
2013年 | 1158篇 |
2012年 | 1158篇 |
2011年 | 1127篇 |
2010年 | 1007篇 |
2009年 | 2418篇 |
2008年 | 2455篇 |
2007年 | 2844篇 |
2006年 | 2858篇 |
2005年 | 2558篇 |
2004年 | 2509篇 |
2003年 | 2126篇 |
2002年 | 1887篇 |
2001年 | 1597篇 |
2000年 | 1506篇 |
1999年 | 1407篇 |
1998年 | 1476篇 |
1997年 | 521篇 |
1996年 | 353篇 |
1995年 | 447篇 |
1994年 | 448篇 |
1993年 | 286篇 |
1992年 | 210篇 |
1991年 | 173篇 |
1990年 | 124篇 |
1989年 | 196篇 |
1988年 | 119篇 |
1987年 | 110篇 |
1986年 | 96篇 |
1985年 | 53篇 |
1984年 | 39篇 |
1983年 | 28篇 |
1982年 | 10篇 |
1981年 | 5篇 |
1980年 | 10篇 |
1979年 | 5篇 |
1977年 | 8篇 |
1954年 | 4篇 |
1897年 | 7篇 |
1877年 | 3篇 |
排序方式: 共有10000条查询结果,搜索用时 16 毫秒
41.
42.
43.
The stability and evolution of cold, shock-bounded slabs is studied using numerical hydrodynamic simulations. We confirm the analysis of Vishniac (1994) [ApJ, 428, 186], who showed that such slabs are unstable if they are perturbed by a displacement larger than their width. The growth rate of this nonlinear thin shell instability (NTSI) is found to increase with decreasing wavelength, in qualitative agreement with Vishniac's analysis. The NTSI saturates when the bending angle becomes large and the growth in the width of the slab pinches off the perturbation. After saturation, the slab remains greatly extended with an average density much less than the original slab density, supported primarily by supersonic turbulence within the slab. Linear perturbations are also found to be unstable in that they can lead to turbulent flow within the slab, although this response to linear perturbations is distinct from, and much less violent than the NTSI.Richard McCray 相似文献
44.
Column density profiles for CN, C3, C2 and NH have been determined from a long-slit CCD spectrum of periodic comet P/Schaumasse (1992x). Comparisons of these profiles with Haser models indicate that the ratios of the CN, C3 and C2 production rates are typical for a short-period comet. Although the scale lengths for NH and its parent species are uncertain, the results indicate that the production rate for NH is much greater than for either C2 or CN. 相似文献
45.
46.
47.
A highly automated moving object detection package 总被引:1,自引:0,他引:1
48.
49.
Cygnus A was the first hyper-active galaxy discovered, and it
remains by far the closest of the ultra-luminous radio galaxies. As
such, Cygnus A has played a fundamental role in the study of virtually
all aspects of extreme activity in galaxies. We present a review of jet
theory for powering the double-lobed radio emitting structures in
powerful radio galaxies, followed by a review of observations of Cygnus
A in the radio, optical, and X-ray relevant to testing various aspects
of jet theory. Issues addressed include: jet structure from pc- to
kpc-scales, jet stability, confinement, composition, and velocity, the
double shock structure for the jet terminus and the origin of multiple
radio hotspots, the nature of the filamentary structure in the radio
lobes, and the hydrodynamic evolution of the radio lobes within a dense
cluster atmosphere, including an analysis of pressure balance between
the various gaseous components. Also discussed are relativistic
particle acceleration and loss mechanisms in Cygnus A, as well as
magnetic field strengths and geometries both within the radio source,
and in the intracluster medium. We subsequently review the
classification, cluster membership, and the emission components of the
Cygnus A galaxy. The origin of the activity is discussed.
Concentrating on the nuclear regions of the galaxy, we review the
evidence for an obscured QSO, also given the constraints on the
orientation of the radio source axis with respect to the sky plane. We
present an overview of models of central engines in AGN and observations
of Cygnus A which may be relevant to testing such models. We conclude
with a brief section concerning the question of whether Cygnus A is
representative of powerful high redshift radio galaxies.
Received October 10, 1995 相似文献