全文获取类型
收费全文 | 3440篇 |
免费 | 311篇 |
国内免费 | 382篇 |
专业分类
测绘学 | 10篇 |
大气科学 | 284篇 |
地球物理 | 1065篇 |
地质学 | 302篇 |
海洋学 | 1056篇 |
天文学 | 692篇 |
综合类 | 61篇 |
自然地理 | 663篇 |
出版年
2024年 | 9篇 |
2023年 | 23篇 |
2022年 | 36篇 |
2021年 | 31篇 |
2020年 | 50篇 |
2019年 | 85篇 |
2018年 | 61篇 |
2017年 | 71篇 |
2016年 | 69篇 |
2015年 | 82篇 |
2014年 | 100篇 |
2013年 | 186篇 |
2012年 | 47篇 |
2011年 | 116篇 |
2010年 | 111篇 |
2009年 | 212篇 |
2008年 | 259篇 |
2007年 | 303篇 |
2006年 | 227篇 |
2005年 | 176篇 |
2004年 | 188篇 |
2003年 | 206篇 |
2002年 | 173篇 |
2001年 | 121篇 |
2000年 | 144篇 |
1999年 | 161篇 |
1998年 | 151篇 |
1997年 | 73篇 |
1996年 | 102篇 |
1995年 | 77篇 |
1994年 | 73篇 |
1993年 | 69篇 |
1992年 | 58篇 |
1991年 | 53篇 |
1990年 | 48篇 |
1989年 | 40篇 |
1988年 | 26篇 |
1987年 | 25篇 |
1986年 | 18篇 |
1985年 | 13篇 |
1984年 | 8篇 |
1983年 | 5篇 |
1982年 | 6篇 |
1981年 | 3篇 |
1980年 | 19篇 |
1979年 | 3篇 |
1978年 | 7篇 |
1977年 | 5篇 |
1954年 | 4篇 |
排序方式: 共有4133条查询结果,搜索用时 78 毫秒
991.
The prompt optical emission of GRB 990123 was uncorrelated to the γ-ray light curve and exhibited temporal properties similar to those of the steeply decaying, early X-ray emission observed by Swift at the end of many bursts. These facts suggest that the optical counterpart of GRB 990123 was the large-angle emission released during (the second pulse of) the burst. If the optical and γ-ray emissions of GRB 990123 have, indeed, the same origin then their properties require that (i) the optical counterpart was synchrotron emission and γ-rays arose from inverse-Compton scatterings (the 'synchrotron self-Compton model'), (ii) the peak energy of the optical-synchrotron component was at ∼20 eV and (iii) the burst emission was produced by a relativistic outflow moving at Lorentz factor ≳450 and at a radius ≳1015 cm, which is comparable to the outflow deceleration radius. Because the spectrum of GRB 990123 was optically thin above 2 keV, the magnetic field behind the shock must have decayed on a length-scale of ≲1 per cent of the thickness of the shocked gas, which corresponds to 106 –107 plasma skin depths. Consistency of the optical counterpart decay rate and its spectral slope (or that of the burst, if they represent different spectral components) with the expectations for the large-angle burst emission represents the most direct test of the unifying picture proposed here for GRB 990123. 相似文献
992.
In this paper we demonstrate application of the Extended Self-Similarity (ESS) concept, recently developed in turbulence physics, for geological and geophysical phenomena. The theoretical background is discussed first and then the ESS properties in fluvial turbulence, sand wave dynamics, Martian topography, river morphometry, gravel-bed mobility, and atmospheric barometric pressure are explored. The main attention is paid to fluvial turbulence and sand waves, while other examples are presented to support the generality of the ESS concept in earth sciences. The results show that the ESS properties of the considered phenomena are remarkably similar to those reported for turbulence, in spite of different underlying mechanisms. This suggests that a general rule should exist which governs a wide class of complex natural phenomena. 相似文献
993.
994.
995.
996.
F. I. González K. Satake E. F. Boss H. O. Mofjeld 《Pure and Applied Geophysics》1995,144(3-4):409-426
The 25 April 1992 Cape Mendocino earthquake generated a tsunami characterized by both coastal trapped edge wave and non-trapped tsunami modes that propagated north and south along the U.S. West Coast. Both observed and synthetic time series at Crescent City and North Spit are consistent with the zero-order edge wave mode solution for a semi-infinite sloping beach depth profile. Wave amplitudes at Crescent City were about twice that observed at North Spit, in spite of the fact that the source region was three times farther from Crescent City than North Spit. The largest observed amplitude was due to an edge wave which arrived almost three hours after the initial onset of the tsunami; since such waves are highly localized nearshore, this suggests that the enhanced responsiveness at Crescent City is at least partly due to local dynamic processes. Furthermore, the substantially delayed arrival of this wave, which was generated at the southern end of the Cascadia Subduction Zone, has significant implications for hazard mitigation efforts along the entire U.S. West Coast. Specifically, this study demonstrates that slow-moving but very energetic edge wave modes could be generated by future large tsunamigenic earthquakes in the CSZ, and that these might arrive unexpectedly at coastal communities several hours after the initial tsunami waves have subsided. 相似文献
997.
Coda site amplification factors are used to eliminate the site effect from records of three circum-PacificT phases recorded by the Hawaiian Volcano Observatory (HVO) network on the island of Hawaii. ObservedT-phase amplitudes across the island generally decrease with increasing distance from the conversion point where acoustic waves
in the SOFAR channel become seismic waves propagating through the crust. However, the decay of the observedT-phase signal across the island is not regular in regions of dense station coverage, in particular, the Kilauea caldera region.
We divide the maximum observedT-phase amplitudes at a given station by the coda site amplification factor obtained for the same station and frequency band
(3.0Hz); the distribution of these amplitudes reveals a smooth pattern over the entire island. The distance over which the
site effect-correctedT-phase amplitude decreases by one-half, combined with the apparent velocity of propagation ofT phases across the island, allows for an approximate determination of near-surfaceQ over much of the island of Hawaii. We found a region of lowQ in the Kilauea summit area (Q≈30) and east rift zone (Q≈60) with considerably higherQ in the Kaoiki and northern portions of the island (Q≈150 to 200). The lowQ values obtained in the Kilauea summit region and east rift zone are significantly lower than estimates of codaQ in the same region, suggestingT phases may be sampling the earth's near-surface properties. 相似文献
998.
999.
NLS EQUATION OF INTERNAL WAVES IN WEAKLY STRATIFIED OCEAN 总被引:1,自引:0,他引:1
The NLS (Non-Linear Schr(?)dinger) equation of internal waves in a wekly stratified ocean is der-ived in phase coordnates in terms of the RPM (Reductive Perturbation Method). It was shown thatwhen AB>0 there exist modulation forms of envelope soliton and dn, and tha when AB<0 there arethree modulation forms dark soliton, sn and cn. Only if K~2>B/A(?) . the side-band perturbation is stable,otherwise unstable. For the stable side-band perturbation there ekisis a modulation form of MdV soliton. 相似文献
1000.