全文获取类型
收费全文 | 257601篇 |
免费 | 5288篇 |
国内免费 | 3326篇 |
专业分类
测绘学 | 6890篇 |
大气科学 | 19119篇 |
地球物理 | 54013篇 |
地质学 | 89540篇 |
海洋学 | 21481篇 |
天文学 | 56180篇 |
综合类 | 1029篇 |
自然地理 | 17963篇 |
出版年
2021年 | 2241篇 |
2020年 | 2608篇 |
2019年 | 2862篇 |
2018年 | 3507篇 |
2017年 | 3269篇 |
2016年 | 5718篇 |
2015年 | 4229篇 |
2014年 | 6947篇 |
2013年 | 14265篇 |
2012年 | 6500篇 |
2011年 | 7839篇 |
2010年 | 6939篇 |
2009年 | 9494篇 |
2008年 | 8332篇 |
2007年 | 7829篇 |
2006年 | 9656篇 |
2005年 | 7692篇 |
2004年 | 7591篇 |
2003年 | 7111篇 |
2002年 | 6690篇 |
2001年 | 5965篇 |
2000年 | 5936篇 |
1999年 | 5199篇 |
1998年 | 5215篇 |
1997年 | 5028篇 |
1996年 | 4664篇 |
1995年 | 4425篇 |
1994年 | 4097篇 |
1993年 | 3831篇 |
1992年 | 3624篇 |
1991年 | 3591篇 |
1990年 | 3754篇 |
1989年 | 3506篇 |
1988年 | 3301篇 |
1987年 | 3844篇 |
1986年 | 3403篇 |
1985年 | 4219篇 |
1984年 | 4734篇 |
1983年 | 4406篇 |
1982年 | 4306篇 |
1981年 | 3915篇 |
1980年 | 3638篇 |
1979年 | 3512篇 |
1978年 | 3481篇 |
1977年 | 3277篇 |
1976年 | 3040篇 |
1975年 | 2962篇 |
1974年 | 2920篇 |
1973年 | 3078篇 |
1972年 | 2024篇 |
排序方式: 共有10000条查询结果,搜索用时 0 毫秒
941.
942.
943.
944.
R. J. Protheroe 《Monthly notices of the Royal Astronomical Society》2003,341(1):230-238
I re-examine the brightness temperature problem in PKS 0405-385, which is an extreme intra-day variable radio quasar with an inferred brightness temperature of ∼5 × 1014 K at 5 GHz, well above the Compton catastrophe limit of ∼1011 K that is reached when the synchrotron photon energy density exceeds the energy density of the magnetic field. If one takes into account the uncertainty in the distance to the ionized clouds responsible for interstellar scintillation causing rapid intra-day variability in PKS 0405-385, it is possible that the brightness temperature could be as low as ∼1013 K at 5 GHz, or even lower. The radio spectrum can be fitted by optically thin emission from mono-energetic electrons, or an electron spectrum with a low-energy cut-off such that the critical frequency of the lowest energy electrons is above the radio frequencies of interest. If one observes optically thin emission along a long narrow emission region, the average energy density in the emission region can be many orders of magnitude lower than calculated from the observed intensity if one assumed a spherical emission region. I discuss the physical conditions in the emission region and find that the Compton catastrophe can then be avoided using a reasonable Doppler factor. I also show that MeV to 100-GeV gamma-ray emission at observable flux levels should be expected from extreme intra-day variable sources such as PKS 0405-385. 相似文献
945.
The proper motions of stars in the main sequence and of luminosity class III giants are analyzed kinematically. A new method has been used for reliably separating all the parameters of the Ogorodnikov-Milne model based on representing the proper motions of the stars in coordinate systems whose poles lie on each of the three principal axes of the galactic trihedron. Solutions for stars in different spectral classes are obtained. The main sequence is found to subdivide into two zones (near and far stars) with a fairly sharp boundary at B-V=0.5. It is shown that the Parenago effect may be related to the different distances from the sun of the main sequence stars. 相似文献
946.
947.
948.
S. Maaløe 《Mineralogy and Petrology》2003,77(1-2):1-24
Summary ?Partial melting of the mantle is polybaric which implies that the phase relations change during partial melting. In addition
to the pressure the composition of the melt depends on the melting mode. Various melting models have been suggested. Here
the basic phase relations of polybaric batch, percolative, and critical melting are considered, using a simple ternary system.
The percolative melts are in equilibrium with their residua, but differ somewhat in composition from those of batch melting.
Critical melting is a fractional type of melting where the residuum contain interstitial melt. The critical melts differ in
composition from batch melts. The linear trends of peridotites from ophiolites show that the extracted melts had nearly constant
compositions, and therefore were extracted within a small pressure interval. A comparison between the trends of mantle peridotite
and experimental batch melts suggests strongly that the melt extracted from the peridotites are in equilibrium with their
residua. This could suggest that either batch or percolative melting are relevant melting modes for the mantle. However, isotopic
disequilibria favor instead a critical mode of melting. This inconsistency can be avoided if the ascending melts are accumulated
within a source region and equilibrate with the residuum before the melt is extracted from the source region. The evidence
for equilibrium suggests that multisaturation of tholeiitic compositions in PT-diagrams is relevant for estimating pressure
and temperature of generation of primary tholeiitic magmas.
Received September 2, 2001; revised version accepted March 20, 2002 相似文献
949.
A new analysis of all 346 published 14C dated Holocene alluvial units in Britain offers a unique insight into the regional impacts of global change and shows how surprisingly sensitive British rivers have been to relatively modest but repeated changes in climate. Fourteen major but probably brief periods of flooding are identified bracketed within the periods 400–1070, 1940–3940, 7520–8100 and at ca. 10 420 cal. yr BP. There is a strong correspondence between climatic deteriorations inferred from mire wet shifts and major periods of flooding, especially at ca. 8000 cal. yr BP and since ca. 4000 cal. yr BP. The unusually long and complete British record also demonstrates that alterations in land cover have resulted in a step change in river basin sensitivity to variations in climate. This has very important implications for assessing and mitigating the impact of increasing severe flooding. In small and medium‐sized river basins land use is likely to play a key role in either moderating or amplifying the climatic signal. Copyright © 2003 John Wiley & Sons, Ltd. 相似文献
950.