全文获取类型
收费全文 | 20242篇 |
免费 | 2216篇 |
国内免费 | 2932篇 |
专业分类
测绘学 | 770篇 |
大气科学 | 973篇 |
地球物理 | 1728篇 |
地质学 | 6332篇 |
海洋学 | 5531篇 |
天文学 | 5108篇 |
综合类 | 990篇 |
自然地理 | 3958篇 |
出版年
2024年 | 85篇 |
2023年 | 258篇 |
2022年 | 622篇 |
2021年 | 631篇 |
2020年 | 706篇 |
2019年 | 793篇 |
2018年 | 600篇 |
2017年 | 725篇 |
2016年 | 723篇 |
2015年 | 718篇 |
2014年 | 1147篇 |
2013年 | 1101篇 |
2012年 | 1124篇 |
2011年 | 1382篇 |
2010年 | 1258篇 |
2009年 | 1636篇 |
2008年 | 1516篇 |
2007年 | 1488篇 |
2006年 | 1347篇 |
2005年 | 1199篇 |
2004年 | 995篇 |
2003年 | 873篇 |
2002年 | 785篇 |
2001年 | 650篇 |
2000年 | 615篇 |
1999年 | 548篇 |
1998年 | 400篇 |
1997年 | 228篇 |
1996年 | 184篇 |
1995年 | 169篇 |
1994年 | 152篇 |
1993年 | 159篇 |
1992年 | 89篇 |
1991年 | 79篇 |
1990年 | 66篇 |
1989年 | 63篇 |
1988年 | 48篇 |
1987年 | 20篇 |
1986年 | 31篇 |
1985年 | 37篇 |
1984年 | 36篇 |
1983年 | 30篇 |
1982年 | 24篇 |
1981年 | 7篇 |
1980年 | 11篇 |
1979年 | 3篇 |
1978年 | 6篇 |
1977年 | 15篇 |
1954年 | 2篇 |
1875年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
1.
《Sedimentology》2018,65(6):2055-2087
This study, conducted in the Catalan Coastal Ranges, north‐east Spain, describes the Upper Devonian Kellwasser event in a shallowing‐upward sequence of black shales, siltstones and quartz arenites. This sequence was deposited in a progradational and regressive coastal system where the sedimentary environment evolved from the inner shelf to a lagoonal pond located landward of the shoreline. Three anomalous succeeding steps have been identified by geochemical analysis. The first one, detected on the inner shelf, was characterized by oxygen depletion and high organic productivity. The second, detected in the nearshore, was caused by hydrothermal activity occurring under normal oxic conditions. The third and most intense step was identified in the muds of the lagoonal pond and has been linked to strong anoxic conditions, elevated clastic input derived from changes in the weathering regime at the source area and moderate hydrothermal activity. The Kellwasser event is thus defined in the study area as stepwise and multi‐causal. This is the first time that the Kellwasser event has been identified in a sedimentary environment behind the shoreline. It is also the first time that it has been reported in the Catalan Coastal Ranges. 相似文献
2.
《Astroparticle Physics》2002,16(4):183-386
Frequency distributions of local muon densities in high-energy extensive air showers (EAS) are presented as signature of the primary cosmic ray energy spectrum in the knee region. Together with the gross shower variables like shower core position, angle of incidence, and the shower sizes, the KASCADE experiment is able to measure local muon densities for two different muon energy thresholds. The spectra have been reconstructed for various core distances, as well as for particular subsamples, classified on the basis of the shower size ratio Nμ/Ne. The measured density spectra of the total sample exhibit clear kinks reflecting the knee of the primary energy spectrum. While relatively sharp changes of the slopes are observed in the spectrum of EAS with small values of the shower size ratio, no such feature is detected at EAS of large Nμ/Ne ratio in the energy range of 1–10 PeV. Comparing the spectra for various thresholds and core distances with detailed Monte Carlo simulations the validity of EAS simulations is discussed. 相似文献
3.
4.
5.
6.
7.
The kinetics of the reactions of C2H radical with ethane (k1), propane (k2), and n-butane (k3) are studied over the temperature range of T = 96-296 K with a pulsed Laval nozzle apparatus that utilizes a pulsed laser photolysis-chemiluminescence technique. The C2H decay profiles in the presence of both the alkane reactant and O2 are monitored by the CH(A2Δ) chemiluminescence tracer method. The results, together with available literature data, yield the following Arrhenius expressions: k1(T) = (0.51 ± 0.06) × 10−10 exp[(−76 ± 30)K/T] cm3 molecule−1 s−1 (T = 96-800 K), k2(T) = (0.98 ± 0.32) × 10−10exp[(−71 ± 60)K/T] cm3 molecule−1 s−1 (T = 96-361 K), and k3(T) = (1.23 ± 0.26) × 10−10 cm3 molecule−1 s−1 (T = 96-297 K). At T = 296 K, k1 is measured as a function of total pressure and has little or no pressure dependence. The results from this work support a direct hydrogen abstraction mechanism for the title reactions. Implications to the atmospheric chemistry of Titan are discussed. 相似文献
8.
Mars Global Surveyor accelerometer observations of the martian upper atmosphere revealed large variations in density with longitude during northern hemisphere spring at altitudes of 130-160 km, all latitudes, and mid-afternoon local solar times (LSTs). This zonal structure is due to tides from the surface. The zonal structure is stable on timescales of weeks, decays with increasing altitude above 130 km, and is dominated by wave-3 (average amplitude 22% of mean density) and wave-2 (18%) harmonics. The phases of these harmonics are constant with both altitude and latitude, though their amplitudes change significantly with latitude. Near the South Pole, the phase of the wave-2 harmonic changes by 90° with a change of half a martian solar day while the wave-3 phase stays constant, suggesting diurnal and semidiurnal behaviour, respectively. We use a simple application of classical tidal theory to identify the dominant tidal modes and obtain results consistent with those of General Circulation Models. Our method is less rigorous, but simpler, than the General Circulation Models and hence complements them. Topography has a strong influence on the zonal structure. 相似文献
9.
10.