全文获取类型
| 收费全文 | 595篇 |
| 免费 | 77篇 |
| 国内免费 | 71篇 |
专业分类
| 测绘学 | 57篇 |
| 大气科学 | 58篇 |
| 地球物理 | 88篇 |
| 地质学 | 180篇 |
| 海洋学 | 49篇 |
| 天文学 | 256篇 |
| 综合类 | 33篇 |
| 自然地理 | 22篇 |
出版年
| 2024年 | 1篇 |
| 2023年 | 4篇 |
| 2022年 | 5篇 |
| 2021年 | 2篇 |
| 2020年 | 11篇 |
| 2019年 | 20篇 |
| 2018年 | 9篇 |
| 2017年 | 9篇 |
| 2016年 | 16篇 |
| 2015年 | 24篇 |
| 2014年 | 23篇 |
| 2013年 | 26篇 |
| 2012年 | 29篇 |
| 2011年 | 19篇 |
| 2010年 | 24篇 |
| 2009年 | 51篇 |
| 2008年 | 52篇 |
| 2007年 | 51篇 |
| 2006年 | 50篇 |
| 2005年 | 49篇 |
| 2004年 | 42篇 |
| 2003年 | 42篇 |
| 2002年 | 34篇 |
| 2001年 | 20篇 |
| 2000年 | 17篇 |
| 1999年 | 11篇 |
| 1998年 | 8篇 |
| 1997年 | 12篇 |
| 1996年 | 10篇 |
| 1995年 | 15篇 |
| 1994年 | 11篇 |
| 1993年 | 11篇 |
| 1992年 | 5篇 |
| 1991年 | 8篇 |
| 1990年 | 9篇 |
| 1989年 | 2篇 |
| 1988年 | 1篇 |
| 1987年 | 2篇 |
| 1986年 | 2篇 |
| 1985年 | 2篇 |
| 1984年 | 1篇 |
| 1982年 | 1篇 |
| 1981年 | 1篇 |
| 1980年 | 1篇 |
排序方式： 共有743条查询结果，搜索用时 15 毫秒
1.
2.
3.
M. Sereno 《Monthly notices of the Royal Astronomical Society》2005,356(3):937-943
Constraints on an exact quintessence scalar-field model with an exponential potential are derived from gravitational lens statistics. An exponential potential can account for data from both optical quasar surveys and radio-selected sources. Based on the Cosmic Lens All-Sky Survey (CLASS) sample, lensing statistics provides, for the pressureless matter density parameter, an estimate of ΩM0 = 0.31+0.12 −0.14 . 相似文献
4.
5.
6.
S. W. Allen R. W. Schmidt A. C. Fabian 《Monthly notices of the Royal Astronomical Society》2002,334(2):L11-L15
We present precise measurements of the X-ray gas mass fraction for a sample of luminous, relatively relaxed clusters of galaxies observed with the Chandra observatory, for which independent confirmation of the mass results is available from gravitational lensing studies. Parametrizing the total (luminous plus dark matter) mass profiles using the model of Navarro, Frenk & White, we show that the X-ray gas mass fractions in the clusters asymptote towards an approximately constant value at a radius r 2500 , where the mean interior density is 2500 times the critical density of the Universe at the redshifts of the clusters. Combining the Chandra results on the X-ray gas mass fraction and its apparent redshift dependence with recent measurements of the mean baryonic matter density in the Universe and the Hubble constant determined from the Hubble Key Project, we obtain a tight constraint on the mean total matter density of the Universe, , and measure a positive cosmological constant, . Our results are in good agreement with recent, independent findings based on analyses of anisotropies in the cosmic microwave background radiation, the properties of distant supernovae, and the large-scale distribution of galaxies. 相似文献
7.
Dark energy has a dramatic effect on the dynamics of the Universe, causing the recently discovered acceleration of the expansion. The dynamics are also central to the behaviour of the growth of large-scale structure, offering the possibility that observations of structure formation provide a sensitive probe of the cosmology and dark energy characteristics. In particular, dark energy with a time-varying equation of state can have an influence on structure formation stretching back well into the matter-dominated epoch. We analyse this impact, first calculating the linear perturbation results, including those for weak gravitational lensing. These dynamical models possess definite observable differences from constant equation of state models. Then we present a large-scale numerical simulation of structure formation, including the largest volume to date involving a time-varying equation of state. We find the halo mass function is well described by the Jenkins et al. mass function formula. We also show how to interpret modifications of the Friedmann equation in terms of a time-variable equation of state. The results presented here provide steps toward realistic computation of the effect of dark energy in cosmological probes involving large-scale structure, such as cluster counts, the Sunyaev–Zel'dovich effect or weak gravitational lensing. 相似文献
8.
S.W. Allen 《Astrophysics and Space Science》2003,285(1):247-256
Chandra X-ray observations of rich, dynamically relaxed galaxy clusters allow the properties of the X-ray gas and the total
gravitating mass to be determined precisely. Here, we discuss how Chandra observations may be used as a powerful tool for
cosmological studies. By combining Chandra X-ray results on the X-ray gas mass fractions in clusters with independent measurements
of the Hubble constant and the mean baryonic matter density of the universe, we obtain a tight constraint on the mean total
matter density of the universe, Οm, and an interesting constraint on the cosmological constant, ΟΛ. Using these results, together with the observed local X-ray luminosity function of the most X-ray luminous galaxy clusters,
a mass-luminosity relation determined from Chandra and ROSAT X-ray data and weak gravitational lensing observations, and the
mass function predicted by numerical simulations, we obtain a precise constraint on the normalization of the power spectrum
of density fluctuations in the nearby universe,σ8. We compare our results with those obtained from other, independent methods.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
9.
GYD-300型全液压动力头工程钻机为全液压驱动,动力头反循环式机型。液压系统采用插装阀集成结构,电液复合操作。使用PC控制监测系统,适时检测孔底各相关压力,对不同地层进行范围设置,实现钻进过程中孔底的自动、手动恒压钻进。重点介绍了该钻机的结构特点、实验情况、主要技术参数等。 相似文献
10.
根据2000年6月10～14日在浙江省西沪港采集的海水样品,利用AA-800石墨炉原子吸收分光光度技术和阳极溶出伏安法测定样品中重金属铜的含量,获得铜在海水中受不同的有机配体控制.不同粒级的铜表观配位容量表明西沪港海水过孔径1.00μm微孔膜的(ACuCC)较高,为144.4nmol/dm3;过0.40和0.20μm滤膜的(ACuCC)分别为103.0和102nmol/dm3;铜的有机配体条件稳定常数的对数值在7.25～9.14之间.铜的总量为21.72nmol/dm3.铜全部为稳定溶解态,其中pH2酸溶态占95.0%,强有机结合态占5.0%.溶解态铜中有机结合态占过滤海水中总铜的61.6%. 相似文献