全文获取类型
收费全文 | 753篇 |
免费 | 125篇 |
国内免费 | 213篇 |
专业分类
测绘学 | 57篇 |
大气科学 | 181篇 |
地球物理 | 221篇 |
地质学 | 326篇 |
海洋学 | 103篇 |
天文学 | 36篇 |
综合类 | 59篇 |
自然地理 | 108篇 |
出版年
2024年 | 1篇 |
2023年 | 8篇 |
2022年 | 33篇 |
2021年 | 37篇 |
2020年 | 32篇 |
2019年 | 33篇 |
2018年 | 41篇 |
2017年 | 45篇 |
2016年 | 48篇 |
2015年 | 45篇 |
2014年 | 60篇 |
2013年 | 54篇 |
2012年 | 60篇 |
2011年 | 50篇 |
2010年 | 40篇 |
2009年 | 40篇 |
2008年 | 39篇 |
2007年 | 32篇 |
2006年 | 35篇 |
2005年 | 24篇 |
2004年 | 22篇 |
2003年 | 23篇 |
2002年 | 26篇 |
2001年 | 20篇 |
2000年 | 40篇 |
1999年 | 35篇 |
1998年 | 26篇 |
1997年 | 17篇 |
1996年 | 16篇 |
1995年 | 15篇 |
1994年 | 20篇 |
1993年 | 7篇 |
1992年 | 6篇 |
1991年 | 9篇 |
1990年 | 15篇 |
1989年 | 8篇 |
1988年 | 8篇 |
1987年 | 2篇 |
1986年 | 3篇 |
1985年 | 1篇 |
1983年 | 1篇 |
1982年 | 1篇 |
1980年 | 4篇 |
1979年 | 2篇 |
1978年 | 1篇 |
1976年 | 1篇 |
1975年 | 2篇 |
1974年 | 1篇 |
1973年 | 1篇 |
1969年 | 1篇 |
排序方式: 共有1091条查询结果,搜索用时 250 毫秒
101.
Yang Yunpeng Chen Guan Meng Xingmin Bian Shiqiang Chong Yan Shi Wei Jiang Wanyu Jin Jiacheng Li Chen Mu Xinliang Yue Dongxia 《Landslides》2022,19(4):789-808
Landslides - Determining the premonitory and dynamic characteristics of landslide dam failures can provide an early warning as well the identification of the evolution of the failure process, and... 相似文献
102.
沉积盆地与近断层地震共同作用会增加地震破坏的风险水平,尤其是盆地下方直下型断层发震情况。采用动力学震源模型刻画断层破裂发震过程,开展沉积盆地直下型断层谱元法地震动模拟研究,探讨不同断层面初始剪应力和成核区位置下三维沉积盆地地表响应规律。研究结果表明,断层面应力降对盆地地表地震动的影响显著,在断层面强度一定的情况下,随着初始剪应力的增大,即应力降增大,盆地地表峰值响应增大,原因在于应力降的改变影响了断层破裂释放能量,进而引起断层破裂速度改变,最终导致盆地地表响应发生变化;改变断层面成核区位置会对盆地内部地震动分布规律产生影响,当成核区位置从断层中间向断层左侧移动时,盆地左侧地震动逐渐减小,而右侧地震动逐渐增大,最终表现为盆地右侧地震动显著高于盆地左侧,原因在于改变成核区位置后,导致近断层地震动的方向性效应发生变化。 相似文献
103.
104.
本文总结了近年来条件非线性最优扰动方法的应用研究的主要进展.主要包括四个方面:(1)将条件非线性最优扰动(CNOP)方法拓展到既考虑初始扰动又考虑模式参数扰动,形成了拓展的CNOP方法.拓展的CNOP方法不仅能够应用于研究分别由初始误差和模式参数误差导致的可预报性问题,而且能够用于探讨初始误差和模式参数误差同时存在的情形;(2)将拓展的CNOP方法分别应用于ENSO和黑潮可预报性研究,考察了初始误差和模式参数误差对其可预报性的影响,揭示了初始误差在导致ENSO和黑潮大弯曲路径预报不确定性中的重要作用;(3)考察了阻塞事件发生的最优前期征兆(OPR)以及导致其预报不确定性的最优增长初始误差(OGR),揭示了OPR和OGR空间模态及其演变机制的相似性及其局地性特征;(4)研究了台风预报的目标观测问题,用CNOP方法确定了台风预报的目标观测敏感区,通过观测系统模拟试验(OSSEs)和/或观测系统试验(OSEs),表明了CNOP敏感区在改进台风预报中的有效性.具体地,台风OGR的主要误差分布在某一特定区域,空间分布具有明显的局地性特征,在台风OGR的局地性区域增加观测,有效改进了台风的预报技巧,该区域代表了台风预报的初值敏感区.事实上,上述El Ni(n)o事件、黑潮路径变异以及阻塞事件的OGR的空间分布也具有明显的局地性特征,这些事件的OGR刻画的局地性区域可能也代表了初值敏感区. 相似文献
105.
José I. Muñoz 《Climate Policy》2013,13(2):87-105
How does financial performance risk affect investments in low-carbon electricity-generating technologies to achieve climate policy targets? A detailed risk simulation of price formation in the Great Britain wholesale power market is used to show that the increasing replacement of fossil facilities with wind, ceteris paribus, may cause a deterioration of the financial risk–return performance metrics for incremental investments. Low-carbon investments appear to be high risk, low return, and as such may require a progressively higher level of support over time than envisaged by the conventional degression trajectories. The increasing riskiness of the wholesale market will to some extent offset the benefits of lower capital costs and operational efficiencies if investors need to satisfy cautious debt coverage ratios alongside positive expected returns. This increased risk is additional to the well-known ‘merit order effect’ of low-carbon investments progressively depressing wholesale prices and hence their expected investment returns. Policy relevance Policy support for renewable technologies such as wind is usually based upon levelized costs and is expected to reduce over time as capital costs and operational efficiencies improve. However, levelized costs do not take full account of the risk aversion that investors may have in practice. Expected policy support reductions may be moderated to some extent by the increased financial performance risk that intermittent technologies bring to the power market. The annual risk-return profiles for incremental investments deteriorate for all technologies as wind replaces fossil fuels. This extra risk premium will need to be incorporated into evaluating policy incentives for new investments in a decarbonizing power market. 相似文献
106.
107.
Fen-Fei Wang Jian-Jun Liu Chun-Lai Li Xin Ren Ling-Li Mu Wei Yan Wen-Rui Wang Jing-Tao Xiao Xu Tan Xiao-Xia Zhang Xiao-Duan Zou Xing-Ye Gao 《中国天文和天体物理学报》2014,(12)
The establishment of a lunar control network is one of the core tasks in selenodesy, in which defining an absolute control point on the Moon is the most important step. However, up to now, the number of absolute control points has been very sparse. These absolute control points have mainly been lunar laser ranging retroreflectors, whose geographical location can be observed by observations on Earth and also identified in high resolution lunar satellite images. The Chang'e-3(CE-3) probe successfully landed on the Moon, and its geographical location has been monitored by an observing station on Earth. Since its positional accuracy is expected to reach the meter level, the CE-3 landing site can become a new high precision absolute control point. We use a sequence of images taken from the landing camera, as well as satellite images taken by CE-1 and CE-2, to identify the location of the CE-3 lander. With its geographical location known, the CE-3 landing site can be established as a new absolute control point, which will effectively expand the current area of the lunar absolute control network by 22%, and can greatly facilitate future research in the field of lunar surveying and mapping, as well as selenodesy. 相似文献
108.
109.
110.
Nicheng?ShiEmail author Zhesheng?Ma Ming?Xiong Mingquan?Dai Wenji?Bai Qingsong?Fang Binggang?Yan Jingsui?Yang 《中国科学D辑(英文版)》2005,48(3):338-345
(Fe4Cr4Ni)9C4 is a metal carbide mineral formed by combination of Fe, Cr and Ni with C. It occurs in a chromite deposit in
the Luobusha ophiolite, Tibet. Based on the determination of its crystal structure, the empirical formula is (Fe4.12Cr3.84Ni0.96)8.92C3.70
and the simplified formula is (Fe4Cr4Ni)4C9. The mineral is hexagonal with a = 1.38392(2) nm, c = 0.44690(9) nm, pace group P63 m c, Z=6 and the calculated specific gravity Dx = 7.089 g/cm3. Fe, Cr and Ni occupy different crystallographic sites and their coordination numbers are approximately 12,
forming an alternate stacking sequence of flat and puckered layers along the c axis. Some metallic atoms have a defect structure. The interatomic distances of Fe, Cr and Ni are 0.2525-0.2666 nm, and the
distances between Fe, Cr, Ni and C are 0.1893-0.2169 nm. The coordination number of carbon is 6. It occurs in interstices
of the metallic atoms Fe, Cr and Ni to form trigonalprismatically coordinated polyhedra. These coordination polyhedra are
linked with each other via shared corners or shared edges into a new type of metal carbide structure. 相似文献