全文获取类型
收费全文 | 1590篇 |
免费 | 278篇 |
国内免费 | 380篇 |
专业分类
测绘学 | 227篇 |
大气科学 | 237篇 |
地球物理 | 376篇 |
地质学 | 928篇 |
海洋学 | 110篇 |
天文学 | 118篇 |
综合类 | 113篇 |
自然地理 | 139篇 |
出版年
2024年 | 9篇 |
2023年 | 41篇 |
2022年 | 99篇 |
2021年 | 93篇 |
2020年 | 91篇 |
2019年 | 77篇 |
2018年 | 84篇 |
2017年 | 66篇 |
2016年 | 88篇 |
2015年 | 89篇 |
2014年 | 97篇 |
2013年 | 102篇 |
2012年 | 68篇 |
2011年 | 100篇 |
2010年 | 84篇 |
2009年 | 101篇 |
2008年 | 85篇 |
2007年 | 102篇 |
2006年 | 77篇 |
2005年 | 74篇 |
2004年 | 43篇 |
2003年 | 46篇 |
2002年 | 47篇 |
2001年 | 51篇 |
2000年 | 51篇 |
1999年 | 63篇 |
1998年 | 51篇 |
1997年 | 41篇 |
1996年 | 28篇 |
1995年 | 34篇 |
1994年 | 43篇 |
1993年 | 34篇 |
1992年 | 19篇 |
1991年 | 16篇 |
1990年 | 14篇 |
1989年 | 3篇 |
1988年 | 3篇 |
1987年 | 3篇 |
1986年 | 9篇 |
1985年 | 6篇 |
1984年 | 5篇 |
1983年 | 1篇 |
1982年 | 1篇 |
1981年 | 2篇 |
1979年 | 3篇 |
1958年 | 2篇 |
1957年 | 2篇 |
排序方式: 共有2248条查询结果,搜索用时 46 毫秒
991.
Xiong Ding-rong Zhang XiongZheng Yong-gang Huang Bang-rongMao Li-sheng Liu Wen-guang 《Chinese Astronomy and Astrophysics》2013
In this paper, we collect the redshift, bolometric luminosity, the full- width at half maximum of the Hβ emission line, the monochromatic luminosity at 5100 Å and the radio loudness for the sample of 117 quasars, including 20 radio-quiet quasars (RQQs) and 97 radio-loud quasars (RLQs). With the reverberation mapping method we calculate the black hole mass and Eddington ratio for this sample, as well as the radio luminosity from the total 5 GHz ?ux density. By analyzing the correlations among them, we obtain the following conclusions: (1) The black hole mass has weak correlations with the bolometric luminosity, radio loudness and radio luminosity for the RQQs, and has strong correlations with the bolometric luminosity, radio loudness and radio luminosity for the RLQs; (2) For the RQQs, the bolometric luminosity has weak correlations with the radio luminosity and 5 100 Å monochromatic luminosity, and for the RLQs, the bolometric luminosity has strong correlations with the radio luminosity and 5 100 Å monochromatic luminosity; (3) The RQQs and RLQs differ in the distributions of the black hole mass, emission line width and Eddington ratio. Based on these results, we suggest: the difference of emission line width between RQQs and RLQs is probably caused by the difference of black hole mass; the fundamental difference between RQQs and RLQs is caused by the difference of their intrinsic physical nature; the black hole mass, black hole spin, Eddington ratio, and host galaxy morphology are the important parameters to explain the origin of radio loudness and the double-peaked distribution; and the radio jet is closely related with the accretion rate of disk. 相似文献
992.
The linear stability analysis of the radial and non-radial oscillations for the evolutionary model of a star with the mass of 0.6∼3 M8 has been per- formed by using the nonlocal and time-dependent convection theory. The results show that the unstable low-temperature stars on the right side of the instabil- ity strip in the HR diagram can be divided into two groups. One is of the stars of solar-like oscillations, composed of the main-sequence dwarfs, subgiants, and the red giants with low- and intermediate-luminosity, which are unstable in the intermediate- and high-order (nr ≥ 12) p-modes, but stable in the low- order (nr ≤ 5) p-modes. Another is of the Mira-like stars, composed of the luminous red giants and AGB stars, which are just contrary to the solar-like stars, unstable in the low-order (nr ≤ 5) p-modes, but stable in the intermediate- and high-order (nr ≥ 12) p-modes. On the red edge of Cepheid (δ Scuti) insta- bility strip, the oscillations of solar-like and Mira-like stars can be explained uniformly by the coupling between convection and oscillations (CCO). For the low-temperature stars on the right side of the instability strip, the CCO is the dominant excitation and damping mechanism for the low- and intermediate-order p-modes, and the stochastic excitation of turbulence becomes important only for the high-order p-modes of solar-like oscillations. 相似文献
993.
中条山铜矿峪铜矿区火山岩的地球化学特征及构造背景 总被引:1,自引:0,他引:1
对铜矿峪火山岩进行常量元素、微量元素及稀土元素研究表明,SiO2质量分数为47.22%~76.00%,平均66.21%,Al2O3含量为11.03%~20.03%,属铝饱和类型。通过常量元素投点图分析,属一种高钾系列火山岩。稀土元素特征表明,火山岩的源岩浆来源于上地慢。在微量元素的球粒陨石标准化图上,表现为不相容元素Rb、K、Ba、Th的高度富集,同时,具有Sr、Tb和Nb、Ti的亏损,其总体配分型式类似于板内拉斑玄武岩。 相似文献
994.
Endosulfan, an organochlorine pesticide, is highly toxic and effective at controlling pests in agriculture, horticulture, and public health programs. In this study, static bioassays were used to evaluate the toxicity of endosulfan to freshwater prawns( Macrobrachium rosenbergii) of various lengths(1.5±0.03,4±0.08, and 7±0.06 cm). Additionally, the activities of peroxidase(POD), acid phosphatase(ACP),alkaline phosphatase, acetylcholinesterase(AChE), and Na + /K +-ATPase were analyzed to refl ect the effects of endosulfan exposure. The 96 h LC 50 of endosulfan for prawns 1.5, 4, and 7 cm long were 1.86, 4.53,and 6.09μg/L, respectively, improved tolerance to endosulfan with growth. The POD activities of test organisms exposed to low concentrations of endosulfan were inhibited, indicating the presence of oxygen damaged tissue. Moreover, a notable decrease in AChE activity was observed due to overstimulation of neurotransmission, which might result in abnormal behavior. The effect caused by endosulfan on phosphatase production in the hepatopancreas of prawns 1.5, 4, and 7 cm long was different because the ability of nonspecifi c immune regulation increased with growth. The 96 h LC 50 values obtained in this study could be used in the formulation of water-quality criteria in China. Moreover, the changes in enzymes activities of M. rosenbergii under stress of endosulfan could be applied in the establishment of early warning indicators for bio-safety. 相似文献
995.
LI Chongyin LING Jian SONG Jie PAN Jing TIAN Hu CHEN Xiong 《Acta Meteorologica Sinica》2014,28(5):671-692
Tropical intraseasonal oscillation (including the Madden-Julian oscillation) is an important element of the atmospheric circulation system. The activities and anomalies of tropical intraseasonal oscillations affect weather and climate both inside and outside the tropical region. The study of these phenomena therefore represents one of the frontiers of atmospheric sciences. This review aims to synthesize and summarize studies of intraseasonal oscillation (ISO) by Chinese scientists within the last 5-10 years. We focus particularly on ISO's mechanisms, its numerical simulations (especially the impacts of diabatic heating profiles), relationships and interactions with ENSO (especially over the western Pacific), impacts on tropical cyclone genesis and tracks over the northwestern Pacific, and influences on the onset and activity of the South and East Asian monsoons (especially rainfall over China). Among these, focuses of ongoing research and unresolved issues related to ISO are also discussed. 相似文献
996.
兵棋是对作战过程进行逻辑推演研究和评估的重要工具,是现代作战模拟的一种重要方法和手段。兵棋的三大要素包括棋盘、棋子和规则,棋盘的经典样式就是六角格网兵棋棋盘,计算机兵棋中也常采用六角格网兵棋棋盘描述战场地形环境。推演过程中通常涉及到大量的坐标转换,因此坐标转换效率对于推演效率具有重要影响。针对经纬度坐标和六角格网编码的转换,提出了直接转换和间接转换两种坐标转换方法,分析了各自的基本转换原理,并给出了坐标转换公式,最后通过实验对两种方法的转换效率进行了分析,证实间接坐标转换法具有更高的转换效率。 相似文献
997.
Huarong Xie Qing Xu Quanan Zheng Xuejun Xiong Xiaomin Ye Yongcun Cheng 《海洋学报(英文版)》2022,41(6):137-145
This study assesses the accuracy and the applicability of the Korteweg-de Vries(KdV) and the nonlinear Schr?dinger(NLS) equation solutions to derivation of dynamic parameters of internal solitary waves(ISWs) from satellite images. Visible band images taken by five satellite sensors with spatial resolutions from 5 m to 250 m near the Dongsha Atoll of the northern South China Sea(NSCS) are used as a baseline. From the baseline, the amplitudes of ISWs occurring from July 10 to 13, 2017 are estimate... 相似文献
998.
地形起伏度最佳分析区域预测模型 总被引:3,自引:0,他引:3
地形起伏度指分析区域内最高点和最低点之差,反映宏观区域内地形的起伏特征,是描述地貌形态的定量指标。确定最佳分析区域是地形起伏度提取算法的核心步骤,以及决定地形起伏度提取结果有效性的关键。本文以全国范围内随机选取的78个实验区域、三种不同尺度的DEM数据作为实验对象,分别进行系列分析区域尺度的地形起伏度计算,建立了基于微观地形特征因子的地形起伏度最佳分析区域预测模型。实验表明:相同区域、不同尺度的DEM数据提取的地形起伏度存在差异,DEM尺度相差较小时,地形起伏度的差异也较小;地形起伏度和实验区域的最大高程、区域高差、平均坡度和平均坡度变率等地形特征因子存在强相关关系;当置信水平为0.05时,预测模型拟合参数的准确率达到95%以上,证明预测模型可以有效地确定最佳分析区域的取值范围。 相似文献
999.
1000.
On April 20, 2013 at 8:02 am, a magnitude 7.0 earthquake occurred in Lushan County, Sichuan Province, China, which induces massive landslides, causes great losses to life and property. Based on the locations of aftershocks provided by the China Earthquake Network Center and the characteristic of Longmenshan active faults system, combined with the current preliminary focal mechanism solution, the fault rupture direction is determined. With the finite fault inversion method, we invert the rupture process of the Lushan M s 7.0 earthquake by teleseismic waveforms data. The inversion results indicate that the main shock is dominated by thrust fault component and the rupture initiated at depth of 15 km, and most of slip ruptured around the hypocenter with the peak slip of about 1.5 m. Most of rupture slips released at the first 20 s and the main rupture occurred at the first 10 s after the onsets of the mainshock. Most of seismic energy released near the hypocenter with a length of 28 km, especially on both sides of the hypocenter with the range of 20 km, and the seismic energy released relatively smaller in other areas. There is a large area with weak slip between the main rupture and another two asperities on both sides of the hypocenter; it may imply that the accumulated strain on the rupture fault has not been completely released. Therefore, there is a significant possibility of having strong aftershocks in the areas where energy is not fully released. This is also the main reason why there are a lot of moderate to strong aftershocks in the Lushan aftershock sequence. In addition, there is an earthquake vacant zone with a length of about 50 km between the Wenchuan M w 7.9 earthquake and this event, which is of high earthquake risk and is deserved to be paid close attention to. 相似文献