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101.
102.
位移反分析的粒子群优化-高斯过程协同优化方法 总被引:2,自引:0,他引:2
针对采用随机全局优化技术进行岩土工程位移反分析存在数值计算量大、效率低的问题,将粒子群优化算法与高斯过程机器学习技术相结合,提出了位移反分析的粒子群优化-高斯过程协同优化方法。该方法利用全局寻优性能优异的粒子群优化算法进行寻优的基础上,采用高斯过程机器学习模型不断地总结历史经验,预测包含全局最优解的最有前景区域,通过提高粒子群搜索效率并降低适应度评价次数,进而有效地降低位移反分析过程中的数值计算工作量。多种测试函数的数学验证和工程算例的研究结果表明该方法是可行的,与传统方法相比较,可显著地降低位移反分析的计算耗时。 相似文献
103.
104.
105.
106.
In this paper, besides general definition of hardness ratio of gamma-ray bursts (GRBs), HR
32, we also presented new definitions of hardness ratios, HR
hl and HR
ll, then presented the results of correlation studies, examining the association between the hardness ratios and the spectral
fitting parameters (E
0 or E
peak, α, β) by using the GRB data observed by BATSE. The HR
hl is defined as the fluence of channel 4 divided by the sum of the fluences of channels 1 to 3,and the HR
ll is defined as the fluence of channel 3 divided by the sum of the fluences of channel 1 and 2. We found that E
0 and E
peak are correlated with hardness ratios, and β is only correlated with log (HR
hl). The α is not correlated with any hardness ratios in the total sample of GRBs, while it correlated with log (HR
ll) and log (HR
32) in the two subsets seperated at log (HR
ll) = 0.34 ×α +0.66, respectively. These results show that a harder spectra tends to be steeper and has a higher E
peak or E
0; HR
hl describes the spectral behaviors in high energy, while both of HR
ll and HR
32 reflect the spectral characteristics in low energy; the spectral behaviors in low energy are different for the two subsets.
We also presented a brief qualitative analysis discussion to the correlations and suggested that the correlations are caused
by both of intrinsic and cosmological effects, but intrinsic effects are dominant.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
107.
108.
Cheng-Yue Su Yi-Ping Qin Jun-Hui Fan Zhang-Yu Han National Astronomical Observatories/Yunnan Observatory Chinese Academy of Sciences Kunming Graduate School of Chinese Academy of Sciences Beijing Department of Physics Guangdong University of Technology Guangzhou Center for Astrophysics Guangzhou University Guangzhou Department of Mechanics University of Science Technology of China Hefei 《中国天文和天体物理学报》2006,6(3):323-330
We investigate the forming of gamma-ray burst pulses with a simple one-dimensional relativistic shock model. The mechanism is that a "central engine" drives forward the nearby plasma inside the fireball to generate a series of pressure waves. We give a relativistic geometric recurrence formula that connects the time when the pressure waves are produced and the time when the corresponding shocks occurred. This relation enables us to relate the pulse magnitude with the observation time. Our analysis shows that the evolution of the pressure waves leads to a fast rise and an exponential decay pulses. In determining the width of the pulses, the acceleration time is more important than that of the deceleration. 相似文献
109.
ZHAO Weibing LI Xingqun 《中国地理科学(英文版)》2006,16(3):203-210
1 Introduction “Tourism is advanced by businesses and governments alike as a development mechanism which can lift people out of poverty and make them equal partners in society. But regardless of how altruistic this claim may sound, it is doubtful whether those who are intended to benefit— at least according to the rhetoric—have gained nearly as much as those promoting tourism through corporate globalization… The tourism sector is tied closely to the globalizing force which pursues profit o… 相似文献
110.
广西五圩矿田三排洞矿床Sb-Au与Pb-Zn-Sb矿化地质地球化学特征与复合成矿分析 总被引:2,自引:2,他引:0
广西丹池成矿带五圩矿田三排洞矿床由早期Sb-Au矿化和晚期Pb-Zn-Sb矿化组成,而五圩矿田其它矿床则仅见Pb-Zn-Sb矿化。本文对比分析了三排洞矿床两类矿化控矿构造产状、包裹体均一温度、盐度、气液相组成、矿物组合、闪锌矿铁含量等差异,探讨两类矿化成因联系,论证其是否为复合成矿作用形成的矿床。早期Sb-Au矿化主要产于走向320°断裂带中,矿体倾向NE,倾角50°~60°,主要由辉锑矿、雄雌黄、辰砂及自然金组成(Au2×10-6),银含量低(20×10-6);Pb-ZnSb矿化产于走向350°断裂带中,矿脉倾向SWW,倾角70°~80°,主要由闪锌矿、脆硫锑铅矿、特硫锑铅矿、硫锑铅矿等组成,富银(100×10-6),贫金(0.1×10-6)。早期和晚期矿化脉中流体包裹体温度峰值分别在160~200℃和180~230℃之间,富CO_2包裹体数占总包裹体数分别约为8%和45%;早期和晚期矿化闪锌矿Fe含量分别为小于0.12%和在1.40%~3.65%之间;早期矿化锑矿物主要为辉锑矿,晚期矿化锑矿物则主要为脆硫锑铅矿、特硫锑铅矿及硫锑铅矿。上述差异表明早期矿化成矿热液具Sb-Au-As-Hg元素组合,相对贫CO_2及Fe,而晚期矿化成矿流体具Pb-Zn-Sb-Ag元素组合,富CO_2及Fe。据五圩矿田其它Pb-Zn-Sb矿床未发生Au成矿作用、三排洞矿床两期矿化受控于不同产状断裂构造、晚期矿化成矿温度高于早期矿化成矿温度、两期矿化成矿热液元素组成尤其是Au和Ag含量及CO_2含量的明显差异等,可以认为三排洞矿床早期Sb-Au和晚期Pb-Zn-Sb矿化为不同成矿作用的产物,两者没有成因联系,三排洞矿床发生了复合成矿作用。同一矿区不同成矿作用可形成不同元素组合矿体。 相似文献