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101.
利用伊利盆地砂岩型铀矿床干酪根热解色谱数据,计算获得氢指数、氧指数等重要指标,在此基础上,应用氢指数、氧指数划分了伊犁盆地铀矿床干酪根类型,再依据烃指数和产率指数对伊犁盆地铀矿床干酪根的成熟度进行了初步评价。 相似文献
102.
基于相空间重构的边坡位移预测 总被引:20,自引:1,他引:19
根据边坡位移时间序列的非线性性质, 应用基于相空间重构的实时预测方法, 可以充分利用时间序列信息, 预测
各种边坡变形演化趋势。 讨论了局域法和基于 Ly apunov 指数的预测法。 实例研究表明, 基于相空间重构的预测方法具
有比非平稳时间序列更高的预测精度和更广的适应性。 相似文献
103.
104.
搅拌是海水混合的重要组成,其强度可由基于拉格朗日观点的有限时间李亚普诺夫指数(Finite Time Lyapunov Exponents,FTLE)定量计算。文章利用卫星高度计资料统计分析了2002~2011年间南海地转流场的FTLE时空变化特征。结果显示,FTLE在越南东南海域强度最大,对应水平搅拌作用最强;而在南海西北、东南区域其值偏低。近10年的南海水平搅拌呈缓慢增强趋势,且存在明显的季节变化,夏季较强而冬季偏弱。FTLE的空间分布与基于欧拉观点的涡动能和应变速率相似,强搅拌的区域,其涡动能和应变速率亦较高。与Okubo-Weiss参数的比较则显示,构成流场拉格朗日拟序结构(Lagrangian Coherent Structures,LCS)的FTLE脊线与流场中涡旋联系紧密,FTLE低值集中在旋转主导的涡旋内部,而高值多在涡旋周围应变主导区域。 相似文献
105.
当气溶胶谱满足Junge分布时,Angstrom指数 (α) 可以准确地描述粒子大小,但真实大气气溶胶很少完全满足这一条件,仅用α判断粒子大小会有较大出入。基于北京、香河、兴隆、太湖4个Aeronet观测站21世纪以来各站历时都超过1年的气溶胶光学厚度资料,获得5511组lnτ与lnλ的二次拟合参数a2,a1,尝试找到一种结合α,a2,a1判断粒子大小的方法。结果表明:当气溶胶为粗粒子时 (Vfine/Vtotal<0.2),α均小于0.75,仅用α就可以较好地判断粒子大小,但当气溶胶以细粒子为主时 (Vfine/Vtotal>0.7),该方法会有较大出入,此时a2,a1可以有效地辅助α判断粒子大小,α>0.75,a2<-0.5或a2<-0.5,a1<-1.0是较好的判据。此外,分析发现国外研究提出的用a2-a1判断粒子大小的方法效果并不理想,尤其在1<a2-a1<2的情况下,粒子的组成有多种可能。 相似文献
106.
In this study, signal processing approaches and nonlinear identification are used to measure seismic responses of reinforced concrete (RC) structures using the shaking table test. To analyze structural nonlinearity, an equivalent linear system with time‐varying model parameters, singular spectrum analysis to elucidate residual deformation, and wavelet packet transformation analysis to yield the energy distribution among components are adopted to detect the nonlinearity. Then, damage feature extraction is conducted using both the Holder exponent and the Level‐1 detail of the discrete wavelet component. Finally, the modified Bouc‐Wen hysteretic model and the system identification process are employed to the shaking table test data to evaluate the physical parameters, including the stiffness degradation, the strength deterioration and the pinching hysteresis. Finally, the identified stiffness and strength degradation functions from the test data of RC frames in relation to the degree of ground shaking, damage index and the identified nonlinear features are discussed. Based on the proposed method, both signal‐based and model‐based identifications, the relationship between the damage occurrence and severity of structural damage can be identified. Copyright © 2010 John Wiley & Sons, Ltd. 相似文献
107.
The backward nonlinear local Lyapunov exponent method(BNLLE) is applied to quantify the predictability of warm and cold events in the Lorenz model. Results show that the maximum prediction lead times of warm and cold events present obvious layered structures in phase space. The maximum prediction lead times of each warm(cold) event on individual circles concentric with the distribution of warm(cold) regime events are roughly the same, whereas the maximum prediction lead time of events on other circles are different. Statistical results show that warm events are more predictable than cold events. 相似文献
108.
Marc Fouchard Elena Lega Christiane Froeschlé Claude Froeschlé 《Celestial Mechanics and Dynamical Astronomy》2002,83(1-4):205-222
It is already known (Froeschlé et al., 1997a) that the fast Lyapunov indicator (hereafter FLI), i.e. the computation on a relatively short time of a quantity related to the largest Lyapunov indicator, allows us to discriminate between ordered and weak chaotic motion. Using the FLI many results have been obtained on the standard map taken as a model problem. On this model we are not only able to discriminate between a short time weak chaotic motion and an ordered one, but also among regular motion between non resonant and resonant orbits. Moreover, periodic orbits are characterised by constant FLI values which appear to be related to the order of periodic orbits (Lega and Froeschlé, 2001). In the present paper we extend all these results to the case of continuous dynamical systems (the Hénon and Heiles system and the restricted three-body problem). Especially for the periodic orbits we need to introduce a new value: the orthogonal FLI in order to fully recover the results obtained for mappings. 相似文献
109.
G. Contopoulos N. Voglis C. Efthymiopoulos C. Froeschlé R. Gonczi E. Lega R. Dvorak E. Lohinger 《Celestial Mechanics and Dynamical Astronomy》1997,67(4):293-317
The spectra of ‘stretching numbers’ (or ‘local Lyapunov characteristic numbers’) are different in the ordered and in the chaotic
domain. We follow the variation of the spectrum as we move from the centre of an island outwards until we reach the chaotic
domain. As we move outwards the number of abrupt maxima in the spectrum increases. These maxima correspond to maxima or minima
in the curve a(θ), where a is the stretching number, and θ the azimuthal angle. We explain the appearance of new maxima in
the spectra of ordered orbits. The orbits just outside the last KAM curve are confined close to this curve for a long time
(stickiness time) because of the existence of cantori surrounding the island, but eventually escape to the large chaotic domain
further outside. The spectra of sticky orbits resemble those of the ordered orbits just inside the last KAM curve, but later
these spectra tend to the invariant spectrum of the chaotic domain. The sticky spectra are invariant during the stickiness
time. The stickiness time increases exponentially as we approach an island of stability, but very close to an island the increase
is super exponential. The stickiness time varies substantially for nearby orbits; thus we define a probability of escape Pn(x) at time n for every point x. Only the average escape time in a not very small interval Δx around each x is reliable. Then
we study the convergence of the spectra to the final, invariant spectrum. We define the number of iterations, N, needed to
approach the final spectrum within a given accuracy. In the regular domain N is small, while in the chaotic domain it is large.
In some ordered cases the convergence is anomalously slow. In these cases the maximum value of ak in the continued fraction expansion of the rotation number a = [a0,a1,... ak,...] is large. The ordered domain contains small higher order chaotic domains and higher order islands. These can be located
by calculating orbits starting at various points along a line parallel to the q-axis. A monotonic variation of the sup {q}as
a function of the initial condition q0 indicates ordered motions, a jump indicates the crossing of a localized chaotic domain, and a V-shaped structure indicates
the crossing of an island. But sometimes the V-shaped structure disappears if the orbit is calculated over longer times. This
is due to a near resonance of the rotation number, that is not followed by stable islands.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
110.
冲积河流泥沙输移幂律函数关系与不平衡输沙理论是对河道不平衡输沙同一物理现象的不同描述,两者既有区别也有联系。比较研究发现:对于恒定均匀流不平衡输沙过程,当输沙位于近平衡态时两者含沙量导函数表达式具有一阶近似等价性,当输沙远离平衡态时前者含沙量导函数中隐含考虑有泥沙恢复饱和系数的变化。基于两者等价性,推导建立了幂律函数指数计算表达式,表明指数随泥沙沉速、单宽流量和沿程距离而变化,且随着输移距离的增大呈指数衰减。基于前者含沙量导函数表达式结构特点,分析建立了相应泥沙恢复饱和系数变化的计算表达式。综合以上成果,改进提出了一种变幂指数的泥沙输移幂律函数计算模型。对库里·阿雷克沉沙池沿程断面输沙指数及含沙量计算结果表明,不同距离过水断面输沙指数的变化规律是合理的,含沙量计算值与实测值变化趋势基本符合。 相似文献