On the impossibility of mean-field dynamos with some spherical symmetry of the motions

Abstract

A spherical mean-field dynamo model is considered in which both the mean motion and the mean electro-motive force due to fluctuating motions show some spherical symmetry. It is shown that under some reasonable assumptions the magnetic field is bound to decay to zero.     

A review of: “Problems of Solar and Stellar Oscillations. Iau Colloquium No. 66. Edited by D. O. Gough. D. Reidel Publishing Company, 493 pp. Df1195.00/U.S. $84.50 (ISBN 90-277-1554-8). 1983.”

Abstract

The model equations describing two-dimensional thermohaline convection of a Boussinesq fluid in a rotating horizontal layer are known to support multiple instabilities, depending on the values of certain control parameters (Arneodo et al., 1985). Most of these multiple instabilities have already been studied for double or triple diffusive convection, where behaviours ranging from simple steady to irregular motions have been found. Here we consider the one remaining bifurcation mentioned by Arneodo et al. (1985): the interaction between a steady and an oscillatory convection roll when the linear spectrum for a single wavenumber comprises one zero and one pair of purely imaginary eigenvalues. The method of centre manifolds and normal forms is used to derive evolution equations for the amplitudes of the convection rolls close to bifurcation and the behaviours associated with the equations is discussed.     

Finite amplitude convection and magnetic field generation in a rotating spherical shell

Abstract

Finite amplitude solutions for convection in a rotating spherical fluid shell with a radius ratio of η=0.4 are obtained numerically by the Galerkin method. The case of the azimuthal wavenumber m=2 is emphasized, but solutions with m=4 are also considered. The pronounced distinction between different modes at low Prandtl numbers found in a preceding linear analysis (Zhang and Busse, 1987) is also found with respect to nonlinear properties. Only the positive-ω-mode exhibits subcritical finite amplitude convection. The stability of the stationary drifting solutions with respect to hydrodynamic disturbances is analyzed and regions of stability are presented. A major part of the paper is concerned with the growth of magnetic disturbances. The critical magnetic Prandtl number for the onset of dynamo action has been determined as function of the Rayleigh and Taylor numbers for the Prandtl numbers P=0.1 and P=1.0. Stationary and oscillatory dynamos with both, dipolar and quadrupolar, symmetries are close competitors in the parameter space of the problem.     

On topographic core-mantle coupling

Abstract

The purpose of this note is two-fold: to draw attention to a perplexing difficulty connected with topographic core-mantle coupling, and to suggest tentatively an explanation. The difficulty is an apparent conflict between the most comprehensive theory of the coupling so far attempted (Anufriev and Braginsky, 1975a, b, 1977a, b) and recent explicit calculations based on magnetic and seismic information (Speith et al., 1986). It is argued that asymmetric deviations from Anufriev and Braginsky's basically axisymmetric model of the underlying core flow are capable of resolving the difficulty.     

近断层地震动作用下LRB隔震储罐地震反应特征研究

采用Bouc-Wen模型模拟铅芯橡胶支座(LRB)非线性力学性能,建立LRB基础隔震储罐地震反应的数值模型.利用叠加原理得到人工合成近断层脉冲型地震动,从实际典型近断层地震动和人工近断层脉冲地震动输入两个角度出发,以远场地震反应为参照,系统探讨了近断层地震动作用下LRB隔震储罐地震反应特点以及近断层地震动运动特征的影响规律.研究发现,近断层地震动作用下LRB隔震储罐地震反应明显大于远场地震反应值,显著的近断层脉冲效应是隔震储罐设计不容忽视的问题.近断层地震动的PGV/PGA值是决定隔震储罐地震反应的综合指标,PGV/PGA值较大时,隔震储罐地震反应脉冲效应突出.另外,脉冲周期、脉冲参与系数以及脉冲类型也是影响LRB隔震储罐地震反应的重要因素.在脉冲参与系数越大、含有脉冲数量越多的近断层地震动作用下,隔震储罐地震反应越强烈.当脉冲周期接近储罐晃动周期时,晃动波高会出现峰值.     

强地震前地下流体趋势异常的再探讨

重新探讨了强地震前地下流体趋势异常,获得了一些认识：地下流体异常不一定存在完整的趋势、短期和短临等异常类型,但趋势异常普遍存在;地下流体特别是地下水位的趋势性异常,其开始时的形态不一定为缓慢变化;地下流体趋势异常不一定具有时空转移特征;地下流体趋势异常可能为“共同前兆”.     

AVO analysis with partial stacking to detect gas anomalies in the GÜEPAJÉ-3D project

We applied analysis AVO with partial stacking to an onshore gas field in order to detect gas at the top of the Ciénaga de Oro formation (FCO), by using seismic gathers of the Güepajé-3D project. The technique was supported by petrophysical analysis of the Ayombe-1 well.The sensitivity of seismic response to changes in the saturating fluid was evaluated by fluid substitution technique in an interval of the Ayombe-1 well. As a result, a class I AVO anomaly at the top of the FCO was observed, even though the gas and water responses were similar. After applying AVO with partial stack technique at the top of FCO, AVO class I anomalies were observed in the Ayombe-1 and Güepajé-1 gas wells and none in the dry Güepajé-3 well. In spite of being reported with gas, the results in the Güepajé-2 well indicated any to an incipient class I anomaly related to a weak seismic response associated to gas.When the technique was applied to the seismic volume of the Güepajé-3D Project, a map of the direct gas indicator was obtained. The map shows a high correlation with the structural surface at top of FCO. Lithic factors such as compaction, cementation and carbonate overlaying the FCO and variable thickness of partial and full saturated layers, may cause anomalies in zones unlikely to contain gas.     

Effect of a uniform magnetic field on nonlinear magnetocenvection in a rotating fluid spherical shell

Abstract

Dynamic interaction between magnetic field and fluid motion is studied through a numerical experiment of nonlinear three-dimensional magnetoconvection in a rapidly rotating spherical fluid shell to which a uniform magnetic field parallel to its spin axis is applied. The fluid shell is heated by internal heat sources to maintain thermal convection. The mean value of the magnetic Reynolds number in the fluid shell is 22.4 and 10 pairs of axially aligned vortex rolls are stably developed. We found that confinement of magnetic flux into anti-cyclonic vortex rolls was crucial on an abrupt change of the mode of magnetoconvection which occurred at Δ = 1 ～ 2, where A is the Elsasser number. After the mode change, the fluid shell can store a large amount of magnetic flux in itself by changing its convection style, and the magnetostrophic balance among the Coriolis, Lorentz and pressure forces is established. Furthermore, the toroidal/poloidal ratio of the induced magnetic energy becomes less than unity, and the magnetized anti-cyclones are enlarged due to the effect of the magnetic force. Using these key ideas, we investigated the causes of the mode change of magnetoconvection. Considering relatively large magnetic Reynolds number and a rapid rotation rate of this model, we believe that these basic ideas used to interpret the present numerical experiment can be applied to the dynamics in the Earth's and other planetary cores.     

钻井液侵入海洋含水合物地层的一维数值模拟研究

本文以墨西哥湾水合物区域为背景,利用数值模拟方法研究了过平衡钻井条件下,当钻井液温度高于地层中水合物稳定温度时,水基钻井液侵入海洋含水合物地层的动态过程及其一般性规律.与侵入常规油气地层相比,耦合水合物分解和再形成是钻井液侵入海洋含水合物地层的主要特征.模拟结果表明,钻井液密度、温度和盐度都对侵入过程有影响.在一定条件下,钻井液密度越大,温度和含盐量越高,则钻井液侵入程度越深,热量传递越远,水合物分解程度越大.分解的水气在合适条件下又会重新形成水合物,影响了钻井液进一步侵入.而重新形成的水合物的饱和度甚至可能高于原位水合物饱和度,在井周形成一个"高饱水合物"环带.这一现象归因于钻井液侵入的驱替推挤、水合物分解的吸热以及地层传热的滞后等因素共同作用.在地层物性一定的条件下,高饱水合物环带的出现与否主要受钻井液温度和盐度控制.水合物分解以及高饱水合物环带的出现对井壁稳定和电阻率测井解释有很大影响.因此,为维护井壁稳定、确保测井准确和减少水合物储层伤害,就必须对钻井液密度、温度和滤失量进行严格控制,防止地层中的水合物大量分解.最好采用控制压力钻井(MPD)和深侧向测井方式,同时尽量选用低矿化度的含水合物动力学抑制剂的钻井液体系,采取低温快速循环方式.     

瘤背石磺体腔细胞分类、免疫相关酶特性及初步转录组学分析

瘤背石磺(Onchidium struma)广泛分布于潮间带和潮下带,是海洋生物向陆地生物辐射进化的重要代表,也是环境监测的指示生物.为丰富瘤背石磺的基础免疫学资料,本文研究了瘤背石磺体腔细胞的类别、细胞密度和体腔液免疫相关酶活性,并通过RNA-Seq测序获得体腔细胞转录本,进行生物信息学分析.结果表明,瘤背石磺主要有...