March 2013 JASEM ISSN 1119-8362 Full-text Available Online at J. Appl. Sci. Environ. Manage. All rights reserved www.ajol.info and Vol. 17 (1) 139-151 www.bioline.org.br/ja Effects of Brinkman number on thermal-driven convective spherical Dynamos . *1M. I. NGWUEKE; T. M. ABBEY Theoretical Physics Group; Department of Physics, University of Port Harcourt, Port Harcourt, Nigeria. *Corresponding author (e-mail:
[email protected]; Phone: 234-703-5891392, 234-803-3409479 ) KEYWORDS: Magnetic field generation, Thermal-driven convection, Brinkman number, Dynamo action, Fluid outer core ABSTRACT: Brinkman number effects on the thermal-driven convective spherical dynamos are studied analytically. The high temperature of the Earth’s inner core boundary is usually conducted by the viscous, electrically conducting fluid of the outer core to the core mantle boundary as the Earth cools. The problem considers conducting fluid motion in a rapidly rotating spherical shell. The consequence of this exponential dependence of viscosity on temperature is considered to be a thermal- driven convective phenomenon. A set of constitutive non-linear equations were then formulated in which the solutions for the flow variables were obtained by perturbation technique. The results illustrate enhancement of dynamo actions, demonstrating that magnetic field generation with time is possible. Moreover, the increased magnetic Prandtl number Pm with high Brinkman number shows dynamo actions for fixed Rayleigh and Taylor number values. The overall analyses succour our