Masterarbeit, 2012
126 Seiten, Note: 3
Chapter 1 Literature Review
1.1 Magnetohydrodynamics
1.2 Definition of Useful Parameters
1.3 Fully Developed flows in Rectangular Curved Duct
1.4 Developing Flow in Pipes and Rectangular Duct
1.5 Rotating Duct
1.6 MHD Flow in a Duct and Pipe
Chapter 2
2.1 Governing Equation
Chapter 3 Numerical Technique
Chapter 4 Flow through a Rotating Rectangular Straight Duct with Magnetic Field along Center Line
4.1 Introduction
4.2 Governing Equation
4.3 Numerical Solution
4.4 Results and Discussion
Chapter 5 Conclusion
This thesis aims to perform numerical calculations to investigate the effects of a magnetic field on incompressible viscous steady fluid flow through a rotating rectangular straight duct. The research focuses on analyzing the combined influence of the Magnetic parameter, Taylor number, Dean number, and aspect ratio on flow characteristics, solution curves, and the evolution of secondary flow structures.
1.1. Magnetohydrodynamics (MHD)
Magnetohydrodynamics (MHD) is a branch of magneto fluid dynamics i.e. continuum mechanics, which deals with the flow of electrically conducting fluids in electric and magnetic fields. The largest advance towards an understanding of such phenomena probably comes from the field of astrophysics. It has been long suspected that most of the matter in the universe is in the plasma or the state of highly ionized gases and much of the basic knowledge in the area of electromagnetic fluid dynamics evolved from these studies.
The field of Magnetohydrodynamics consists of the study of a continuous, electrically conducting fluid under the influence of electromagnetic fields, as a branch of plasma physics. Originally, MHD included only the study of strictly incompressible fluid but today the terminology is applied to studies of partially ionized gases as well as the other names have been suggested, such as magneto-fluid-mechanics or magneto-aero-dynamics, but original nomenclature has persisted. The essential requirement for problems to be analyzed under the laws of MHD is that the continuum approach be applicable.
There are many natural phenomena and engineering problems are susceptible to MHD analysis. It is useful in astrophysics because much of the universe is filled with widely spaced charged particles and permeated by magnetic fields and so the continuum assumption becomes applicable. Geophysicists encounter MHD phenomena in the interaction of conducting fluids and magnetic fields that are present in and around heavenly bodies. Engineers employee have been used MHD principles to design of heat exchangers, pumps and flow meters, space vehicle propulsion, control and re-entry problems, designing communications and radar system, creating novel power generating systems and developing confinement schemes for controlled fusion.
Chapter 1 Literature Review: Provides an overview of magnetohydrodynamics, relevant dimensionless parameters, and existing research on flow in curved, rotating, and MHD-affected ducts.
Chapter 2: Defines the governing mathematical model for incompressible viscous fluid flow in a rotating rectangular duct, including momentum and continuity equations.
Chapter 3 Numerical Technique: Details the spectral method and numerical tools, such as Chebyshev polynomials and the Newton-Raphson iteration, used to solve the governing equations.
Chapter 4 Flow through a Rotating Rectangular Straight Duct with Magnetic Field along Center Line: Presents the numerical results and discussion on flow patterns, secondary flow structures, and the influence of magnetic and rotational parameters.
Chapter 5 Conclusion: Summarizes the key findings regarding the physical characteristics of the flow, vortex solutions, and the effect of parameters on the axial flow profile.
Magnetohydrodynamics, Fluid Flow, Rotating Duct, Rectangular Duct, Spectral Method, Magnetic Parameter, Taylor Number, Dean Number, Aspect Ratio, Secondary Flow, Vortex Solution, Numerical Simulation, Chebyshev Polynomial, Newton-Raphson Method, Axial Flow
The thesis investigates the numerical behavior of incompressible, steady, viscous fluid flow through a straight rectangular duct that is rotating at a constant angular velocity, subjected to a magnetic field.
The flow is governed by the interaction of the Magnetic parameter (Mg), Taylor number (Tr), Dean number (Dn), and the aspect ratio of the duct.
The goal is to analyze how these specific parameters affect the secondary flow structures and the axial flow characteristics within the rotating rectangular duct.
The research primarily employs the Spectral method, supported by Chebyshev polynomials, Collocation methods, and the Newton-Raphson iteration technique.
The results chapter focuses on presenting steady solution curves and visualizing secondary flow stream lines and axial flow contours across various operational ranges of Mg and Tr.
Key terms include Magnetohydrodynamics, Rotating Duct, Spectral Method, Vortex Solution, and Magnetic Parameter.
Higher magnetic parameters and large Taylor numbers tend to weaken the strength of fluid particles and often cause the maximum axial flow to transition into a ring-shaped profile.
The study identifies various vortex solutions, ranging from 2-vortex to 6-vortex structures, depending on the specific combination of magnetic, rotational, and flow parameters.
Der GRIN Verlag hat sich seit 1998 auf die Veröffentlichung akademischer eBooks und Bücher spezialisiert. Der GRIN Verlag steht damit als erstes Unternehmen für User Generated Quality Content. Die Verlagsseiten GRIN.com, Hausarbeiten.de und Diplomarbeiten24 bieten für Hochschullehrer, Absolventen und Studenten die ideale Plattform, wissenschaftliche Texte wie Hausarbeiten, Referate, Bachelorarbeiten, Masterarbeiten, Diplomarbeiten, Dissertationen und wissenschaftliche Aufsätze einem breiten Publikum zu präsentieren.
Kostenfreie Veröffentlichung: Hausarbeit, Bachelorarbeit, Diplomarbeit, Dissertation, Masterarbeit, Interpretation oder Referat jetzt veröffentlichen!

