Course Title: |
"Multi-Scale Fluid Dynamics: Physical Concepts" |
Course Number: |
ME7953 (X-listed as PHYS7233, MATH7999-n, PETE7241) |
Prerequisites: |
MATH2090 or MATH4027 or MATH2065+MATH2085; PHYS2102 or PHYS1202 |
Text(s) & Readings: |
- Karniadakis, Beskok & Aluru ()
" Microflows and Nonoflows "
- Probstein or Levich ()
" Physiochemical Hydrodynamics "
- Vogel / Childress /Lighthill ()
" Life in Moving Fluids / Mechanics of Swimming and Flying / Mathematical Biofluiddynamics "
- Kundu or Panton ()
" Fluid Mechanics "
- Gill or Pedlosky or Pond ()
" Dynamical Oceanography / Geophysical Fluid Dynamics "
- Battaner or Choudhuri ()
" Astrophysical Fluid Dynamics "
- Brenner and/or Oran/Boris ()
" Multiphase Flows / Reactive Flows "
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Description |
An introduction to fluid dynamics from a multi-disciplinary perspective. The first half of the course will emphasize how the principal concepts that underpin our understanding of fluid flows apply to a wide range of physical scales; the second half of the course will take the form of four separate, discipline-specific modules. Physical concepts initially will be presented without mathematics, using examples drawn from various disciplines. Then, the physical concepts will be expressed in mathematical terms to make them tangible for the solution of numerous problems. Example problems initially will be introduced on the simplest of levels and will be chosen so that they can be expanded upon and brought to a higher level (in terms of both formulation and solution method) during the second half of the course. The focus will be on problems with analytical or semi-analytical solutions, but close coordination with XD-II will allow extension to numerical solutions. |
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Schedule |
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"The Big Picture "
- Nature
- Conceptual Model
- Mathematical Formulation - Solution
- Prediction
- Understanding - Intervention
Definitions of Fundamental Physical Variables;
Properties of Materials;
Shake the dust off Mathematics (covered as needed)
- Scalars, Vectors, Tensors
- Symbolic and Indicial Notation
- Matrices & Determinants
- Tensor Transformations
- Eigenvalues and Eigenvectors
- Tensor Fields & Tensor Calculus
- Integral Theorems of Gauss and Stokes
|
Nikitopoulos |
Equilibrium;
The Continuum Concept/Hypothesis;
Body/Surface Forces;
Traction and Stress |
Nikitopoulos |
What Happens at Boundaries;
Kinematics of Deformation & Motion
- Deformation
- Motion and its Decomposition
|
Nikitopoulos |
Kinematics of Deformation & Motion (cont.)
- Material and Spatial Coordinates
- Lagrangian & Eulerian (Field) Descriptions
- Material Derivatives
- Deformation Rate
- Acceleration
- Vorticity
|
Nikitopoulos |
Conservation and Transport Processes (as seen from various disciplines)
- Mass
- Momentum - Moment of Momentum
- Energy
- Entropy - Dissipation
d p /dt = F eng + F ocean + F bio + F astro |
Nikitopoulos |
Conservation Laws and Transport Processes (continued)
- Formulations for Non-Inertial Frames
- Constitutive Equations (Closures)
- Auxiliary Relations
- Boundary Conditions
The Issue of Scales
- Dimensional Analysis
- Similarity
|
Nikitopoulos |
Biology Module (Part I: Internal Bio-Fluid-Mechanics)
- Laminar natural convection between vertical channels
- Flow through porous media: Derivation of Darcy's Law
- Flow through collapsible tubes
|
Lynn
Tyagi |
Biology Module (Part II: External Bio-Fluid-Mechanics)
- Creeping Flow
- Undulating Fibre (Lighthill's propulsion theory)
|
Lynn
Tyagi |
Engineering Module (Part I)
- Boundary Layer (Physical/Mathematical, Laminar/Turbulent)
- Burger's Problem (Non-linear, Smoothing of Discontinuities)
|
Nikitopoulos |
Engineering Module (Part II)
- Isentropic Compressible Flow (with Shock Waves?)
- Electrokinetic Flow
|
Nikitopoulos |
Oceanography Module (Part I)
- Thermohaline Circulation
- Shallow Water Theory
|
Rouse
Li |
Oceanography Module (Part II)
- Western Boundary Current Solutions
- Wind-Driven Circulation - Eckman Layers
|
Rouse
Li |
Astronomy Module (Part I)
- Hydrostatic Balance and the Structure of Stars
- The Gravitational Free-Fall Problem
|
Tohline |
Astronomy Module (Part II)
- Slow contraction of a star due to Radiative Losses
- The Roche potential for Binary stars in Circular Orbits
Conclude with a return to " The Big Picture " (Bring it all back together) |
Tohline |