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Program Structure
TMBW-2014 consists of keynote and invited lectures by international experts,
contributed talks and poster presentations by participants, and round
table discussions.
I. Key-note and invited lectures, and contributed talks
II. Poster presentations by participants
III. Round tables and open discussions
Focused topics of TMBW-2014 are:
- Interfacial Dynamics and Hydrodynamic instabilities (INT): instabilities of Rayleigh-Taylor, Kelvin-Helmholtz,
Richtmyer-Meshkov, Landau-Darrieus, Saffman-Taylor; formation and evolution of phase boundaries, interfacial mixing.
- Turbulence and Mixing (TURB): canonical and non-canonical turbulence, convection, rotating fluids, reactive and supersonic flows, active and passive scalar mixing.
- High Energy Density Physics (HEDP): inertial
confinement, magnetic and heavy-ion fusion, Z-pinches, light-material and
laser-plasma interaction, non-equilibrium heat transfer, material science, astrophysical applications.
Topics of Program "Turbulent Mixing and Beyond" include:
- Turbulence and Mixing (TURB): invariant, scaling, spectral properties, scalar transports, convection
- Wall-Bounded Flows (WALLS):
structure and fundamentals, non-canonical turbulent boundary layers,
including unsteady and transitional flows, supersonic and hypersonic
flows, shock-boundary layer interactions
- Non-Equilibrium Processes (NON): unsteady, multiphase and shock-driven
turbulent flows,
anisotropic non-local dynamics, connection of continuous description at
macro-scales to kinetic processes at atomistic scales
- Interfacial Dynamics (INT): the instabilities of Rayleigh-Taylor, Kelvin-Helmholtz,
Richtmyer-Meshkov, Landau-Darrieus, Saffman-Taylor
- High Energy Density Physics (HEDP): inertial
confinement and heavy-ion fusion, Z-pinches, light-material and
laser-plasma interaction, non-equilibrium heat transfer
- Material Science (MS): material transformation under high strain rates, equation of
state, impact dynamics, mixing at nano- and micro-scales
- Astrophysics (AST): supernovae, interstellar medium, star formation, stellar interiors,
early Universe, cosmic-microwave background, accretion disks
- Magneto-hydrodynamics (MHD): magnetic
fusion and magnetically confined plasmas, magneto-convection, magneto-rotational
instability, dynamo
- Canonical Plasmas (PLA): coupled plasmas, anomalous resistance, ionosphere
- Physics of Atmosphere (ATM): environmental fluid dynamics, forecasting, turbulent flows in stratified media and atmosphere
- Geophysics and Earth Science (GEO): mantle-lithosphere tectonics, oceanography,
turbulent convection under rotation, planetary interiors
- Combustion (COMB): dynamics
of flames and fires, deflagration-to-detonation transition, blast waves and
explosions, flows with chemical reactions, reactive flows in jet engines
- Mathematical Aspects of Non-Equilibrium Dynamics (MATH): vortex dynamics, singularities, discontinuities,
asymptotic dynamics, weak solutions, well- and ill-posedness, continuous transports
out of thermodynamic equilibrium
- Stochastic Processes and Probabilistic Description (STO): long-tail distributions and anomalous diffusion, data
assimilation and processing methodologies, error estimate and uncertainty
quantification, statistically unsteady processes
- Advanced Numerical Simulations (NUM): continuous DNS/LES/RANS, Molecular dynamics,
Monte-Carlo, predictive modeling, validation and verification of numerical
models
- Experimental Diagnostics (EXP): model experiments in high energy density and low
energy density regimes, plasma diagnostics, fluid flow visualizations and
control, opto-fluidics, novel optical method, holography, advanced technologies
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