Dynamics of inertial and non-inertial particles in geophysical flows
Presentation Type
Poster
Faculty Advisor
Eric Forgoston
Access Type
Event
Start Date
26-4-2023 12:30 PM
End Date
26-4-2023 1:30 PM
Description
We consider the dynamics of inertial and non-inertial particles in a single-layer, quasi-geostrophic (QG) ocean model. We investigate the underlying structures of the flow field by examining their Lagrangian coherent structures (LCS) which are found by computing finite-time Lyapunov exponents (FTLE). We study the behavior of massless non-inertial particles using the fluid velocity fields from the QG model and compare it with the behavior of massless inertial particles in a double-gyre model, duffing oscillator, and bickley jet. For inertial particles with finite size and mass, we use the Maxey-Riley equation to describe the particle's motion, and compare the particles' behavior in a double-gyre flow, duffing oscillator, and bickley jet. We explore the preferential aggregation of inertial particles and demonstrate how particle clustering depends on the density ratio and the Stokes number.
Dynamics of inertial and non-inertial particles in geophysical flows
We consider the dynamics of inertial and non-inertial particles in a single-layer, quasi-geostrophic (QG) ocean model. We investigate the underlying structures of the flow field by examining their Lagrangian coherent structures (LCS) which are found by computing finite-time Lyapunov exponents (FTLE). We study the behavior of massless non-inertial particles using the fluid velocity fields from the QG model and compare it with the behavior of massless inertial particles in a double-gyre model, duffing oscillator, and bickley jet. For inertial particles with finite size and mass, we use the Maxey-Riley equation to describe the particle's motion, and compare the particles' behavior in a double-gyre flow, duffing oscillator, and bickley jet. We explore the preferential aggregation of inertial particles and demonstrate how particle clustering depends on the density ratio and the Stokes number.