Primary Production
Marine Microbial Ecology
Laminar and Turbulent Flow
Turbulent Flow
Freshwater Microbial Ecology
Diversity of Protists III
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Updated: Apr 5, 2026

Chemotactic Response of Marine Micro-Organisms to Micro-Scale Nutrient Layers
Published on: May 28, 2007
Itzhak Fouxon1,2, Alexander Leshansky1
1Department of Chemical Engineering, Technion, Haifa 32000, Israel.
This study explores how ocean turbulence affects the upward movement of phytoplankton. Using the Pedley-Kessler model, researchers simulate how spherical microorganisms interact with turbulent flow. They find that turbulence can either slightly perturb or completely randomize the upward drift of phytoplankton. In some cases, the drift is determined by local vorticity or follows a Gaussian distribution. The study identifies a parameter range where phytoplankton motion can be described as diffusion in an effective potential. Solving the Fokker-Planck equation reveals an exponential steady-state distribution of propulsion orientation. The researchers observe that phytoplankton concentrate on fractals with vertical stripes. The nonisotropic pair-correlation function indicates vertical clustering. The power law for particle distances suggests increased collision rates in turbulent conditions. The predictions are valid for Navier-Stokes turbulence and await experimental validation.
Area of Science:
Background:
Ocean turbulence influences the movement of microscopic organisms like phytoplankton. Prior research has shown that turbulence can affect the distribution of plankton, but the exact mechanisms remain unclear. It was already known that phytoplankton exhibit upward motion due to buoyancy and flagellar propulsion. However, the interaction between this motion and turbulent flow structures is not fully understood. This gap motivated researchers to explore how turbulence alters the orientation and movement of phytoplankton. No prior work had resolved how turbulence might either randomize or enhance the clustering of these organisms. Understanding this could help predict plankton distribution in the ocean. The study aims to clarify the conditions under which turbulence either disrupts or enhances phytoplankton motion. This uncertainty drives the need for a detailed model of phytoplankton dynamics in turbulent flows.
Purpose Of The Study:
The study aims to investigate how turbulence influences the upward motion of phytoplankton in the ocean. The specific problem is to determine whether turbulence enhances or disrupts the vertical movement of these organisms. The motivation comes from the need to understand how turbulence affects plankton distribution and collision rates. The researchers propose to model phytoplankton as spherical microorganisms interacting with turbulent flow. They aim to identify parameter ranges where turbulence either randomizes or enhances the upward drift. The study also seeks to determine how turbulence affects the spatial clustering of phytoplankton. The researchers propose to use the Pedley-Kessler model to describe the interaction with the flow. The goal is to predict the fractal dimensions and collision rates under different turbulence conditions.
Main Methods:
The researchers use the Pedley-Kessler model to describe phytoplankton interaction with turbulent flow. They simulate spherical microorganisms in a turbulent environment. The model considers the orientation and propulsion of phytoplankton. The study applies the Fokker-Planck equation to analyze orientation diffusion. They solve this equation to find the steady-state distribution of propulsion orientation. The model also incorporates an effective potential to describe orientation changes. The researchers calculate fractal dimensions of phytoplankton concentration patterns. They use the turbulent energy spectrum to predict collision rates and clustering behavior.
Main Results:
The study finds that turbulence can either weakly perturb or completely randomize the upward drift of phytoplankton. In some parameter ranges, the drift is determined by local vorticity or follows a Gaussian distribution. The researchers identify a parameter range where phytoplankton motion can be described as diffusion in an effective potential. Solving the Fokker-Planck equation yields an exponential steady-state distribution of propulsion orientation. They find that phytoplankton motion can be described by a smooth flow in certain conditions. In these cases, phytoplankton concentrate on fractals with vertical stripes. The pair-correlation function shows increased concentration in the vertical direction. The distance between particles follows a power law with a negative exponent determined by the turbulent energy spectrum.
Conclusions:
The study concludes that turbulence can either randomize or enhance the upward motion of phytoplankton. The authors propose that turbulence influences phytoplankton orientation through an effective potential. They find that phytoplankton motion can be modeled as diffusion in this potential. The exponential steady-state distribution of propulsion orientation supports this model. The researchers observe that phytoplankton concentrate on fractals with vertical stripes. The nonisotropic pair-correlation function indicates vertical clustering. The power law for particle distances suggests increased collision rates in turbulent conditions. The predictions are valid for Navier-Stokes turbulence and await experimental validation.
Turbulence can either weakly perturb or completely randomize the upward drift of phytoplankton. In some cases, the drift is determined by local vorticity or follows a Gaussian distribution.
The researchers use the Pedley-Kessler model to describe how spherical microorganisms interact with turbulent flow.
An effective potential is used when phytoplankton interaction with the flow can be consistently described as diffusion of orientation.
Solving the Fokker-Planck equation yields an exponential steady-state distribution of phytoplankton's propulsion orientation.
Turbulence leads to vertical clustering of phytoplankton, with a nonisotropic pair-correlation function and fractal dimensions.
The power law with a negative exponent indicates increased collision rates due to turbulence, with the exponent determined by the turbulent energy spectrum.