Abstract
Patchiness plays a fundamental role in phytoplankton ecology by dictating the rate at which individual cells encounter each other and their predators. The distribution of motile phytoplankton species is often considerably more patchy than that of nonmotile species at submetre length scales, yet the mechanism generating this patchiness has remained unknown. Here we show that strong patchiness at small scales occurs when motile phytoplankton are exposed to turbulent flow. We demonstrate experimentally that Heterosigma akashiwo forms striking patches within individual vortices and prove with a mathematical model that this patchiness results from the coupling between motility and shear. When implemented within a direct numerical simulation of turbulence, the model reveals that cell motility can prevail over turbulent dispersion to create strong fractal patchiness, where local phytoplankton concentrations are increased more than 10fold. This ‘unmixing’ mechanism likely enhances ecological interactions in the plankton and offers mechanistic insights into how turbulence intensity impacts ecosystem productivity.
Introduction
Patchiness in the distribution of phytoplankton has long intrigued fishermen and scientists alike, because it generates hotspots of organisms at higher trophic levels^{1,2} and modulates species diversity^{3}, rates of fish recruitment^{4} and population stability^{5}. While phytoplankton patchiness at large spatial scales is driven by reproduction, growth is too slow to generate structure at scales 1 km visàvis the homogenizing effect of turbulence^{6,7}. Below this bottleneck scale, patchiness generated by locally enhanced growth is transferred to progressively smaller scales by turbulent stirring.
Whereas traditional plankton sampling techniques that utilize nets and bottles average over scales of metres, new technologies, including highresolution fluorometers^{8,9}, underwater imaging^{10,11} and syringe arrays^{12}, offer vastly improved resolution of plankton distributions, and have revealed that the microscale (~1–10 cm) distribution of motile phytoplankton species (for example, dinoflagellates) is often considerably more patchy than the distribution of nonmotile species (for example, diatoms)^{10,11,12}. However, the mechanisms that underlie this observation have remained elusive. Here we show that phytoplankton motility, when occurring in a turbulent flow, generates intense patchiness, far exceeding that of randomly distributed, nonmotile populations.
Results
H. akashiwo motility within a steady vortex flow
Following the tradition of using a vortical flow as a first proxy for smallscale turbulence^{13}, we exposed the motile, harmful algal bloom forming phytoplankter H. akashiwo to a steady vortex pair created via cavity flow (Fig. 1a; Methods). Video microscopy revealed that motile cells formed dense patches (Fig 1c, Supplementary Movie 1). In addition to swimming into downwelling regions, as previously predicted^{14,15} and observed in pipe flow^{16}, they accumulated inside the vortices’ cores, showing that individual vortices can trigger striking patches of motile phytoplankton. In contrast, killed cells remained randomly distributed (Supplementary Fig. S2), demonstrating that motility was an essential ingredient of patchiness.
Motility is a pervasive trait of phytoplankton. For example, 90% of species forming harmful algal blooms can swim^{17}. Motility allows cells to reside near the surface during daylight hours to enhance light acquisition while accessing deeper waters with more nutrients and lower predation risk at night^{18,19}. To migrate through the water column, many species rely on a stabilizing torque that biases their swimming in the vertical direction^{20,21}. This stabilizing torque competes with the viscous torque exerted on cells by fluid shear (specifically, the spatial gradients in fluid velocity that contribute to vorticity), which acts to overturn cells. The resulting directed motility is termed gyrotaxis, and the gyrotactic reorientation timescale, B—the characteristic time a perturbed cell takes to return to its vertical equilibrium orientation, k—provides a measure of how unstable the cell is to shear^{20,21,22}.
Gyrotactic motility within simulated flow fields
The hypothesis that the observed patchiness (Fig. 1c) originated from the coupling of motility and the shear in the vortical flow is strongly supported by a mathematical model of gyrotactic motility^{21} (Methods). When parameterized with the measured swimming properties of H. akashiwo, this model yields cell distributions in close agreement with experiments (Fig. 1c; Supplementary Fig. S4; Supplementary Movies 1 and 2). However, will patches of cells also occur in turbulent flow, where individual vortices are shortlived and the action of many vortices tends to disperse patchiness? To find out, we seeded a direct numerical simulation (DNS) of isotropic, homogeneous turbulence with up to 3.2 × 10^{6} cells, whose motility was governed by the same model of gyrotaxis, and followed their trajectories until their spatial distribution reached a statistical steady state (Methods). We found that turbulence drives intense patchiness in the distribution of motile phytoplankton (Fig. 2b; Supplementary Movie 3), whereas nonmotile cells follow the flow and remain randomly distributed (Fig. 2a).
While marine turbulence is comprised of fluid motion at many scales, phytoplankton cells (~1–100 μm) only experience the shear from small scales where fluid viscosity dissipates energy. The characteristic size and shear rate of these dissipative scales are proportional to the Kolmogorov length scale, η_{K}=(ν^{3}/ε)^{1/4}~0.1–10 mm, and Kolmogorov shear rate, ω_{K}=(ε/ν)^{1/2}~0.01–10 s^{−1}, respectively, where ν is the kinematic viscosity of seawater and ε the rate at which turbulent energy is dissipated^{23,24,25}. Two dimensionless parameters then control the cells’ fate: the swimming number, Φ=V_{C}/V_{K}, measuring the swimming speed V_{C} relative to characteristic smallscale fluid velocities V_{K}=η_{K}ω_{K}=(νε)^{1/4} (the Kolmogorov velocity), and the stability number, Ψ=Bω_{K}, measuring how unstable upward swimming cells are to overturning by shear. We note that while most turbulent energy is dissipated by fluid motion with length scales larger than η_{K} (ref. 23) the Kolmogorov scales remain the appropriate parameters for dimensionless analysis (Supplementary Fig. S8; Supplementary Methods).
Through coupling with turbulence, motility can increase local cell concentrations by one or more orders of magnitude. To quantify local cell concentrations, we used a threedimensional Voronoi tessellation^{26} (Fig. 2d; Supplementary Methods). The fraction f of cells having the largest local concentration were defined as patches and used to compute the patch concentration enhancement factor, Q=(C—C_{P})/C_{M}, where C is the mean cell concentration within patches, C_{P} is its counterpart for a random (that is, nonmotile) distribution of cells (which also harbours fluctuations in cell concentration), and C_{M} is the overall cell concentration. Thus, Q is a dimensionless measure of the increase in the local cell concentration due to motility. We found that motility can profoundly affect patch intensity. For example, the 10% most aggregated motile cells (f=0.1) for Ψ=1 and Φ=2.68 were nearly 10 times (Q=8) more concentrated than the 10% most aggregated nonmotile cells (Fig. 2e). For the 1% most aggregated cells (f=0.01), the enhancement is >50fold (Q=51). As patches are continuously born by motility and killed by turbulent dispersion, each cell transiently samples regions with high concentrations of conspecifics, on average spending a fraction of time f in regions where the local concentration is Qfold larger than that of a random distribution.
The patchiness intensity depends on both phytoplankton physiology and environmental conditions. Fast swimming cells (large Φ) with intermediate stability (Ψ~1) form the most concentrated patches (Fig. 2f). Owing to the incompressibility of the fluid, cells can form patches only if they swim across streamlines to converge within specific regions of the flow: they do so most effectively when their speed is large and their stabilizing torque strikes a balance between producing a swimming direction that is highly unstable and isotropic (Ψ>>1) and one that is very stable and uniformly upwards (Ψ<<1; Supplementary Fig. S9)^{22}.
Motilitydriven unmixing generates strong patchiness for conditions that commonly occur in the ocean. The reorientation timescale, while known only for a handful of species^{16,20,21,27,28,29}, generally spans the range B~1–10 s, which, for typical turbulent dissipation rates (ε=10^{−8}–10^{−6} m^{2} s^{−3}), corresponds to Ψ~1. Phytoplankton swimming speeds^{30,31}, V_{C}~100–1,000 μm s^{−1}, are often comparable to or larger than the Kolmogorov velocities, V_{K}~300–1,000 μm s^{−1}, associated with these dissipation rates, suggesting Φ can often be of order unity. Thus, we expect that phytoplankton routinely inhabit regions of the [Ψ, Φ] parameter space where patchiness is intense (Fig. 2f). Importantly, our results indicate that phytoplankton do not need to swim faster than the speed of largescale turbulent fluctuations to defy the homogenizing effect of turbulent dispersion, as previously suggested^{10}, they only need to swim at speeds comparable to Kolmogorov fluctuations.
Which feature of turbulence is responsible for patchiness? In contrast to steady vortical flow, where multiple mechanisms produce patches^{15}, in turbulent flow we found a consistent, strong correlation between cell location and downward flow velocity (Fig. 3d), suggesting that patchiness results from a dominant mechanism: cell focusing in local downwelling regions. This result generalizes previous observations of gyrotactic focusing in laminar downwelling flows^{21} and is rationalized by a theoretical analysis of the compressibility of the cell velocity field v=u+Φp (the superposition of flow velocity, u, and swimming velocity, Φp, where p is the swimming direction and all velocities are nondimensionalized by V_{K}). As v has nonvanishing divergence, (for Ψ<<1; where u_{z} is the vertical component of u; Methods), patches form () where ^{2}u_{z}>0, or equivalently in downwelling flow (u_{z}<0), because ^{2}u_{z} and u_{z} are negatively correlated (Supplementary Fig. S7; Methods). Both of these predictions are in good agreement with simulations (Fig. 3d; Supplementary Fig. S6), suggesting our analytical results offer a rational, mechanistic framework to interpret how motile phytoplankton form patches in disordered flows.
Motility substantially decreases the distance between neighbouring phytoplankton cells, altering the topology of their distribution. We found that the probability p(r) that a pair of cells reside less than a distance r from each other is enhanced for r<10η_{K} and this enhancement is >100fold for r<0.2η_{K} (for Ψ=0.68, Φ=3; Fig. 3a). For ε=10^{−6} m^{2} s^{−3} (η_{K}~1 mm), this translates to a >100fold increase in the probability that a conspecific resides within ~200 μm of a given cell. Whereas nonmotile cells are randomly distributed in threedimensional space, with p(r)~r^{3}, for motile cells we found that p(r)~r^{D} with D<3 (Fig. 3a), signifying that the cell distribution is not volumefilling, but instead occupies a lowerdimensional fractal set^{32}. Fractal clustering of particles in fluids is well known, for example in particles floating on fluid surfaces^{33} and water droplets in clouds^{34}, and arises as a consequence of an effective compressibility, which here stems from the ability of cells to swim across streamlines. Our analysis of the divergence of v correctly predicts the patchiness topology: weakly compressible flows are expected to produce particle distributions residing on a fractal set of codimension D=3 − a(ΨΦ)^{2}, where a is a constant and Ψ<<1 (Methods and Falkovich et al.^{34}). This relation successfully captured the behaviour of the fractal dimension D computed from simulations for Ψ<1 (Fig. 3c), confirming that the interaction of motility and turbulent flow results in an effective compressibility, which generates patchiness.
Discussion
Patchiness generated by motilitydriven unmixing may have a multitude of consequences for phytoplankton. On the one hand, patchiness may be advantageous during times of sexual reproduction, as it reduces distances between conspecific cells and could increase the local concentration of phytoplanktonexuded toxins that stifle competitors^{35}. On the other hand, patchiness could be detrimental because it sharpens competition for nutrients^{36} and enhances grazing by zooplankton^{37,38}, whose finely tuned foraging strategies allow them to retain their position within centimeterscale prey patches^{2}. The interaction of motility and turbulence could thus be an important determinant of the relative success of different phytoplankton species and provide a mechanistic basis to help decipher the powerful role turbulence is known to exert on plankton community composition^{39}.
Unlike passive mechanisms that generate patchiness, such as turbulent stirring, motilitydriven unmixing stems from active cell behaviour, opening the intriguing possibility that phytoplankton could regulate their smallscale spatial distribution by adaptively adjusting their position in [Ψ, Φ] space (Fig. 2f). Cells could regulate Φ by modulating swimming speed and Ψ by altering flagellar stroke^{20}, overall shape^{40} or chloroplast position^{41}. Individuals could then actively increase encounter rates with conspecifics, without need for chemical communication, by swimming faster and tuning stability such that Ψ~1, or minimize predation risk by slowing down and avoiding the intermediate stability regime. Regardless of whether this mechanism is adaptive or static, these results suggest that smallscale patchiness is a corollary of vertical phytoplankton migration, and that motilitydriven patch formation may thus be as common as the species that migrate through the water column. Future field and laboratory experiments may reveal the tradeoffs of directed motility in a turbulent ocean and how it shapes the fate of those at the bottom of the marine food web.
Methods
Phytoplankton culturing and preparation
H. akashiwo was grown by inoculating 2 ml of exponential phase culture into 25 ml of sterile f/2 medium, then incubating at 25 °C under continuous fluorescent illumination (70 μE m^{−2} s^{−1}) for 21 days. The culture used in experiments was prepared by diluting 75 ml of the 21day old culture with 500 ml of f/2 media to achieve a final cell concentration of ~2.5 × 10^{4} cells ml^{−1}. This concentration strikes a balance between maximizing the number of cells within the central plane (Fig. 1a, green box) and avoiding the bioconvective instabilities that arise when cell concentration exceeds a critical threshold^{21}. In control experiments (Supplementary Fig. S2), cells were killed using ethanol (10% v/v) before their introduction into the device.
Experimental vortex apparatus
Two counterrotating vortices were generated within a custommade transparent acrylic device (Fig. 1a and Supplementary Fig. S1). A 0.3 ml s^{−1} flow of a H. akashiwo culture was driven through each of the two vertical channels of the device using a syringe pump (Harvard Apparatus, PHD 2000) loaded with two syringes (Monoject, 140 ml). A random distribution of cells was initialized within the central cavity of the device (Fig. 1a, green box) by clamping one of the two flexible tubes (Cole Parmer CFlex, ID 3 mm) that convey flow to the device, which induced a unidirectional flow through the central cavity. Once the tube was unclamped, vortical flow was restored and the experiment began.
A laser sheet, generated using a continuous wave 8 mW HeliumNeon laser (Uniphase, model 1105 P) and a planoconcave cylindrical lens (Thorlabs, 20 mm focal length), illuminated cells along a 1.6mm thick central plane (−0.8 mm<y*<0.8 mm, where the asterisk denotes a dimensional variable) where the flow was nearly twodimensional due to symmetry. All images were captured at 20 Hz with a CCD (chargecoupled device) camera (PCO 1600, Cooke) attached to a dissecting microscope (SMZ1000, Nikon).
Simulations of gyrotaxis within the experimental flow field
To model the flow within the experimental device, we solved the threedimensional NavierStokes equations with the finite element software COMSOL Multiphysics (Burlington, MA), using the experimental device’s exact geometry and imposed flow rates. Gyrotactic motility was modelled by integrating the equation for the evolution of the swimming direction of a bottomheavy spherical cell^{21}
where p is the unit vector along the swimming direction, ω*=* × u* is the fluid vorticity, t* is time, k=[0,0,1] is a unit vector in the vertical upwards (+z*) direction, and B is the gyrotactic reorientation timescale, the characteristic time a perturbed cell takes to return to vertical if ω*=0. The first term on the right hand side describes the tendency of a cell to remain aligned along the vertical direction due to bottomheaviness, while the second term captures the tendency of vorticity to overturn a cell by imposing a viscous torque on it. We neglect the effect of cells on the flow. The cell position, X*=(x*, y*, z*), was computed by integrating the velocity resulting from the superposition of the swimming velocity, V_{C} p, and the flow velocity, u*:
Cell positions and swimming directions were initialized at random locations within the device and randomly on a unit sphere, respectively. Reflective boundary conditions were applied at all solid boundaries. The swimming speed, V_{C}, of each cell was drawn from a probability distribution obtained from H. akashiwo cells swimming within the central plane of the experimental device in the absence of flow. Cell trajectories were obtained from movies recorded at 20 Hz using automated software (PredictiveTracker; Ouellette et al.^{42}). To estimate the threedimensional swimming velocity from its measured (x*, z*) projection, we assumed isotropy in x* and y* to obtain V_{C}=(2v_{x}*^{2}+v_{z}*^{2})^{1/2} where v_{x}* and v_{z}* are the instantaneous cell swimming speeds in the x* and z* direction, respectively. The resulting probability density for the cell swimming speed has a mean of 75 μm s^{−1} (Supplementary Fig. S3). All 70,000 cells used in the simulation had a gyrotactic reorientation parameter of B=2 s, based on a previous estimate for H. akashiwo^{27}.
Simulations of gyrotaxis within isotropic turbulence
We solved the threedimensional NavierStokes equations in a fully periodic cubic domain of size L_{B}=2π with M mesh points using a pseudospectral method with a vector potential representation to ensure fluid incompressibility^{43}. To eliminate aliasing errors, we used the 2/3 dealiasing technique, which sets the largest 1/3 of all wave numbers to zero after each computation of the nonlinear terms in the NavierStokes equation^{44}, such that the largest resolved wavenumber is k_{max}=(1/3)M^{1/3}. Statistically stationary turbulence was sustained by applying homogeneous, isotropic, timeuncorrelated Gaussian forcing over a narrow shell of small wavenumbers^{45}, which produces integralscale fluid fluctuations (that is, the size L of the largest eddy) on the order of the domain size.
Once the velocity field had reached a statistical steady state, gyrotactic cells were initialized with random position in the domain and with orientations randomly distributed over the unit sphere. We seeded the simulation box with 300,000–3,200,000 cells depending on the Taylor Reynolds number Re_{λ} (Supplementary Table S1; Supplementary Methods). Cell trajectories were integrated using the nondimensional form of equations 1 and 2,
where time was nondimensionalized by 1/ω_{K}, lengths by the Kolmogorov length scale η_{K} and velocities by the Kolmogorov velocity V_{K}=ω_{K}η_{K}. Dimensionless parameters are Φ=V_{C}/V_{K} and Ψ=Bω_{K} (ω_{K} is the Kolmogorov vorticity scale). At each time step of the simulation, the local fluid flow properties (ω and u) at the particle locations were calculated using a trilinear interpolation from the computational mesh points.
Previous studies have demonstrated that the trajectories of passive tracer particles integrated via this numerical scheme accurately capture both the velocity^{46} and the acceleration^{47} statistics of the underlying DNSderived flow. Moreover, previous studies on clustering of inertial particles^{48} have demonstrated the efficacy of this method to resolve subKolmogorov scale fractal aggregations, which we also observed for gyrotactic swimmers.
All analyses were performed after cells had reached a statistically steady distribution, which requires ~30–50 Kolmogorov time scales (1/ω_{K}), corresponding in our simulations to 1–2 integral time scales (the characteristic timescale of the largest eddies in the flow).
Theoretical prediction of accumulation in downwelling regions
In general, the cell velocity field, v=u+Φp, and its divergence, ·v, depend on the history of the trajectory of individual cells and can only be calculated statistically. However, in the limit of a large stabilizing torque (Ψ<<1) the cell orientation quickly reaches equilibrium with the local fluid vorticity, such that v can be directly calculated using the instantaneous flow field. Assuming Ψ<<1, the solution to equation 3 is
to leading order in Ψ. This predicts that cells swim upwards with a deviation proportional to Ψ from the vertical. Imposing the incompressibility of the flow (·u=0) and applying the definition of vorticity, substitution of equation 5 into equation 4 yields
where u_{z} is the vertical component of fluid velocity, normalized by the Kolmogorov velocity, V_{K}. Equation 6 predicts that the cell velocity is compressible and that aggregations form in regions where ^{2}u_{z}>0. This prediction was confirmed in the DNS simulations by calculating ‹^{2}u_{z}›, defined as the mean of ^{2}u_{z} at the position of the cells (Supplementary Fig. S6). We found that ‹^{2}u_{z}› reaches a maximum for Ψ~1 and increases monotonically with Φ, which mirrors the dependence of the aggregation intensity on Ψ and Φ (Figs 2f and 3b; Supplementary Fig. S6), indicating that cells form patches in regions where ‹^{2}u_{z}› is large.
The prediction that cells collect where ^{2}u_{z}>0 generalizes prior observations that gyrotactic cells tend to collect in downwelling flows^{21}, because regions of the flow where ^{2}u_{z}>0 tend be highly correlated with regions of downwelling (u_{z}<0). This correlation can be demonstrated either by analysing the results from the DNS (Supplementary Fig. S7) or via theoretical analysis. The latter is briefly outlined here. By recasting the NavierStokes equations as an energy balance one can write^{25}
where all variables are dimensional (asterisks omitted for brevity), ε is the average energy dissipation rate and the last equality assumes isotropic flow. We can then rewrite the averaged quantity in the last term as:
where ‹^{2}u_{z}u_{z}=u› is a conditional average and P(u) is the probability density distribution of a single component of the flow velocity field at a fixed point, which for turbulent flows is well approximated by the following Gaussian distribution^{25}:
Using a closure theory that assumes homogeneous, isotropic turbulent flow^{49}, the conditional average in equation 8 can be approximated, to leading order, as
Equation 10 is obtained by using a linear approximation for the conditional average and substituting equation 9 into equation 8 and the result into equation 7 (ref. 49). The relation in equation 10, which shows good agreement with our simulations (Supplementary Fig. S7) predicts that, on average, regions with positive ^{2}u_{z} are correlated with downwelling flow (u_{z}<0), and vice versa.
These two predictions, that is, that cells collect where ^{2}u_{z}>0 and that ^{2}u_{z}~−u_{z}, taken together, indicate that an effective compressibility in the cell velocity field (produced by the cells’ motility) results in the formation of patches within downwelling regions, rationalizing the results from the turbulence simulations.
Theoretical prediction of D
In the previous section we showed that the cell's velocity field v has nonvanishing divergence in the limit of a strong stabilizing torque (Ψ<<1). In this limit, cells behave as passive tracers transported by a weakly compressible flow, v=u+δ w with ·w=−^{2}u_{z} and δ=ΨΦ (equation 6). It has been previously shown that tracers in weakly compressible flows (δ<<1) tend to form transient clusters of fractal codimension (3−D)∝δ^{2} (refs 34, 50, 51, 52). Thus for gyrotactic swimmers with Ψ<<1, the fractal dimension is predicted as
where a is a constant that depends on the flow. This result is in good agreement with our simulations for Ψ<1 (Fig. 3c).
Additional information
How to cite this article: Durham W. M. et al. Turbulence drives microscale patches of motile phytoplankton. Nat. Commun. 4:2148 doi: 10.1038/ncomms3148 (2013)
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Acknowledgements
We thank David Kulis and Donald Anderson for supplying H. akashiwo, Calcul en MidiPyrénées and Cineca Supercomputing Center for use of highperformance computational facilities, and Katharine Coyte, Kevin Foster, Nuno Oliveira and Jonas Schluter for comments on the manuscript. We acknowledge the support of the Human Frontier Science Program (to W.M.D.), MIUR PRIN2009PYYZM5 and EU COST Action MP0806 (to G.B., M.C. and F.D.), MIT MISTIFrance program (to E.C. and R.S.), and NSF grants OCE0744641CAREER and CBET1066566 (to R.S.).
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W.M.D., M.B. and R.S. were responsible for vortex experiments and simulations thereof, W.M.D., E.C., F.D.L., G.B., M.C. and R.S. performed and analysed DNS simulations, F.D.L., G.B. and M.C. developed analytical tools to interpret DNS simulations, W.M.D. and R.S. wrote the paper with input from all authors.
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Supplementary information
Supplementary Figures, Table, Methods and References.
Supplementary Figures S1S9, Supplementary Table S1, Supplementary Methods and Supplementary References. (PDF 830 kb)
Supplementary Movie 1
Phytoplankton motility in a steady vortex pair drives aggregations of cells. The toxic phytoplankton species Heterosigma akashiwo swimming within the central plane of the experimental device forms patches within the central downwelling region and within the vortex cores. The first still image shows cell trajectories collected over 1.5 s of the experiment. Nonmotile, killed cells did not form aggregations. The arrow denotes the direction of gravity. (MOV 3517 kb)
Supplementary Movie 2
A model of gyrotactic cell motility accurately captures the patterns of cell patchiness observed in experiments. An individualbased model of gyrotaxis embedded within a simulation of the experimental flow field shows agreement with patterns of cell patchiness observed in experiments (Supplementary Movie 1). The model was parameterized with measured motility parameters of H. akashiwo. The simulation was developed using the experimental device's exact geometry and imposed flow rates. The arrow denotes the direction of gravity. (MOV 7251 kb)
Supplementary Movie 3
Gyrotactic motility in turbulence unmixes the distribution of cells, forming intense patches. An isotropic, homogenous turbulent flow (Re? = 36) seeded with 104 cells whose trajectories are governed by the equations of gyrotaxis (with ?=0.6 and F=3), shows that an initially random distribution of motile cells rapidly forms patches, increasing the local cell concentrations by more than tenfold. Nonmotile cells remain randomly distributed. Time t is nondimensionalized by the Kolmogorov timescale 1/?K. The cells' preferred swimming direction, k, is vertically upwards. (MOV 8333 kb)
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Durham, W., Climent, E., Barry, M. et al. Turbulence drives microscale patches of motile phytoplankton. Nat Commun 4, 2148 (2013). https://doi.org/10.1038/ncomms3148
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DOI: https://doi.org/10.1038/ncomms3148
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