2,274 research outputs found

    Bounds on solutions of the rotating, stratified, incompressible, non-hydrostatic, three-dimensional Boussinesq equations

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    We study the three-dimensional, incompressible, non-hydrostatic Boussinesq fluid equations, which are applicable to the dynamics of the oceans and atmosphere. These equations describe the interplay between velocity and buoyancy in a rotating frame. A hierarchy of dynamical variables is introduced whose members Ωm(t)\Omega_{m}(t) (1m<1 \leq m < \infty) are made up from the respective sum of the L2mL^{2m}-norms of vorticity and the density gradient. Each Ωm(t)\Omega_{m}(t) has a lower bound in terms of the inverse Rossby number, Ro1Ro^{-1}, that turns out to be crucial to the argument. For convenience, the Ωm\Omega_{m} are also scaled into a new set of variables Dm(t)D_{m}(t). By assuming the existence and uniqueness of solutions, conditional upper bounds are found on the Dm(t)D_{m}(t) in terms of Ro1Ro^{-1} and the Reynolds number ReRe. These upper bounds vary across bands in the {D1,Dm}\{D_{1},\,D_{m}\} phase plane. The boundaries of these bands depend subtly upon Ro1Ro^{-1}, ReRe, and the inverse Froude number Fr1Fr^{-1}. For example, solutions in the lower band conditionally live in an absorbing ball in which the maximum value of Ω1\Omega_{1} deviates from Re3/4Re^{3/4} as a function of Ro1,ReRo^{-1},\,Re and Fr1Fr^{-1}.Comment: 24 pages, 3 figures and 1 tabl

    The role of BKM-type theorems in 3D3D Euler, Navier-Stokes and Cahn-Hilliard-Navier-Stokes analysis

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    The Beale-Kato-Majda theorem contains a single criterion that controls the behaviour of solutions of the 3D3D incompressible Euler equations. Versions of this theorem are discussed in terms of the regularity issues surrounding the 3D3D incompressible Euler and Navier-Stokes equations together with a phase-field model for the statistical mechanics of binary mixtures called the 3D3D Cahn-Hilliard-Navier-Stokes (CHNS) equations. A theorem of BKM-type is established for the CHNS equations for the full parameter range. Moreover, for this latter set, it is shown that there exists a Reynolds number and a bound on the energy-dissipation rate that, remarkably, reproduces the Re3/4Re^{3/4} upper bound on the inverse Kolmogorov length normally associated with the Navier-Stokes equations alone. An alternative length-scale is introduced and discussed, together with a set of pseudo-spectral computations on a 1283128^{3} grid.Comment: 3 figures and 3 table

    Conditional regularity of solutions of the three dimensional Navier-Stokes equations and implications for intermittency

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    Two unusual time-integral conditional regularity results are presented for the three-dimensional Navier-Stokes equations. The ideas are based on L2mL^{2m}-norms of the vorticity, denoted by Ωm(t)\Omega_{m}(t), and particularly on Dm=ΩmαmD_{m} = \Omega_{m}^{\alpha_{m}}, where αm=2m/(4m3)\alpha_{m} = 2m/(4m-3) for m1m\geq 1. The first result, more appropriate for the unforced case, can be stated simply : if there exists an 1m<1\leq m < \infty for which the integral condition is satisfied (Zm=Dm+1/DmZ_{m}=D_{m+1}/D_{m}) 0tln(1+Zmc4,m)dτ0 \int_{0}^{t}\ln (\frac{1 + Z_{m}}{c_{4,m}}) d\tau \geq 0 then no singularity can occur on [0,t][0, t]. The constant c4,m2c_{4,m} \searrow 2 for large mm. Secondly, for the forced case, by imposing a critical \textit{lower} bound on 0tDmdτ\int_{0}^{t}D_{m} d\tau, no singularity can occur in Dm(t)D_{m}(t) for \textit{large} initial data. Movement across this critical lower bound shows how solutions can behave intermittently, in analogy with a relaxation oscillator. Potential singularities that drive 0tDmdτ\int_{0}^{t}D_{m} d\tau over this critical value can be ruled out whereas other types cannot.Comment: A frequency was missing in the definition of D_{m} in (I5) v3. 11 pages, 1 figur

    The 3D incompressible Euler equations with a passive scalar: a road to blow-up?

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    The 3D incompressible Euler equations with a passive scalar θ\theta are considered in a smooth domain ΩR3\Omega\subset \mathbb{R}^{3} with no-normal-flow boundary conditions \bu\cdot\bhn|_{\partial\Omega} = 0. It is shown that smooth solutions blow up in a finite time if a null (zero) point develops in the vector \bB = \nabla q\times\nabla\theta, provided \bB has no null points initially\,: \bom = \mbox{curl}\,\bu is the vorticity and q = \bom\cdot\nabla\theta is a potential vorticity. The presence of the passive scalar concentration θ\theta is an essential component of this criterion in detecting the formation of a singularity. The problem is discussed in the light of a kinematic result by Graham and Henyey (2000) on the non-existence of Clebsch potentials in the neighbourhood of null points.Comment: 5 pages, no figure

    Knowledge development for organic systems: An example of weed management

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    Despite the large amount information on weed biology and specific weed control measures produced by researchers, organic farmers still prioritise weeds as an important area for further research. A recent project investigating weed management in organic farming systems has established that knowledge and learning are key requirements for this to be effective. Development of relevant, practically useful knowledge depends on access to information generated ‘scientifically’ by researchers and also to knowledge generated as a result of farmer experience with weeds. This requires that farmers, advisors and researchers take a participatory approach to collecting and processing information on weed management, using it to develop new and relevant knowledge. The appropriate framework for knowledge development is thus a collegiate one in which all stakeholders’ value and learn from the observations and experience of others. These findings have implications for the way in which research is conducted and funded

    Lagrangian analysis of alignment dynamics for isentropic compressible magnetohydrodynamics

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    After a review of the isentropic compressible magnetohydrodynamics (ICMHD) equations, a quaternionic framework for studying the alignment dynamics of a general fluid flow is explained and applied to the ICMHD equations.Comment: 12 pages, 2 figures, submitted to a Focus Issue of New Journal of Physics on "Magnetohydrodynamics and the Dynamo Problem" J-F Pinton, A Pouquet, E Dormy and S Cowley, editor
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