Publikationen

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Tympel, Saskia; Boeck, Thomas; Krasnov, Dmitry; Schumacher, Jörg
Vortex generation in a liquid metal duct flow near a magnetic dipole. - In: Proceedings in applied mathematics and mechanics, ISSN 1617-7061, Bd. 13 (2013), 1, S. 333-334

http://dx.doi.org/10.1002/pamm.201310162
Tympel, Saskia; Boeck, Thomas; Schumacher, Jörg
Laminar and transitional liquid metal duct flow near a magnetic point dipole. - In: Journal of fluid mechanics, ISSN 1469-7645, Bd. 735 (2013), S. 553-586

The flow transformation and the generation of vortex structures by a strong magnetic dipole field in a liquid metal duct flow is studied by means of three-dimensional direct numerical simulations. The dipole is considered as the paradigm for a magnetic obstacle which will deviate the streamlines due to Lorentz forces acting on the fluid elements. The duct is of square cross-section. The dipole is located above the top wall and is centred in spanwise direction. Our model uses the quasistatic approximation which is applicable in the limit of small magnetic Reynolds numbers. The analysis covers the stationary flow regime at small hydrodynamic Reynolds numbers Re as well as the transitional time-dependent regime at higher values which may generate a turbulent flow in the wake of the magnetic obstacle. We present a systematic study of these two basic flow regimes and their dependence on Re and on the Hartmann number Ha, a measure of the strength of the magnetic dipole field. Furthermore, three orientations of the dipole are compared: streamwise-, spanwise- and wall-normaloriented dipole axes. The most efficient generation of turbulence at a fixed distance above the duct follows for the spanwise orientation, which is caused by a certain configuration of Hartmann layers and reversed flow at the top plate. The enstrophy in the turbulent wake grows linearly with Ha which is connected with a dominance of the wall-normal derivative of the streamwise velocity.



http://dx.doi.org/10.1017/jfm.2013.491
Thess, André; Boeck, Thomas
Electromagnetic drag on a magnetic dipole interacting with a moving electrically conducting sphere. - In: IEEE transactions on magnetics, ISSN 1941-0069, Bd. 49.2013, 6, Pt. 2, S. 2847-2857

In this paper, we report an analytical study of the forces and torques acting upon a magnetic dipole interacting with a moving electrically conducting sphere. The work is motivated by the question whether Lorentz force velocimetry [Thess et al., Phys. Rev. Lett., vol. 96, 2006, 164501] - a noncontact flow measurement technique for liquid metals and electrolytes - can be applied to granular materials as well. We derive explicit expressions for all forces and torques for the case of low magnetic Reynolds number and small particle size. After a discussion of symmetry and reciprocity relations among the forces and torques, we apply the general theory to the particular cases of a translating (nonrotating) and rotating (nontranslating) sphere. The analysis for the purely translating sphere leads to the conclusion that the force is proportional to where is the radius of the sphere and is its minimum distance to the magnetic dipole. This result indicates that Lorentz force velocimetry can indeed be applied to granular metallic materials. The analysis for the purely rotating sphere leads to the result that the torque is proportional to. This result can be applied to derive a rigorous solution for a rotary Lorentz force flowmeter interacting with a rotating sphere. This solution implies that, contrary to intuitive expectation, a frictionless rotary Lorentz force flowmeter rotates with only 4/5 of the angular velocity of the sphere with which it interacts rather than undergoing synchronous rotation.



http://dx.doi.org/10.1109/TMAG.2012.2236565
Doumenc, Frederic; Chénier, E.; Trouette, B.; Boeck, Thomas; Delcarte, C.; Guerrier, Béatrice; Rossi, Maurice
Free convection in drying binary mixtures: solutal versus thermal instabilities. - In: International journal of heat and mass transfer, ISSN 1879-2189, Bd. 63 (2013), S. 336-350

Free convection occuring during the drying of plane layers of polymer solutions may be due to various mechanisms, based on buoyancy or Marangoni effect, of thermal or solutal origin. This theoretical and numerical work provides all the required tools to analyze thoroughly the problem. In this transient flow, different methods (frozen time, non-normal, nonlinear methods) are proposed to predict critical times for convection onset and threshold values for convection. Nonlinear and non-normal methods give similar results, within the uncertainty inherent to any transient problem. It is shown that, when linear stability analysis indicates the presence of several instability mechanisms, it is necessary to invoke nonlinear arguments to establish the leading mechanism. The proposed methodology is then applied to experimental results from the literature for two polymer solutions (Polyisobutylene/toluene and Polystyrene/toluene).



https://doi.org/10.1016/j.ijheatmasstransfer.2013.03.070
Pauluis, Olivier; Schumacher, Jörg
Radiation impacts on conditionally unstable moist convection. - In: Journal of the atmospheric sciences, ISSN 1520-0469, Bd. 70 (2013), 4, S. 1187-1203

The present work analyzes the impacts of radiative cooling in three-dimensional high-resolution direct numerical simulations of moist Rayleigh-Bénard convection. An atmospheric slab is destabilized by imposing a warm, moist lower boundary and a colder, dryer upper boundary. These boundary conditions are chosen such that the atmosphere is relaxed toward a conditionally unstable state in which unsaturated air parcels experience a stable stratification and unsaturated parcels experience an unstable one. Conditionally unstable moist Rayleigh-Bénard convection in the absence of radiative transfer produces self-aggregated convectively active cloudy regions separated by a quiescent unsaturated environment. Such convection is strongly limited by diffusion and is unable to transportmuch energy. As radiative cooling partially compensates for the adiabatic warming in the unsaturated environment and destabilizes the lower unsaturated boundary, its inclusion results in a significant enhancement of convective activity and cloud cover. A dry convectively unstable region develops at the lower boundary in a way that is reminiscent of the planetary boundary layer. Convective transport increases through the entire layer, leading to a significant enhancement of the upward transport of energy and water.



http://dx.doi.org/10.1175/JAS-D-12-0127.1
Kumar, Bipin; Schumacher, Jörg; Shaw, Raymond A.
Cloud microphysical effects of turbulent mixing and entrainment. - In: Theoretical and computational fluid dynamics, ISSN 1432-2250, Bd. 27 (2013), 3/4, S. 361-376

Turbulent mixing and entrainment at the boundary of a cloud is studied by means of direct numerical simulations that couple the Eulerian description of the turbulent velocity and water vapor fields with a Lagrangian ensemble of cloud water droplets that can grow and shrink by condensation and evaporation, respectively. The focus is on detailed analysis of the relaxation process of the droplet ensemble during the entrainment of subsaturated air, in particular the dependence on turbulence timescales, droplet number density, initial droplet radius and particle inertia. We find that the droplet evolution during the entrainment process is captured best by a phase relaxation time that is based on the droplet number density with respect to the entire simulation domain and the initial droplet radius. Even under conditions favoring homogeneous mixing, the probability density function of supersaturation at droplet locations exhibits initially strong negative skewness, consistent with droplets near the cloud boundary being suddenly mixed into clear air, but rapidly approaches a narrower, symmetric shape. The droplet size distribution, which is initialized as perfectly monodisperse, broadens and also becomes somewhat negatively skewed. Particle inertia and gravitational settling lead to a more rapid initial evaporation, but ultimately only to slight depletion of both tails of the droplet size distribution. The Reynolds number dependence of the mixing process remained weak over the parameter range studied, most probably due to the fact that the inhomogeneous mixing regime could not be fully accessed when phase relaxation times based on global number density are considered.



http://dx.doi.org/10.1007/s00162-012-0272-z
Tympel, Saskia; Krasnov, Dmitry; Boeck, Thomas; Schumacher, Jörg
Distortion of liquid metal flow in a square duct due to the influence of a magnetic point dipole. - In: Proceedings in applied mathematics and mechanics, ISSN 1617-7061, Bd. 12 (2012), 1, S. 567-568

We consider liquid metal flow in a square duct with electrically insulating walls under the influence of a magnetic point dipole using three-dimensional direct numerical simulations with a finite-difference method. The dipole acts as a magnetic obstacle. The Lorentz force on the magnet is sensitive to the velocity distribution that is influenced by the magnetic field. The flow transformation by an inhomogeneous local magnetic field is essential for obtaining velocity information from the measured forces. In this paper we present a numerical simulation of a spatially developing flow in a duct with laminar inflow and periodic boundary conditions.



http://dx.doi.org/10.1002/pamm.201210272
Kumar, Bipin; Janetzko, Florian; Schumacher, Jörg; Shaw, Raymond A.
Extreme responses of a coupled scalar-particle system during turbulent mixing. - In: New journal of physics, ISSN 1367-2630, Bd. 14 (2012), 115020, insges. 21 S.

https://doi.org/10.1088/1367-2630/14/11/115020
Emran, Mohammad Shah; Schumacher, Jörg
Conditional statistics of thermal dissipation rate in turbulent Rayleigh-Bénard convection. - In: The European physical journal. Soft matter. - Berlin : Springer, 2000- , ISSN: 1292-895X , ZDB-ID: 2004003-9, ISSN 1292-895X, Bd. 35.2012, 10, 35:108, insges. 8 S.

The statistical properties of the thermal dissipation rate in turbulent Rayleigh-Bénard convection in a cylindrical cell are studied by means of three-dimensional direct numerical simulations for a fixed Prandtl number Pr = 0.7 and aspect ratio = 1. The Rayleigh numbers Ra are between 107 and 3×1010. We apply a criterion that decomposes the cell volume into two disjoint subsets: the plume-dominated part and the turbulent background part. The plume-dominated set extends over the whole cell volume and is not confined to the boundary layers. It forms a complex spatial skeleton on which the heat is transported in the convection cell and its volume fraction decreases with increasing Rayleigh number. The latter finding holds also when the threshold, which separates both subvolumes, is varied. The Rayleigh number dependence of the mean moments and probability density functions of the thermal dissipation are analyzed on the subvolumes and related to other possible divisions of the convection volume, such as into boundary layer and bulk. The largest thermal dissipation events are always found in the plume-dominated subset.



http://dx.doi.org/10.1140/epje/i2012-12108-8
Tympel, Saskia; Boeck, Thomas; Krasnov, Dmitry; Schumacher, Jörg
Deflection of laminar liquid metal flow by a magnetic point dipole. - In: 23rd International Congress of Theoretical and Applied Mechanics, 2012, FM11-006, insges. 2 S.

We study distortion of laminar liquid metal flow by a magnetic point dipole in a straight square duct. This basic configuration is of fundamental interest for Lorentz force velocimetry, where the Lorentz force opposing the relative motion of conducting medium and magnetic field is measured to determine the flow velocity. The total force is highly dependent on the velocity profile, which changes its shape due to the acting Lorentz force itself. We are interested in the deflection of the flow and its dependence on magnitude and distribution of the magnetic field. To this end, we perform direct numerical simulations with an accurate finite-difference scheme in the limit of small magnetic Reynolds numbers. The hydrodynamic Reynolds number is choosen to be high enough to allow the generation of vortices and turbulent structures.