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Hydrodynamic problems

The tliree equation (A3,3,13). equation (A3,3,14) and equation (A3.3.15) are a usefiil starting point in many hydrodynamic problems. We now apply them to compute the density-density correlation fiinction... [Pg.723]

The column diameter is normally determined by selecting a superficial velocity for one (or both) of the phases. This velocity is intended to ensure proper mixing while avoiding hydrodynamic problems such as flooding, weeping, or entrainment. Once a superficial velocity is determined, the cross-sectional area of the column is obtained by dividing the volumetric flowrate by the velocity. [Pg.25]

The dependence of Vs on rheological parameters-shear stress on the wall and /notion coefficient — as far as the author knows, for filled polymers was not investigated somewhat completely, though its determination is necessary for a specific solution of hydrodynamic problems related to the flow of filled polymers. [Pg.88]

Certain hydrodynamical problems, as well as mass-transfer problems in the presence of surface-active agents, have been investigated theoretically under steady-state conditions (L3, L4, L10, R9). However, if we take into account the fact that in gas-liquid dispersions, the nonstationary term must appear in the equation of mass- or heat-transfer, it becomes apparent that an exact analysis is possible if a mixing-contacting mechanism is adopted instead of a theoretical streamline flow around a single bubble sphere. [Pg.362]

The constancy of the diffusion layer over the entire surface and thus the uniform current-density distribution are important features of rotating-disk electrodes. Electrodes of this kind are called electrodes with uniformly accessible surface. It is seen from the quantitative solution of the hydrodynamic problem (Levich, 1944) that for RDE to a first approximation... [Pg.66]

In consideration of the hydrodynamic problem alone, it is usually attempted to characterize the studied system by three quantities, the characteristic length / (e.g. the length of the plate in the direction of the flowing liquid or the radius of a rotating disk), the velocity of the flowing liquid outside the Prandtl layer V0 and the kinematic viscosity v. [Pg.152]

Physical properties of solutions Hydrodynamic problems and disturbance of the flow profile might appear when solutions with different properties, such as density or viscosity, are introduced into the manifold. [Pg.345]

The size, shape and charge of the solute, the size and shape of the organism, the position of the organism with respect to other cells (plankton, floes, biofilms), and the nature of the flow regime, are all important factors when describing solute fluxes in the presence of fluid motion. Unfortunately, the resolution of most hydrodynamics problems is extremely involved, and typically bioavailability problems under environmental conditions are in the range of problems for which analytical solutions are not available. For this reason, the mass transfer equation in the presence of fluid motion (equation (17), cf. equation (14)) is often simplified as [48] ... [Pg.456]

Flow and mass transfer the transport of the two phases through an extractor and the production of intensive phase contact are complex hydrodynamic problems. Mass transfer provides the main dimensions of the extractor. This chapter is chiefly interested in a suitable extractor design, but also in the restrictions of the calculation. [Pg.373]

SIN A Code for Computing One-Dimensional Reactive Hydrodynamic Problems", LASL Rept... [Pg.183]

DE - A Two-Dimensional Eulerian Hydro-dynamic Code for Computing One-Component Reactive Hydrodynamic Problems , Los Alamos Scientific Laboratory Report LA-3629-MS (1966) 23b) C.L. Mader, "FORTRAN-SIN - A One-Dimensional Hydrodynamic Code for Problems Which Include Chemical Reactions, Elastic-Plastic Flow, Spalling, and Phase Transitions , Los Alamos Scientific Laboratory Report LA-3720(1967) 24) R.C. Sprowls, "Com-... [Pg.184]

Items a and c are pure hydrodynamic problems d is much closer to a physical chemist. However, in the present article, we shall consider only problem b, treating it as a particular case of the general theory of new phase formation. [Pg.121]

It must be said that there are some hypothetical presumptions in this part of the theory, all originating in the simplified mathematical treatment of a complicated hydrodynamic problem. Nevertheless, these simplifications lead to reasonable results, as is shown below. [Pg.40]

Recently, Schwartz et al. [13-15], treated the nonlinear hydrodynamic problem involving large amplitude modulations of the angular velocity. [Pg.260]

Correct modeling of the flow near the front of a stream requires a rigorous solution of the hydrodynamic problem with rather complicated boundary conditions at the free surface. In computer modeling of the flow, the method of markers or cells can be used 124 however this method leads to considerable complication the model and a great expenditure of computer time. The model corresponds to the experimental data with acceptable accuracy if the front of the streamis assumed to be flat and the velocity distribution corresponds to fountain flow.125,126 The fountain effect greatly influences the distribution of residence times in a channel and consequently the properties of the reactive medium entering the mold. [Pg.81]

The solution of the hydrodynamic problem of boundary layer flow, excluding the effects of surface tension, requires simplification of the formulation this is achieved by introducing the flow function t /. Then the transition to a system of differential equations written for a new coordinate system (turn angle and flow function) can be made, and we can find the form of the free surface... [Pg.140]

Two additional parameters are the angular position of the point at which the film thickness is maximum, 0rot, and the ratio of the maximum thickness of the film to its mean thickness e. The zone of large Re and small Fr is shaded in Fig. 4.22 in the right bottom. The existence of circular closed flow lines proves to be impossible hence, a stable solution of the hydrodynamic problem is also impossible. The zone of quasi-solid rotation A is marked in the top left comer film flow is absent here and 1 < e < 1.01. This zone is reached either at Fr = const by decreasing Re (due to an increase in viscosity) or at Re = const by increasing Fr (through an increase in to). Two transient zones are marked with the numbers 1 and 2 in the lower unstable zone of Fig. 4.22. In zone 1, the... [Pg.141]

Let us analyze isothermal polymerization in a tubular reactor of finite length. The formulation of the hydrodynamic problem is based on some obvious assumptions ... [Pg.153]

The second approach is a fractional-step method we call asymptotic timestep-splitting. It is developed by consideration of the specific physics of the problem being solved. Stiffness in the governing equations can be handled "asymptotically" as well as implicitly. The individual terms, including those which lead to the stiff behavior, are solved as independently and accurately as possible. Examples of such methods include the Selected Asymptotic Integration Method (4,5) for kinetics problems and the asymptotic slow flow algorithm for hydrodynamic problems where the sound speed is so fast that the pressure is essentially constant (6, 2). ... [Pg.341]

For sufficiently large electrodes with a small vibration amplitude, aid < 1, a solution of the hydrodynamic problem is possible [58, 59]. As well as the periodic flow pattern, a steady secondary flow is induced as a consequence of the interaction of viscous and inertial effects in the boundary layer [13] as shown in Fig. 10.10. It is this flow which causes the enhancement of mass-transfer. The theory developed by Schlichting [13] and Jameson [58] applies when the time of oscillation, w l is small in comparison with the time taken for a species to diffuse across the hydrodynamic boundary layer (thickness SH= (v/a>)ln diffusion timescale 8h/D), i.e., when v/D t> 1. Re needs to be sufficiently high for the calculation to converge but sufficiently low such that the flow does not become turbulent. Experiment shows that, for large diameter wires (radius, r, — 1 cm), the condition is Re 2000. The solution Sh = 0.746Re1/2 Sc1/3(a/r)1/6, where Sh (the Sherwood number) = kmr/D and km is the mass-transfer coefficient,... [Pg.400]

From the usual plate-type distillation and absorption columns, it was but natural to attempt to devise stagewise equipment for G/S processing, for better heat economy and better utilization of the contacting media. But instability of the downcomer for solids transfer between stages remained for many years an unsolved hydrodynamic problem, and even to this data, the stable operation of many solids downcomers still depends on mechanical devices. [Pg.284]

The exact solution of the convection-diffusion equations is very complicated, since the theoretical treatments involve solving a hydrodynamic problem, i.e., the determination of the solution flow velocity profile by using the continuity equation or -> Navier-Stokes equation. For the calculation of a velocity profile the solution viscosity, densities, rotation rate or stirring rate, as well as the shape of the electrode should be considered. [Pg.114]

The jets seem to be launched in the central region of the objects, either by the star itself or by the disk surface close to the star and it is thought that magnetic fields are responsible for the collimation of the thin jets. The detailed processes underlying the phenomenon are not well understood because of the inherent difficulties of treating magneto-hydrodynamic problems. [Pg.59]

However, the hydrodynamic problem that Stokes solved to get F = 67cn/v pertains to a sphere moving in an incompressible continuum fluid. This is a far cry indeed from the actuality of an ion drifting inside a discontinuous electrolyte containing particles (solvent molecules, other ions, etc.) of about the same size as the ion. Furthermore, the ions considered may not be spherical. [Pg.453]

Stellar nucleosynthesis also needs continuing attention. The biggest remaining problem in theoretical stellar evolution and nucleosynthesis continues to be the treatment of convective mixing, which affects both structure and nucleosynthesis. This is also a hydrodynamical problem requiring improved computing power, and should provide a source of entertainment (and argument) for some time. [Pg.211]

The first particle moves toward the second immobile particle and rotates around the line of centers (see Figure 5.35a). This is an axisynunetric rotation problem (a two-dimensional hydrodynamic problem) which was solved by Jeffery and Stimson and Jeffery for two identical spheres moving with equal velocities along their line of centers. Cooley and 0 NeilF ° calculated the forces for two nonidentical spheres moving with the same speed in the same direction or, alternatively, moving toward each other. A combination of these results permits evaluation of the total forces and torques acting on the particles. [Pg.227]


See other pages where Hydrodynamic problems is mentioned: [Pg.708]    [Pg.335]    [Pg.507]    [Pg.713]    [Pg.34]    [Pg.152]    [Pg.133]    [Pg.130]    [Pg.128]    [Pg.423]    [Pg.34]    [Pg.187]    [Pg.51]    [Pg.98]    [Pg.18]    [Pg.1259]    [Pg.70]    [Pg.120]    [Pg.66]    [Pg.206]    [Pg.206]    [Pg.211]    [Pg.186]    [Pg.381]   
See also in sourсe #XX -- [ Pg.619 ]




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