Theoretical considerations on ultrasound assisted atomization of fluid sheets

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1 Theoretical considerations on ultround sisted atomization of fluid sheets B. Heislbetz DLR - German Aerospace Center, Space Propulsion Institute D-7439 Hardthausen, Germany Abstract We present theoretical investigations about the mechanism of ultround sisted atomization of liquid sheets. Therefore a linear stability analysis of a free fluid sheet influenced by an external, harmonically modulated excitation, in the presence of a geous atmosphere, is conducted. The treatment of the hydrodynamic problem for Euler fluids shows that the temporal evolution of the free sheet surfaces can be described by a set of two coupled differential equations with time dependent coefficients. To reach physical relevance and obtain a more realistic fluid characterization, dissipation effects are included. The derived equations were analyzed both analytically by means of the multiple scale perturbation method and by numerical calculations. Introduction Atomization, the disintegration of a bul liquid into fine, preferably monodisperse droplets and the sociated mechanisms of surface magnification, is widely used for the combustion in liquid fuel rocet propulsions, diesel engines or g turbines. It is also used in many industrial applications lie spray drying, metall powder, mirco- and nano-particle production or spray coating well to produce and deliver agent loaded aerosoles for medical or agricultural usage. The brea-up mechanisms and disintegration processes of liquid ets and sheets usually build up by ducts, narrow slits or impinging ets have been analysed i.e. by Taylor 11], Li & Tanin 6], Lin 7] and several other researchers. As a result, the bic brea-up mechanism and thus the droplet sizes are inherently dependent both on the fluid properties and the experimental given flow rates and geometrical specifications. This narrows for a present experimental setup the possibilities on flexible control of the droplet diameter only on variation of the liquid or geous flow rates. Hence ultround devices are used to affect the disintegration process independent of geous or liquid flow rates by means of an external excitation. Several experimental investigations well numerical aproaches using CFD (see for example 1], 1], 5]), have been conducted showing that a destabilization of oscillatory wave modes on the liquid sheet surfaces is excited, which initialize sheet brea up Corresponding author: bernhard.heislbetz@dlr.de Proceedings of the 1 th ILASS-Europe Meeting 7 processes, due to high frequency forcing. And thus, the formation of ligaments and droplets is directly influenceable by an external excitation. In spite of the wide variety of applications and advantages of these atomization method, the bic physical mechanism and principles of the brea-up process have not been investigated sufficiently up to now. In order to have a better understanding of the ultround sisted fluid atomization, the stability of a free liquid sheet in the presence of a harmonic modulated external forcing is investigated analytically. The Hydrodynamic System We consider a layer of a ideal, immiscible and incompressible fluid with an undisturbed thicness H = h which is surrounded by an sumed ideal, immiscible and incompressible geous atmosphere. A surface tension σ act between the fluid layer and the geous ambiente. The fluids were externally forced due to high frequency time variing gravitational or pressure fields in direction perpendicular to the fluid interfaces. Fig. 1.,. show the schematic setup of the considered problem. Starting from the bic hydrodynamic equations, the dynamic of the fluid bul is governed by ρ i t + u ]u i = Π i (x,t) (1) where the velocity field u have to fullfill the continuity equation u i =. ()

2 The subscript i = 1, denotes the respective liquid or geous fluid layers. The value ρ i represents the density of the fluids, where Π denotes body forces generated by a external, time variing gravitational or pressure field. Below, we don t have to distinguish between modulated pressure or gravity fields, because both act volumina forces. Thus we choose without loss of generality a time variing gravity field, where the ce of a modulated pressure field can be treaten in the same way. The dynamic of the interfaces η (x,t); = 1,, which seperate the fluid layers, is governed by the inematic surface condition D Dt η (x,t) = t η + u η =. (3) We eliminate the horizontal velocity in Eq.(1) by multiplying with e z and performing a transformation into a frame of reference that moves with the external forcing. Thus in Eq. (1) the explicite time dependence drops out. z h h Π(t) η η Undisturbed liquid sheet 1 Liquid sheet surfaces Figure 1. Setch of a symmetrical wave mode. Initially the liquid layer h a undisturbed thicness H = h, where the surfaces are located at z = ±h. z h η h Π(t) η Undisturbed liquid sheet Figure. Antisymmetrical wave mode. Boundary Conditions 1 Liquid sheet surfaces Assuming that the fluid layers initially are stationary and seperated by flat interfaces, we have to regard several interfacial boundary conditions. Introducing the notation X X i X η (4) x x which denotes the ump of the value X at the -th interface seperating the fluids i and, at the interfacial boundaries the velocity h to be continuous u = (5) and the umps of the normal stresses are balanced by surface tension ρ t u + ρfw(t) = σ 4 η. (6) Here we have to remar that the boundary conditions for the normal stresses become explicitly time dependent, due to the transformation into a new frame of reference. Linear Evolution Equations In the comoving frame of reference we have initially no fluid movement, a constant hydrostatic pressure and interfaces between the fluid layers with a plane geometry. In order to analyse the stability of the bic state, we linearize the hydrodynamic equations well the boundary conditions around the bic solutions u = η i =. It can be shown that after linearization the horizontal and vertical flow fields decouple. In consequence of the fact that in linear regime the temporal evolution of the fluid interfaces (3) is only affected by the vertical flow field, we can separate flows and consider only fluid movements in z-direction: t ( zz )w 1 =,h z (7) t ( zz )w =, h z h (8) t ( zz )w 3 =, z h, (9) where w i is the vertical velocity in the fluid layer i and the wave number. Due to the requirement that the surrounding fluid layers are of infinit high, it is sumed that the velocity field in the outer sheets tends to zero for z ±, thus the solution of Eq. (7) - (9) can be expressed w 1 (z,t) = A(t)exp( z) (1) w (z,t) = B(t)sinh(z) + C(t)cosh(z) (11) w 3 (z,t) = D(t)exp(z). (1) After determine the unnown time dependent functions A(t), B(t), C(t), D(t) by means of the linearized interfacial boundary conditions (5), (6) and inetic surface condition (3) we obtain, introducing symmetric and antisymmetric modes of the interface deformations, denoted η s (t), η a (t) and given by η s (t) = η 1 (t) η (t) (13) η a (t) = η 1 (t) + η (t), (14)

3 a system ooupled differential equations with time variing coefficients: t η s (t) = T s ση s (t) ρfw(t)η a (t) ] (15) t η a (t) = T a ση a (t) ρfw(t)η s (t) ], (16) where we use T a = /coth(h),t s = coth(h) and ρ = ρ 1 ρ abbreviations. Phenomenological Incorporation of Viscous Damping The movement of a real fluid leads always to energy dissipation due to the fluids viscosity. In ces of a small viscous dissipation and under the condition that the velocities are not too large, one can calculate a damping coefficient 4] by considering the ratios of the averaged inetic energy E in and the sociated averaged temporal dissipation rate t E in, where t E in = ρ i ν i ( i u ) dv (17) and E in = ρ i u dv (18) hold. By means of the solutions (1) - (1) a damping coefficient can be determined γ = 1 t E in = ν. (19) E in To simplify matters, we have only considered the properties of the fluid sheet, because its density well its viscosity is at let up to orders of magnitude higher than the values of the geous atmosphere and hence have a bigger influence on the damping. After incorporation of the derived damping coefficient in the differential equation system (15), (16) the temporal evolution equations for external forced wea viscous fluids read ( t + γ a ) t η a = () αη a ρg(1 + fw(t))η s] T a ( t + γ s ) t η s = (1) αη s ρg(1 + fw(t))η a] T s Analytical treatment The derived evolution equations (15), (16) well (), () can not be solved in general. Thus a approximate analytical method is used. Assuming that the amplitude of the external forcing is sufficient small, we follow Nayfeh and Moo 9] and Mohammed et al. 8], to obtain ymptotic expressions to determine the stability of the given problem, using the method of multiple time scales. Introducing a smallness parameter ǫ, we can define different time scales given by T n = ǫ n t, n =,1,..., () where the time derivative operators can be expressed d dt = D + ǫd ; and Dl = / Tl hold. Rewriting equations (15), (16) d dt = D + ǫd D (3) ( t + α 11 )η a + (α 1 + ǫf 1 W(t))η s = (4) ( t + α )η s + (α 1 + ǫf 1 W(t))η a = (5) and sume that the solutions of the system (4), (5) may be expanded in the form η a,s (t,ǫ) = η a,s (T,T 1 ) + ǫη a,s 1 (T,T 1 ) +... (6) we substitute (6), () and (3), into (4), (5) and equating lie powers of ǫ. Thus we find in lowest order (D + α 11 )η a + α 1 η s = (7) (D + α )η s + α 1 η a =. (8) The solutions of (7), (8) can be sought in the form η a = η s = α 1 A (T 1 )e iωt + cc (9) (ω α 1 )A (T 1 )e iωt + cc, (3) where the unnown A is a complex, slow variing amplitude and cc is the abbreviation of the complex conugate expressions of the preceding terms. For solvability the frequencies ω, = 1, have to fullfill the relation ω 1 = α 11 + α and ω = α 11 + α + (α11 α ) + 4α 1 α 1 ] 1 (α11 α ) + 4α 1 α 1 ] 1, (31). (3) Substituting the solutions (9), (3) into the first order expansion of the system, given by (D + α 11 )η a 1 + α 1 η s 1 = (33) D D 1 η a + f 1 W(T )η s (D + α )η s 1 + α 1 η a 1 = (34) D D 1 η s + f 1 W(T )η a, 3

4 we choose η a 1 = η s 1 = α 1 B (T 1 )e iωt + cc (35) (ω α 1 )B (T 1 )e iωt + cc, (36) solutions, due to the structure of the lhs of Eqs. (33), (34). Taing into account the conditions (31), (3) this choice yields to requirements for the complex coefficients A of the zero order solution which build the secular terms on the rhs of the first order expansion (33), (34): id 1 α 1 ω A (T 1 )e iωit (37) f 1 (ω α 11 )A (T 1 )e iωit W(T ) + cc = id 1 (ω α 11 )A (T 1 )e iωit (38) f 1 α 1 A (T 1 )e iωit W(T ) + cc =. As a consequence of the ansatz (35), (36) and depending on the external forcing W(T ), the secular terms have to vanish. In order to solve the problem of a high frequency, ultronic excitated fluid sheet, we specify the external periodic forcing term W(T ) = cos(ωt ), and hence the differential equations (15), (16) well (), () become coupled equations of the Mathieutype. We restrict our analytical treatment on the ce of main resonance, which appears, if the stimulation frequency Ω approaches ω 1 or ω. Treating the ce Ω ω 1, where the second ce with Ω ω could be eily received by means of the substitution ω 1 ω, we introduce a detuning parameter σ which is given ǫσ = ω 1 Ω. (39) The incorporation of Eq. (39) in Eqs. (37), (37) leads, under the sumption ω ω 1 and after the neglect of high frequency terms, due to the Rotating Wave Approximation, to relations for the elimination of the secular terms. After some algebraic calculations it can be derived that the slow variing amplitude A 1 (T 1 ) h to fullfill the equation: D 1 A 1 = i α 1f 1 + f 1 (ω 1 α 11 ) ω 1 (ω 1 (α 11 α 1 )) Ā1e iσt1 (4) where Ā1 denotes the conugate complex amplitude. In order to solve Eq. (4) we separate A 1 into its real and imaginary part A 1 = (u + iv)exp(iσt 1 ). (41) 4 and substitute (41) into (4). Equating the derived expressions into real and imaginary values, we obtain two differential equations for u and v: ( α1 f 1 + f 1 (ω ) 1 α 11 ) D 1 u = ω 1 (ω1 (α 11 α 1 )) + σ v (4) ( α1 f 1 + f 1 (ω ) 1 α 11 ) D 1 v = ω 1 (ω1 (α 11 α 1 )) σ u (43) Using the ansatz we obtain the amplitude (41) u = ξ exp(λt 1 ) (44) v = ζ exp(λt 1 ), (45) A 1 = (ξ + iζ)exp((λ + iσ)t 1 ). (46) Thus the system is stable if λ <, with ((ω 1 λ = ± α ) 11)f 1 + α 1 f 1 4ω 1 (ω1 α σ 11 + α 1 ). (47) In the ce oritical system behaviour λ h to vanish. This requirement leeds to ( ) (ω σ 1, = ± 1 α 11 )f 1 + α 1 f 1 4ω 1 (ω1 α. (48) 11 + α 1 ) Hence the transition curves are given by the expressions Ω = ω 1 + ǫσ 1 (ω 1 ) (49) Ω = ω 1 + ǫσ (ω 1 ). (5) The stability relations in the ce of wea viscous fluid sheets can be derived by umming a small damping given by γ = ǫγ. This leads to the system ( t + ǫγ t + α 11 )η a + (α 1 + ǫf 1 W(t))η s = (51) ( t + ǫγ t + α )η s + (α 1 + ǫf 1 W(t))η a = (5) which can be treaten in the preceding calculations. Numerical Treatment To confirm the approximative analytical calculations, we examine the derived evolution equations (15), (16) and (), () by numerical means. Because we consider a time periodic excitation with period π/ω given by W(t) = cos(ωt), one can sume, a result of the Floquet Theory, that the solutions of the considered equations are also time harmonic functions, having the form η i (t) = e λt η i (t), η i (t) = η i (t+π); i = s,a (53) Following Beyer & Friedrich 3], we expand the periodic functions η i (t) into Fourier series η i (t) = e (λ+iµ)t lim N n n= N η i ne inωt (54)

5 and obtain an infinite dimensional algebraic set of equations for the amplitudes of the wave modes 4 A s nη s n = α 1 η a n + ǫf 1 A a nη a n = α 1 η s n + ǫf 1 N n = N N n = N W n,n η a n (55) W n,n η s n, (56) sub sy harm sy where the coefficients A s n,a a n are given ] A s n = {λ + i(µ + nω)} + α 11 ] A a n = {λ + i(µ + nω)} + α and the excitation terms leads to (57) (58) W n,n = 1 π Ω dτe i(n n )Ωτ W(τ). (59) π The truncation of the Floquet ansatz at a finit but adequate high value of N leads to a linear, finitedimensional eigenvalue problem. Further on, to obtain critical behavior of the system, we have to demand λ = in Eqs. (57), (58) and choose µ = or µ = 1/ to calculate the stability branches for the harmonic or subharmonic solutions, respectively. Applying this we can numerical solve system (55), (56) and determine the critical forcing amplitude ǫ = by means of standart routines. 5 1 ˆcm 1 Figure 3. Analytically calculated stability regions of an ideal fluid sheet. denotes the scaled critical forcing amplitude and the wave number in ˆcm 1. Transition curves of the subharmonic solutions are termed sub where the branches of the harmonic solution are denoted by harm. The substructures belonging to the antisymmetric or symmetric sy wave modes respectively. As in the ce of the clsical Faraday Instability ], the (,)-plane is seperated in different tongue-lie regions, belonging to the subharmonic and harmonic solutions. As a result it can be seen, that the harmonic well the subharmonic tongue h a substructure. The solvability relations (31), (3) allow to distinguish between tongues belonging to the antisymmetrical and the symmetrical wave modes, respectively. 4 Results and Discussion With the analytical derived expressions (49), (5) we are able to calculate the instability branches for a free liquid sheet under an harmonic high frequency, ultronic excitation. For the subsequent considerations we have used the fluid parameters of water to model the fluid sheet and the values of air for the surrounding geous atmosphere. A thicness of h = 1e 3 cm for the fluid sheet w selected and a forcing frequency w choosen Ω/π = 5 Hz. Figure 3. shows the results of the multiple time scale approximation. 5 Figure 4. Influence of damping on the stability regions of a fluid sheet. The transition curve with red dots ( ) belongs to the undamped fluid sheet where the curve with blac crosses (+) belongs to the subharmonic solution of antisymmetrical wave mode of the the damped system. 5

6 Due to the neglect of viscosity, we see that the tips of the instability zones reach the axis of abscissae. This means in the physical interpretation, that infinitesimal small forcing amplitudes can destabilize the fluid sheet and thus initialize sheet brea up. This quite unphysical result w revised due to the phenomenological modelling of viscous dissipation effects. The incorporation of damping terms into the system leads to a excitation threshold shown in Fig. 4. and thus a finite (critical) forcing amplitude is necessary to excite waves on the fluid sheet. Figures 5. and 6. show the numerical calculated stability regions. The obtained results confirm the analytical considerations. Furthermore one can see that the harmonic solutions are in general more damped then the subharmonic ones, where excitation of symmetric wave modes need a higher forcing amplitude compared to the antisymmetric wave modes. As a result subharmonic, ymmetric waves are the most unstable, because their critical threshold is the lowest one. e+5 It h to be pointed out, that the interpretation of the subtongues instability regions belonging to the antisymmetric and symmetric wave modes w only possible by means of the analytical calculations. Conclusion We have derived the bic equations describing the external excitation of the surfaces waves of a free liquid sheet in a geous atmosphere. Thereby we have shown that the linear stability analysis leads to a set ooupled differental equations with time dependent coefficients. The equations have been extended, due to the inclution of viscous dissipation effects. Considering an external excitation in the form W(t) = cos(ωt), the differential equations system becomes coupled equations of the Mathieu-type. These equations have been solved analytical well numerical. The results of the calculations show that the instability zones for a thin liquid sheets under an external harmonic forcing splits into branches for the symmetric and antisymmetric surface wave modes for subharmonic and harmonic solutions respectively. This result shows that the principal mechanism of ultronic sisted fluid atomization is given by parametric resonance. References ˆcm 1 Figure 5. Numerical calculated stability regions of an undamped liquid sheet e ˆcm 1 Figure 6. Influence of damping on the stability regions of a fluid sheet. The critical wave number c belongs to the minima of the tongues 1] Abramov, O.V., Borisov, Y.Y and Oganyan, R.A.: Sov. Phys. Acoust., 33, ] Benamin, T.B. and Ursell, F.: Proc. R. Soc. London A, 5, ] Beyer, J. and Friedrich, R.: Phys. Rev. E, 51, ] Landau, L.D. and Lifschitz, E.M.: Hydrodynami, Aademie, Berlin, ] Lessmann, N., Bothe, D., Warnece H.-J.: Chem. and Eng. Tech, ECCE-4, 4. 6] Li, X. & Tanin, R.S.: Journal of Fluid Mechanics, 6, ] Lin, S.P.: Breaup of liquid sheets and ets, Cambridge University Press, 3. 8] Mohammed, A.E.L. et al.: Il Nuovo Cimento, 8, ] Nayfeh, A.H and Moo, D.T.: Nonlinear Oscillations, John Wiley & Sons, New Yor, ] Reipschläger at al: Proc. 18th Annual Conf. Liquid Atomization and Spray Systems, ILASS- Europe, Zaragoza. 11] Taylor, G.I.: Proc. R. Soc. London A, 53,

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