1 Introduction
In this work we examine the dynamics of an elastic sphere with an embedded viscous layer, excited by an impinging acoustic plane wave. We focus on configurations with similar acoustic and viscous-elastic time scales as well as acoustic wavelengths comparable with the sphere radius. The characteristic time scale of the linearized interaction between an elastic structure and a creeping flow scales as $\propto \unicode[STIX]{x1D707}/y$ (e.g. Elbaz & Gat Reference Elbaz and Gat2014) where the relevant Womersley number scales as $\propto \unicode[STIX]{x1D70C}r^{2}y/\unicode[STIX]{x1D707}^{2}$ ( $y$ is Young’s modulus, $\unicode[STIX]{x1D707}$ is viscosity, $r$ is characteristic length and $\unicode[STIX]{x1D70C}$ is density). Thus, the characteristic time scale of the viscous-elastic interaction can be reduced, without increasing inertial effects, by decreasing $r^{2}/\unicode[STIX]{x1D707}$ inversely with $\unicode[STIX]{x1D707}/y$ . For geometries in the micrometre scale, fluid–structure interaction at the creeping regime may occur at time scales similar to the acoustic time scale $r/c$ , where $c$ is the speed of sound.
Transient and oscillatory viscous-elastic interaction dynamics are relevant to various fields (Duprat & Stone Reference Duprat and Stone2015). Among these are biological configurations such as propulsion of micro-organisms by flagella (Wiggins & Goldstein Reference Wiggins and Goldstein1998; Camalet & Jülicher Reference Camalet and Jülicher2000; Tony, Lauga & Hosoi Reference Tony, Lauga and Hosoi2006), analysis and testing of corneal biomechanics (Chauhan & Radke Reference Chauhan and Radke2002; Duchemin & Vandenberghe Reference Duchemin and Vandenberghe2014; Han et al. Reference Han, Tao, Zhou, Sun, Zhou, Ren and Roberts2014) and flows in small blood vessels (Lowe & Pedley Reference Lowe and Pedley1995; Heil Reference Heil1997; Canic & Mikelic Reference Canic and Mikelic2003). Other relevant fields are geophysical gravity currents involving elastic surfaces (Balmforth, Craster & Hewitt Reference Balmforth, Craster and Hewitt2015; Hewitt, Balmforth & De Bruyn Reference Hewitt, Balmforth and De Bruyn2015), elastic peeling problems (McEwan & Taylor Reference McEwan and Taylor1966; Hosoi & Mahadevan Reference Hosoi and Mahadevan2004; Lister, Peng & Neufeld Reference Lister, Peng and Neufeld2013) and applications such as viscous-elastic pumps for the creeping flow regime (Arco et al. Reference Arco, Vélez-Cordero, Lauga and Zenit2014).
The subject of an acoustic plane wave impinging on an elastic spherical configuration has been studied extensively (e.g. Love Reference Love1927; Faran Reference Faran1951; Logan Reference Logan1965). A common interest in such problems is acoustic scattering (Bowen & Urzhumov Reference Bowen and Urzhumov2016), which defines the target strength of the sphere and is of importance to applications such as ultrasound tests, tomography and seismology. Various previous studies examined embedded layers as a mechanism to achieve a desired reduction of target strength of a spherical configuration. These include Guild, Alu & Haberman (Reference Guild, Alu and Haberman2011), who studied the effect of a single metamaterial layer and showed a target strength reduction of up to 30 dB for specific frequencies. In a later study Guild et al. (Reference Guild, Hicks, Haberman, Alù and Wilson2015) examined the effect of spherical fluid layers surrounding non-spherical elastic structures, and obtained a reduction of 30–40 dB in scattering strength. Torrent & Sánchez-Dehesa (Reference Torrent and Sánchez-Dehesa2008) have proposed to use a large number of alternating metamaterial layers, and later Huang, Zhong & Liu (Reference Huang, Zhong and Liu2014) have extended this approach to include turbulent flow, with moderate success. Analysis of acoustic scattering from spherical configurations with an embedded viscous layer is presented in Skelton & James (Reference Skelton and James1997). However, due to an initial assumption of P-waves propagating within the fluidic layer, and since viscosity is represented only as a damping mechanism to these waves, the mathematical treatment of Skelton & James (Reference Skelton and James1997) could not be extended to the creeping regime, which is governed by the relevant Reynolds equation.
In this context, the goal of the current work is to study the interaction between viscous-elastic dynamics and acoustic waves, for micro-configurations with similar viscous-elastic and acoustic time and length scales. This requires extension of the analysis of a spherical layered elastic structure and incorporation of the parabolic Reynolds equation into the spectral series solution for the hyperbolic elastic and acoustic regions. The structure of this work is as follows. In § 2 we define the problem, apply order-of-magnitude analysis and develop the Reynolds equation to a series of Legendre polynomials. In § 3 we develop the spectral stiffness matrix for the creeping fluidic layer and incorporate it into the global stiffness matrix of the elastic sphere. In § 4 we present and discuss the pressure and velocity within the fluidic layer, as well as the effect of the viscous layer on the displacements and target strength of the sphere. In § 5 we give concluding remarks.
2 Problem formulation and order-of-magnitude analysis
We examine an acoustic wave interacting with a core-in-shell geometry consisting of an elastic sphere surrounded by thin viscous and elastic layers. In order to examine configurations with significant spatial pressure variation, we focus on acoustic wavelengths similar to the radius of the sphere. The configuration is illustrated in figure 1 and contains four regions: region 1 ( $r\leqslant r^{(1)}$ ) is an inner elastic sphere; region 2 ( $r^{(1)}<r\leqslant r^{(2)}$ ) is a thin viscous layer with negligible inertial effects; region 3 ( $r^{(2)}<r\leqslant r^{(3)}$ ) is an elastic spherical shell; and region 4 ( $r^{(3)}<r$ ) is an acoustic region with negligible viscous effects. We examine micro-configurations where the characteristic time scale of viscous-elastic interaction is similar to the time scale of the acoustic wave.
We employ a spherical coordinate system, denoted by $(\unicode[STIX]{x1D703},\unicode[STIX]{x1D719},r)$ , with origins located at the centre of the sphere at rest. Time is denoted by $t$ . The velocity of the acoustic wave is parallel to the $\unicode[STIX]{x1D719}=\unicode[STIX]{x1D703}=0$ direction and thus the configuration is axisymmetric with regard to the $\unicode[STIX]{x1D719}=\unicode[STIX]{x1D703}=0$ line. The displacements and velocity in region $M$ are defined by $\boldsymbol{d}^{(M)}=(d_{r}^{(M)},d_{\unicode[STIX]{x1D703}}^{(M)})$ and $\boldsymbol{u}^{(M)}=(u_{r}^{(M)},u_{\unicode[STIX]{x1D703}}^{(M)})$ , respectively, where $\boldsymbol{u}^{(M)}=\unicode[STIX]{x2202}\boldsymbol{d}^{(M)}/\unicode[STIX]{x2202}t$ . Stress in region $M$ is denoted by $\unicode[STIX]{x1D70E}_{jk}^{(M)}$ , where the stress is in the $j$ -direction and acts on the plane perpendicular to the $k$ -direction. Density is denoted by $\unicode[STIX]{x1D70C}^{(M)}$ . In the fluidic regions ( $M=2,4$ ) we denote pressure as $p^{(M)}$ . The pressure amplitude of the acoustic wave in region 4 is denoted by $p_{a}$ , the acoustic wavelength is denoted by $l$ and the speed of sound is $c^{(M)}$ .
The Newtonian fluidic layers are governed by Navier–Stokes equations, while the linearly elastic regions are governed by the Cauchy–Navier equations. For all regions, conservation of mass,
and conservation of momentum (neglecting body forces),
are applied, where $\bar{\unicode[STIX]{x1D748}}^{M}$ is the stress tensor. In the fluidic regions ( $M=2,4$ ) the constitutive relation is given by
where $p=-\text{tr}(\bar{\unicode[STIX]{x1D748}}^{(M)})/3$ , while in the elastic layers ( $M=1,3$ ) (Howell, Kozyreff & Ockendon Reference Howell, Kozyreff and Ockendon2009)
For the fluidic regions ( $M=2,4$ ) $\unicode[STIX]{x1D707}^{(M)}$ and $\unicode[STIX]{x1D706}^{(M)}$ are the shear and bulk viscosity coefficients, respectively. For the elastic regions ( $M=1,3$ ) $\unicode[STIX]{x1D706}^{(M)}$ and $\unicode[STIX]{x1D707}^{(M)}$ are the Lamé constants, given by
and
where $y^{(M)}$ is Young’s elastic modulus and $\unicode[STIX]{x1D708}^{(M)}$ is Poisson’s ratio. In addition, we require the fluid in region 2 to be governed by interaction between fluid viscosity and the elasticity of the bounding regions $(1,3)$ , and thus assume negligible compressibility effects, $\unicode[STIX]{x1D70C}^{(2)}=\text{const}$ .
Our analysis examines configurations that agree with the following small geometric parameters, representing the ratio between the width of the viscous layer and the radius of the inner sphere,
and the width of the elastic shell layer to the radius of the inner sphere
In addition, we focus on the acoustic pressure field, which is significantly non-uniform across the surface of the sphere. This sets the characteristic acoustic wavelength in region 4 to ${\sim}O(r^{(1)})$ and thus the characteristic acoustic time scale is $t_{a}=r^{(1)}/c^{(4)}$ . We denote $t^{\ast }$ as the characteristic viscous-elastic time scale and $(d_{r}^{\ast },d_{\unicode[STIX]{x1D703}}^{\ast })$ are characteristic displacements of the elastic regions. The geometric requirements (2.6) are thus supplemented by the physical requirements of similar viscous-elastic and acoustic time scales,
small elastic displacements,
negligible inertia in region 2,
and negligible viscosity in region 4,
where $(\unicode[STIX]{x1D6FC}^{(2)})^{2}$ and $(\unicode[STIX]{x1D6FC}^{(4)})^{2}$ denote the Womersley numbers in regions 2 and 4, respectively.
We apply order-of-magnitude analysis in order to quantify the physical requirements described in (2.7) in terms of material properties and geometric parameters of the layered sphere. Hereafter normalized variables are denoted by capital letters and characteristic values are denoted by superscript asterisks.
We define the normalized radial coordinate and time,
and the normalized velocity and pressure of region 2,
where $(u_{r}^{(2),\ast },u_{\unicode[STIX]{x1D703}}^{(2),\ast })$ is the characteristic speed in region 2. The normalized displacements of the elastic boundaries of region 2 are
and
The characteristic fluid velocity, solid displacement and viscous-elastic time scale may be estimated by substituting (2.8)–(2.11) into (2.1)–(2.4) and applying order-of-magnitude analysis. From the governing equations of the creeping region 2, we obtain
and
Order-of-magnitude analysis of the governing equations of the elastic region 3, and specifically (2.4), yields
and
Applying (2.7) and substituting (2.8)–(2.11) into (2.1)–(2.3), the leading-order normalized governing equation for region 2 is the relevant linearized Reynolds equation,
From (2.12)–(2.15), we can relate our physical requirements (2.7) to the geometric and material properties of the configuration. These include the requirements of similar viscous-elastic and acoustic time scales,
small deformations,
negligible inertial effects in region 2,
and negligible viscous effects in region 4
The requirements of small deformation in region 3 (2.17b ) and negligible inertial effects in region 4 (2.17d ) are easily satisfied for a wide range of common geometric configurations and material properties. However, the requirement of negligible inertial effects in region 2 (2.17c ) combined with the requirement of similar acoustic and viscous-elastic time scales (2.17a ) severely limits the range of validity of the current analysis. Even for highly viscous fluids (e.g. silicone oil with $\unicode[STIX]{x1D707}^{(2)}\approx 100~\text{Pa}~\text{s}$ ) and rigid solids (e.g. steel with $y^{(3)}=200$ GPa and $\unicode[STIX]{x1D708}^{(3)}=0.29$ ) surrounded by water ( $\unicode[STIX]{x1D70C}^{(4)}=1000~\text{kg}~\text{m}^{-3}$ and $c^{(4)}=1484~\text{m}~\text{s}^{-1}$ ), the above requirements limit the sphere diameter to $2r^{(1)}\leqslant 2$ mm and thus to ultrasound frequencies ${\geqslant}750$ kHz. In addition, since $(r^{(2)}-r^{(1)})/r^{(1)}\ll 1$ , the results are practically valid only for microfluidic configurations where $r^{(2)}-r^{(1)}\approx 100~\unicode[STIX]{x03BC}\text{m}$ or less.
3 Incorporating the Reynolds equation into the acoustic stiffness matrix
Acoustic scattering of plane waves from spherical configurations has been studied extensively, and the treatment of regions 1, 3 and 4 may be found elsewhere (e.g. Love Reference Love1927; Logan Reference Logan1965; Skelton & James Reference Skelton and James1997) and will be omitted here. The aim of this section is the incorporation of the parabolic region 2 into the standard scheme for the hyperbolic elastic and acoustic regions. In spherical coordinates, the impinging plane wave in region 4, denoted by $P_{i}^{(4)}=p_{i}^{(4)}/p_{a}$ , is given by
where $k=\unicode[STIX]{x1D714}/c^{(4)}$ is the impinging wavenumber, $L_{n}$ is Legendre polynomial and $\text{j}_{n}$ is the spherical Bessel function of the first kind.
The total scattered pressure in the external acoustic fluid, denoted by $P_{s}^{(4)}=P_{r}^{(4)}+P_{e}^{(4)}$ , can be presented as the sum of the pressure reflected from a rigid sphere, $P_{r}^{(4)}$ , and the additional pressure due to elastic displacements of the sphere, $P_{e}^{(4)}$ (all pressures are scaled by $p_{a}$ ). The acoustic scattering due to a rigid sphere, given by $P_{r}^{(4)}=p_{r}^{(4)}/p_{a}$ , is
where $\text{h}_{n}$ is the spherical Hankel function of the first kind.
We thus hereafter focus on calculation of acoustic scattering due to elastic displacements of the sphere $P_{e}^{(4)}$ . In order to incorporate the dynamics of the Reynolds equation governing region 2 (2.16) into the calculation of $P_{e}^{(4)}$ , we require series solution of the radial displacements and stress on the boundaries of region 2 to be of the form
where $D_{R}^{(1)}$ and $D_{R}^{(2)}$ are amplitudes of radial displacements at $R=R^{(1)}$ and $R=R^{(2)}$ , respectively. Similarly, $S_{RR}^{(1)}$ and $S_{RR}^{(2)}$ are amplitudes of radial stress at $R=R^{(1)}$ and $R=R^{(2)}$ , respectively. In addition, we require series solution of the tangential displacements and stress on the boundaries of region 2 to be of the form
where $D_{\unicode[STIX]{x1D703}}^{(1)}$ and $D_{\unicode[STIX]{x1D703}}^{(2)}$ are amplitudes of displacements in the $\unicode[STIX]{x1D703}$ -direction at $R=R^{(1)}$ and $R=R^{(2)}$ , respectively. The parameters $S_{R\unicode[STIX]{x1D703}}^{(1)}$ and $S_{R\unicode[STIX]{x1D703}}^{(2)}$ are amplitudes of shear stress at $R=R^{(1)}$ and $R=R^{(2)}$ , respectively.
In the examined limit of incompressible lubrication flow, the pressure in region 2 is independent of $r$ , and applying (3.3a ) yields a general solution in terms of the orthogonal Legendre polynomials
where $P_{n}^{(2)}$ are constants representing the pressure amplitude of each Legendre mode. Substituting (3.3) and (3.4) into (2.16) and utilizing the identity
yields $P_{n}^{(2)}$ ,
and $U_{\unicode[STIX]{x1D703},n}^{(2)}$ can be obtained from the tangential momentum equation,
where $H=(r-r^{(1)})/(r^{(2)}-r^{(1)})$ . Since substitution of (3.6) into the lubrication equation (2.16) yields $u_{\unicode[STIX]{x1D703}}^{(2)}$ and $\unicode[STIX]{x1D70E}_{r\unicode[STIX]{x1D703}}^{(2)}$ to be series of the derivatives of Legendre polynomials, the series representation of region 2 agrees with the requirements of both (3.3a ) and (3.3b ). Thus we can proceed and incorporate parabolic region 2 into the acoustic scheme for the hyperbolic regions 1, 3 and 4.
Hereafter we revert to dimensional parameters. Applying the leading-order lubrication relations $p^{(2)}\sim \unicode[STIX]{x1D70E}_{rr}^{(2)}$ and $\unicode[STIX]{x1D70E}_{r\unicode[STIX]{x1D703}}^{(2)}\sim \unicode[STIX]{x1D707}^{(2)}\unicode[STIX]{x2202}u_{\unicode[STIX]{x1D703}}^{(2)}/\unicode[STIX]{x2202}r$ , we can obtain from (3.6) and (3.7) a relation between the traction vector $\boldsymbol{s}_{n}=[\unicode[STIX]{x1D70E}_{rr,n}^{(1)},\unicode[STIX]{x1D70E}_{r\unicode[STIX]{x1D703},n}^{(1)},\unicode[STIX]{x1D70E}_{rr,n}^{(3)},\unicode[STIX]{x1D70E}_{r\unicode[STIX]{x1D703},n}^{(3)}]$ created by excitation of the form of Legendre polynomial of order $n$ and the displacement vector $\boldsymbol{d}_{n}=[d_{r,n}^{(1)},d_{\unicode[STIX]{x1D703},n}^{(1)},d_{r,n}^{(3)},d_{\unicode[STIX]{x1D703},n}^{(3)}]$ on the boundaries of region 2. This yields $\{\boldsymbol{d}_{n}\}=[\unicode[STIX]{x1D637}_{ij}]^{-1}\{\boldsymbol{s}_{n}\}$ , where $\unicode[STIX]{x1D637}_{ij}$ is the dimensional stiffness matrix for the Reynolds region 2 given by
A global spectral matrix of the tractions and the displacements for Legendre mode $n$ , connecting Reynolds region 2 to regions 1, 3 and 4, may now be obtained,
where $\unicode[STIX]{x1D70E}_{rr,n}^{(3)}=-p_{a}i^{n+1}(2n+1)(c^{(4)})^{2}/\unicode[STIX]{x1D714}^{2}r^{(3)}h_{n}^{\prime }(r^{(3)}\unicode[STIX]{x1D714}/c^{(4)})$ is the stress applied by the impinging plane wave. The coefficients for the acoustic region 4 and the elastic regions 1 and 3 are presented in the Appendix and their derivation may be obtained from Skelton & James (Reference Skelton and James1997). Specifically, $f_{11}$ is defined in (A 1), $\boldsymbol{e}$ is defined in (A 2) and $\boldsymbol{g}$ is defined in (A 23).
Mode $n=0$ corresponds to spatially uniform pressure in region 4, for which the stiffness matrix of region 2 ( $\unicode[STIX]{x1D637}_{ij,n}$ ) and thus the global stiffness matrix (3.10) are singular. This singularity expresses the trivial solution for the fluid $\unicode[STIX]{x1D703}$ -direction momentum conservation equation. Resolving this requires directly applying mass conservation to region 2, yielding $d_{r,n=0}^{(1)}=d_{r,n=0}^{(2)}$ combined with symmetry requirements $d_{\unicode[STIX]{x1D703},n=0}^{(3)}=d_{\unicode[STIX]{x1D703},n=0}^{(2)}=d_{\unicode[STIX]{x1D703},n=0}^{(1)}=0$ . The resulting simplified system of equations for the displacements for $n=0$ is
4 Results and comparison to a fully elastic sphere
Figure 2 presents the velocity and pressure fields in region 2 due to the impinging acoustic plane wave. In order to comply with the physical requirements described in (2.17a ), the examined configuration consists of highly rigid elastic regions 1 and 3 (steel with $y^{(1)}=y^{(3)}=200$ GPa, $\unicode[STIX]{x1D708}^{(1)}=\unicode[STIX]{x1D708}^{(3)}=0.29$ ) and the embedded viscous film of region 2 is a highly viscous silicone oil ( $\unicode[STIX]{x1D70C}^{(2)}=970~\text{kg}~\text{m}^{-3},\unicode[STIX]{x1D707}^{(2)}=100~\text{Pa}~\text{s}$ ). The geometry of the layered sphere is defined by $r^{(1)}=0.6$ mm, $r^{(2)}=1.2r^{(1)}$ and $r^{(3)}=1.4r^{(1)}$ . The sphere is submerged in water ( $\unicode[STIX]{x1D70C}^{(4)}=1000~\text{kg}~\text{m}^{-3},\unicode[STIX]{x1D707}^{(4)}=10^{-3}~\text{Pa}~\text{s}$ ) with speed of sound of $c^{(4)}=1480~\text{m}~\text{s}^{-1}$ .
Figure 2(a) presents the $r$ -averaged speed in the $\unicode[STIX]{x1D703}$ -direction $\langle U_{\unicode[STIX]{x1D703}}\rangle$ , defined by
for impinging wavelengths of $\unicode[STIX]{x1D706}/r^{(1)}=0.5$ (green dashed line), $1$ (black full line) and $1.5$ (red dotted line). In all cases, the magnitude of the average speed, induced due to both the pressure gradient and the elastic displacements of the boundaries in the $\unicode[STIX]{x1D703}$ -direction, is maximal near $\unicode[STIX]{x1D703}\approx 160^{\circ }$ . The density of the velocity peaks increases inversely with $\unicode[STIX]{x1D706}/r^{(1)}$ and, while $\unicode[STIX]{x1D706}/r^{(1)}=1$ yields the maximal values of $\langle U_{\unicode[STIX]{x1D703}}\rangle$ , all wavelengths yield speeds with similar order of magnitude.
Figure 2(b) presents the pressure in region 2 versus $\unicode[STIX]{x1D703}$ for identical wavelengths as in figure 2(a) ( $\unicode[STIX]{x1D706}/r^{(1)}=0.5$ , $1$ and $1.5$ ). Similarly to $\langle U_{\unicode[STIX]{x1D703}}\rangle$ , the pressure increases in the direction in which the wave impinges on the surface of the sphere. Unlike figure 2(a), an order-of-magnitude difference in the characteristic pressure is evident for $\unicode[STIX]{x1D706}/r^{(1)}=0.5$ compared to $\unicode[STIX]{x1D706}/r^{(1)}=1.5$ , representing a smaller effective length scale in the $\unicode[STIX]{x1D703}$ -direction (see (2.12)). The maximal pressure difference within the creeping layer occurs for $\unicode[STIX]{x1D706}/r^{(1)}=1$ , where the viscous-elastic and acoustic time and length scales are identical. In addition, for $\unicode[STIX]{x1D706}/r^{(1)}=1$ and $1.5$ the number of zeros of $\langle U_{\unicode[STIX]{x1D703}}\rangle$ is identical to the number of extremum points of $P$ (for $0^{\circ }<\unicode[STIX]{x1D703}<180^{\circ }$ ). However, for $\unicode[STIX]{x1D706}/r^{(1)}=0.5$ , the first zero of $\langle U_{\unicode[STIX]{x1D703}}\rangle$ is at $\unicode[STIX]{x1D703}\approx 80^{\circ }$ and there are several small extremum points of $P$ without a corresponding zero of $\langle U_{\unicode[STIX]{x1D703}}\rangle$ . This indicates that $\langle U_{\unicode[STIX]{x1D703}}\rangle$ at the backward surface of the sphere (relative to the direction of the impinging wave) is dominated by $\unicode[STIX]{x1D703}$ -displacement of the elastic shell and not by the pressure gradient.
Figure 3 presents the average absolute magnitude of the displacements of the outer shell in the radial and tangential directions for a fully elastic sphere (grey lines) and an elastic sphere containing a thin creeping layer (black lines). The properties of the sphere are identical to the case presented in figure 2. The multiple peaks presented correspond to resonance frequencies of the fully elastic sphere. The effect of the thin creeping layer is clearly significant, and effectively eliminates the fluctuations in the radial displacements of the elastic sphere as a function of the wavelength of the impinging acoustic plane wave. In addition, while no tangential displacements occur for a fully elastic sphere, the creeping layer creates significant tangential displacements, which are similar in magnitude to the radial deflections. Figure 4 supplements figure 3 and presents a more detailed description of the displacements of the outer surface of the sphere for a given wavelength. Figure 4(a–c) presents wavelengths of $\unicode[STIX]{x1D706}/r^{(1)}=0.5$ , $1$ and $1.5$ , respectively. For all wavelengths, in accordance with results of figure 3, the amplitude of the displacements is significantly reduced. In addition, for $\unicode[STIX]{x1D706}/r^{(1)}=1$ and $1.5$ , additional maxima points of the deflection field are created due to the embedded creeping layer.
Figure 5 presents the effect of the creeping fluid layer on the target strength $T_{s}$ of the sphere. The target strength, measured in decibels, represents acoustic visibility and following common practice is defined here by
The total scattered pressure in the external acoustic fluid $p_{s}^{(4)}=p_{r}^{(4)}+p_{e}^{(4)}$ is the sum of the pressure reflected from a rigid sphere $p_{r}^{(4)}$ (3.2) and the additional pressure due to elastic displacements of the sphere, $p_{e}^{(4)}$ , given by
Figure 5(a) compares target strength (defined by (4.2)) of a fully elastic sphere (grey line) with an elastic sphere with a viscous layer (black line) versus the scaled wavelength of the impinging plane wave. All of the physical and geometric parameters are identical to these used in figure 2, with the exception of $\unicode[STIX]{x1D707}^{(2)}$ , which is defined by setting the ratio $t^{\ast }/t_{a}=\unicode[STIX]{x1D707}^{(2)}c^{(4)}/(\unicode[STIX]{x1D700}^{(1)})^{3}\unicode[STIX]{x1D700}^{(2)}\unicode[STIX]{x1D706}^{(3)}r^{(1)}=1$ . The viscous layer significantly reduces the fluctuations of target strength with the wavelength $\unicode[STIX]{x1D706}/r^{(1)}$ . The difference between the minimal and maximal values of the target strength is reduced from ${\approx}27$ dB (from ${\approx}-27$ to ${\approx}0.25$ ) for the fully elastic sphere to ${\approx}8.7$ dB (from ${\approx}-13.4$ to ${\approx}-4.7$ ) for the sphere with a creeping layer. Furthermore, for wavelengths in the range $0.5\leqslant \unicode[STIX]{x1D706}/r^{(1)}\leqslant 0.9$ the fluctuations are under 1 dB and the target strength is only weakly dependent on the wavelength $\unicode[STIX]{x1D706}/r^{(1)}$ . As the impinging wavelength increases, the effect of the creeping layer is diminished, becoming negligible for $\unicode[STIX]{x1D706}/r^{(1)}\approx 2$ . This occurs since the sphere experiences spatially uniform temporally oscillating pressure at the limit of large wavelengths, which involves no viscous flow in region 2 and is described by the fully elastic $n=0$ mode (see (3.10)).
Figure 5(b) is a close-up of figure 4(a) for the region $0.5\leqslant \unicode[STIX]{x1D706}/r^{(1)}\leqslant 0.9$ and compares several values of $t^{\ast }/t_{a}=\unicode[STIX]{x1D707}^{(2)}c^{(4)}/(\unicode[STIX]{x1D700}^{(1)})^{3}\unicode[STIX]{x1D700}^{(2)}\unicode[STIX]{x1D706}^{(3)}r^{(1)}$ denoted by markers within the figure. While a region of stability of target strength is evident for all values of $t^{\ast }/t_{a}$ , the wavelength range of this region is maximal for $t^{\ast }/t_{a}=1$ . Viscosity may be expected to have maximal effect for $t^{\ast }/t_{a}\approx 1$ since for $t^{\ast }/t_{a}\gg 1$ the viscous layer does not have sufficient time to react to the acoustic oscillations. For the opposite case of $t^{\ast }/t_{a}\ll 1$ , the viscous layer will be in a quasi-steady state and will have nearly uniform pressure $p^{(2)}\approx \text{const}$ .
5 Concluding remarks
This work examined the dynamics of an acoustic plane wave impinging on the surface of a sphere with an embedded creeping layer, focusing on micro-configurations with similar viscous-elastic and acoustic time and length scales. By expanding the linearized spherical Reynolds equation into the relevant spectral series solution for the hyperbolic elastic regions, a global stiffness matrix of the layered elastic sphere was obtained.
As expected, the results showed that both the pressure and velocity within the creeping layer are maximal near the region on which the plane wave impinges. In addition, the maximal pressure difference induced by the acoustic wave on the creeping region 2 was shown to occur for $\unicode[STIX]{x1D706}/r^{(1)}=1$ , where the viscous-elastic and acoustic regions have identical time and length scales. Comparing an elastic sphere with an embedded creeping layer to a fully elastic sphere, a significant reduction in magnitude and fluctuations (with regard to wavelength) are observed for both the displacements of the solid and the target strength of the sphere. This effect was most significant for $\unicode[STIX]{x1D706}/r^{(1)}=1$ .
The physical regime examined in this work required similar characteristic acoustic and viscous-elastic time- and length scales, as well as negligible inertial effects in the creeping region 2 and negligible viscous effects in the acoustic region 4. Order-of-magnitude analysis yielded that the region of validity of this physical regime is limited to micro-configurations involving highly viscous fluids. Extension to greater length scales may be obtained by combining multiple spheres, which may be viewed as a metamaterial. Alternatively, a similar physical regime may be examined in porous structures, which commonly involve micrometre-sized pores.
Appendix. Components of the global stiffness matrix
For completeness, we list here the components of the global stiffness matrix (3.9) representing regions 1, 3 and 4 (see Skelton & James Reference Skelton and James1997). We denote $\text{j}_{n}$ , $\text{y}_{n}$ and $\text{h}_{n}$ as the spherical Bessel function of the first kind, the spherical Bessel function of the second kind, and the spherical Hankel function of the first kind, respectively.
In region 4, we define $k^{(4)}=\unicode[STIX]{x1D714}/c^{(4)}$ , where $c^{(4)}$ is the speed of sound. In § 4 the value of $c^{(4)}=1480~\text{m}~\text{s}^{-1}$ is used, representing sea water, and the relevant component in (3.10) is
For the elastic regions $M=1$ and $M=3$ we define $k_{s}^{(M)}=\unicode[STIX]{x1D714}/c_{s}^{(M)}$ and $k_{l}^{(M)}=\unicode[STIX]{x1D714}/c_{l}^{(M)}$ , where $c_{s}^{(M)}$ and $c_{l}^{(M)}$ are speeds of pure transverse and longitudinal waves in the elastic solid, respectively. In § 4 the values of $c_{s}=3130~\text{m}~\text{s}^{-1}$ and $c_{l}=5760~\text{m}~\text{s}^{-1}$ are used, corresponding to steel. The coefficient matrix of elastic region 3 is given by
where $\unicode[STIX]{x1D644}_{0}$ is a diagonal matrix with diagonal values of $[1,1,-1,-1]$ required in order to adjust for directionality in the boundary conditions. The components of matrix $\unicode[STIX]{x1D656}$ are
and the components of matrix $\unicode[STIX]{x1D657}$ are
The stiffness matrix of the interior elastic sphere (region 1) is given by
where the components of the matrix $\unicode[STIX]{x1D668}$ are
and the components of the matrix $\unicode[STIX]{x1D669}$ are