11
Existence of torsional surface waves in an earth’s crustal layer lying over a sandy mantle Sumit Kumar Vishwakarma 1,2,and Shishir Gupta 1 1 Department of Applied Mathematics, Indian School of Mines, Dhanbad 826 004, India. 2 Department of Mathematics, Birla Institute of Technology and Science–Pilani, Hyderabad 500 078, India. Corresponding author. e-mail: [email protected] [email protected] This paper aims to study the dispersion of torsional surface waves in a crustal layer being sandwiched between a rigid boundary plane and a sandy mantle. In the mantle, rigidity and initial stress vary linearly while density remains constant. Dispersion relation has been deduced in a closed form by means of variable separable method in the form of Whittaker function. The velocity equation for isotropic layer over a homogeneous half-space has been obtained which coincides with the standard result of Love wave under the effect of rigid boundary. 1. Introduction The earth is layered solid under high initial stresses. Due to atmosphere, variation of temper- ature, gravitating pull, slow process of creep and pressure due to overburdened layer, a large quan- tity of stresses (may be critical initial stresses) are stored in the layer of the earth. Artificially gen- erated seismic waves provide information about the configuration of the rock layer for oil explo- ration, ground water prospecting and on smaller scale information as to the rigidity of shallow layer for engineering purposes. A straight mathematical attack may produce explicit or numerical solutions even for rather complex solid media. The math- ematical expression provides the bridge between modelling results and field application. Any dis- turbance in earth’s interior may serve as the basic reason of seismic wave propagation. The theoret- ical study of wave propagation consists of finding the solution of a partial differential equation or a system of partial differential modelling under ini- tial and boundary conditions. The propagation of seismic waves through the earth’s interior is gov- erned exactly by mathematical laws similar to the laws of light waves in optics. If the propagation velocities and other elastic properties were uni- form throughout the earth, seismic waves would radiate from the focus of the earthquake in all the directions through the earth along rectilinear path or rays. In general, however, the wave veloc- ity increases with depth and consequently, seismic rays are not straight lines but lines curved with the concave side upward providing the shortest time past through the earth. Earth is a gravitating initially stressed medium due to the presence of overburdened layers. The presence of gravity field and internal friction of dry sandy material will have effect on the propagation of the waves. The acceleration due to gravity g has a greater role to play in studying the dynamic and static problems of the earth. Kepceler (2010) has studied torsional wave dispersion relations in a pre-stressed bi-material compounded cylinder with an imperfect interface. Propagation of torsional surface waves in a homogeneous layer of finite Keywords. Torsional wave; mantle; Biot’s gravity parameter; graphical user interface. J. Earth Syst. Sci. 122, No. 5, October 2013, pp. 1411–1421 c Indian Academy of Sciences 1411

Existence of torsional surface waves in an earth’s crustal layer lying over a sandy mantle

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Existence of torsional surface waves in an earth’scrustal layer lying over a sandy mantle

Sumit Kumar Vishwakarma1,2,∗ and Shishir Gupta

1

1Department of Applied Mathematics, Indian School of Mines, Dhanbad 826 004, India.2Department of Mathematics, Birla Institute of Technology and Science–Pilani,

Hyderabad 500 078, India.∗Corresponding author. e-mail: [email protected] [email protected]

This paper aims to study the dispersion of torsional surface waves in a crustal layer being sandwichedbetween a rigid boundary plane and a sandy mantle. In the mantle, rigidity and initial stress varylinearly while density remains constant. Dispersion relation has been deduced in a closed form by meansof variable separable method in the form of Whittaker function. The velocity equation for isotropic layerover a homogeneous half-space has been obtained which coincides with the standard result of Love waveunder the effect of rigid boundary.

1. Introduction

The earth is layered solid under high initialstresses. Due to atmosphere, variation of temper-ature, gravitating pull, slow process of creep andpressure due to overburdened layer, a large quan-tity of stresses (may be critical initial stresses) arestored in the layer of the earth. Artificially gen-erated seismic waves provide information aboutthe configuration of the rock layer for oil explo-ration, ground water prospecting and on smallerscale information as to the rigidity of shallow layerfor engineering purposes. A straight mathematicalattack may produce explicit or numerical solutionseven for rather complex solid media. The math-ematical expression provides the bridge betweenmodelling results and field application. Any dis-turbance in earth’s interior may serve as the basicreason of seismic wave propagation. The theoret-ical study of wave propagation consists of findingthe solution of a partial differential equation or asystem of partial differential modelling under ini-tial and boundary conditions. The propagation of

seismic waves through the earth’s interior is gov-erned exactly by mathematical laws similar to thelaws of light waves in optics. If the propagationvelocities and other elastic properties were uni-form throughout the earth, seismic waves wouldradiate from the focus of the earthquake in allthe directions through the earth along rectilinearpath or rays. In general, however, the wave veloc-ity increases with depth and consequently, seismicrays are not straight lines but lines curved with theconcave side upward providing the shortest timepast through the earth.

Earth is a gravitating initially stressed mediumdue to the presence of overburdened layers. Thepresence of gravity field and internal friction of drysandy material will have effect on the propagationof the waves. The acceleration due to gravity ghas a greater role to play in studying the dynamicand static problems of the earth. Kepceler (2010)has studied torsional wave dispersion relations in apre-stressed bi-material compounded cylinder withan imperfect interface. Propagation of torsionalsurface waves in a homogeneous layer of finite

Keywords. Torsional wave; mantle; Biot’s gravity parameter; graphical user interface.

J. Earth Syst. Sci. 122, No. 5, October 2013, pp. 1411–1421c© Indian Academy of Sciences 1411

1412 Sumit Kumar Vishwakarma and Shishir Gupta

thickness over an initially stressed heterogeneoushalf-space have been recently studied by Guptaet al. (2012a) whereas propagation of torsionalsurface waves in dry sandy medium under grav-ity has been studied by Dey et al. (1998). Refer-ences can be made to Dey and Sarkar (2002); Selim(2007); Ozturk and Akbbarov (2009); Akbarovet al. (2011) and Gupta et al. (2012b, c) for theirexcellent contribution in investigating torsionalsurface wave in various mediums under various cir-cumstances. Behaviour of torsional surface wave inan elastic layer with void pores has been studied byDey et al. (2003) whereas torsional wave propaga-tion in a thin rectangular domain using asymptoticapproach has been handled by Davini et al. (2008).Golamhossen (2000) pointed out the propagationof waves in an elastic cylinder with voids while adetailed study has been made in axially symmet-ric problems for a porous elastic solid by Lesanand Nappa (2003). Some authors investigated theeffect of nonlinear variations in the elastic moduli,density and initial stress with various geo-media.Dey et al. (1996) discussed the possibility of prop-agation of torsional surface waves in a nonhomo-geneous elastic medium with polynomial variationof rigidity and density, i.e., μ = μ0 (1 + az)2n andρ = ρ0 (1 + az)m. They found that inhomogeneityparameter being non-linearly associated with rigid-ity and density has a prominent effect on torsionalsurface wave. Very recently, Chattaraj et al. (2011)investigated the propagation of torsional surfacewave in anisotropic poroelastic medium under ini-tial stress, where he has taken quadratic varia-tion in the directional rigidities, density and initialstress, i.e., N = N0 (1 + αz)2 , L = L0 (1 + αz)2,ρ = ρ0 (1 + αz)2, P = P0 (1 + αz)2. They foundthat the effect of quadratic variation is more pro-nouncing at higher frequency. Although the natureand characteristic of the curves for nonlinear vari-ations are similar to that being plotted for linearvariation in the present problem; on the basis ofthe studies being made by the authors in past, itcan be concluded that the effect of quadratic varia-tion on the phase velocity of torsional surface wavemay come out to be similar to that of the linearone, and has no special contribution or empha-size over the torsional surface wave. The reason forthis may lie to the fact that the basic character-istic of surface wave is that it decreases as depthincreases. Therefore z2 and higher power of z havebeen neglected and only linear variation has beenpreferred in the present problem. The works doneby Georgiadis et al. (2000); Quintanilla (2001);Midya (2004); Arora and Tomar (2007) and Guptaet al. (2013) cannot be overlooked as their con-tributions are commendable towards seismic wavepropagation.

So far, it has been found that the effect of grav-ity on the propagation of torsional surface wave inan inhomogeneous anisotropic layer has remainedunattempted. Therefore, in the present paper, anattempt has been made to study the propagation oftorsional surface waves in an anisotropic inhomo-geneous layer over gravitating dry sandy mantle.Torsional surface wave is a wave with amplitudedecaying exponentially with distance from the freesurface. Inside the earth, a very hard layer (alsoknown as ‘rigid’) is present. Since the compositionof the earth is heterogeneous including a very hardlayer, the inhomogeneous medium and the rigidinterface play significant roles in the propagationof the seismic waves. A dry sandy mantle may bedefined as a half-space consists of sandy particlesretaining no moistures or water vapours, the char-acteristic of which has been defined by η known assandy parameter.

For the present study, the heterogeneity takenis caused by variation in directional rigidities anddensity in the layer whereas heterogeneity taken inthe mantle is caused by variation in rigidity andinitial stress. The crust region of our planet is com-posed of various heterogeneous layers with differentgeological parameters. As pointed out by Bullen(1940), the density inside the earth varies at dif-ferent rates with different layers within the earth.He approximated density law inside the earth as aquadratic polynomial in depth parameter for 413–984 km depth. For depth from 984 km to the cen-tral core, Bullen approximated the density as alinear function of depth parameter. Sari and Salk(2002) took the variation in the density of sedi-ments with depth as a hyperbolic function. Like-wise, different authors have taken different formsof variation, like harmonic, linear, quadratic, expo-nential, etc., for simulating the variation in densityand other geological parameters inside the earth.Therefore, in the present paper, variations takenin the layer are N = N0e

z/α, L = L0ez/α, ρ =

ρ0ez/α, whereas variation taken in the mantle are

μ = μ1 (1 + a z) , P = P1 (1 + b z) , ρ = ρ1,where α is a constant having dimension equal tolength and a, b are constants having dimensionequal to inverse of length. ‘z’ is a vertical coordi-nate axis, positive downward having origin at theinterface (as shown in figure 1). It may also becalled as depth coordinate. In the half-space, rigid-ity varies linearly whereas density remains con-stant throughout; this is called Gibson half-space(Vardoulakis 1984). Keeping this in view, anattempt has been made to find out whether suchan inhomogeneous layer can allow torsional sur-face wave to propagate through it when lower Gib-son half-space (mantle) is dry and sandy underthe effect of gravitation. It is observed that thephase velocity of torsional surface wave increases

Existence of torsional surface waves in earth’s crustal layer 1413

Figure 1. Three-dimensional geometry of the problem.

with the increase of compressive initial stress whiledecreases as the tensile initial stress decreases.It has also been found that the phase velocityincreases as the inhomogeneity parameter associ-ated with rigidity and the initial stress increaseswhile decreases as the inhomogeneity parameterassociated with directional rigidity and density ofthe layer increases. It is observed that the pres-ence of gravity field always allow the torsional sur-face wave to propagate. It has also been concludedthat the torsional surface wave propagates moresmoothly in the layer when the lower half-space iselastic in comparison to dry sandy half-space. Fur-ther, anisotropy has also much effect in enhancingthe velocity of torsional surface wave.

The present study of the dispersion of torsionalwaves in an anisotropic inhomogeneous crustallayer over a sandy mantle can be used to refine ourknowledge of crustal and sub-crustal region nearthe earth surface. This study may also be usefulfor the study of seismic waves generated by artifi-cial explosions. Effect of torsional waves cannot beignored in assessment of damage caused by earth-quake waves. Hence, the present study with theassumed variation in rigidity, density and stressmay be useful in predicting nature of torsionalsurface wave in inhomogeneous geo-media.

2. Statement of the problem

To study the torsional surface waves, a cylin-der coordinate system is introduced with z-axistowards the interior of the gravitating dry sandyGibson half-space. A Gibson half-space is onewhere rigidity varies linearly while density remainsconstant. The study has been made to get the dis-persion equation of torsional surface wave in aninhomogeneous anisotropic layer of thickness H,over a sandy half-space under the effect of grav-ity, initial stress and rigid boundary as shown infigure 1. The origin of the coordinate system is

located at the surface of the half-space at the centreof a circular region.

3. Solution

3.1 Solution of the inhomogeneousanisotropic layer

If r and θ be radial and circumferential coordi-nates respectively, and if the wave travels along theradial direction only, the equation of motion in thelayer may be written as (Biot 1965):

∂σrθ

∂r+

∂σzθ

∂z+

2rσrθ = ρ

∂2v

∂t2(1)

where v(r, z, t) is the displacement along θ direc-tion and ρ is the density.

For a non-homogeneous anisotropic elastic me-dium, the stresses are related to strain by

σrθ = 2Nerθ, σzθ = 2Lezθ (2)

where erθ = 12

(∂v∂r

− vr

), ezθ = 1

2∂v∂z

. N and L aredirectional rigidities of the medium along r and zdirections, respectively.

Using the above relations, equation (1) takes theform

N

(∂2v

∂r2− v

r2+

1r

∂v

∂z

)+

∂z

(L

∂v

∂z

)= ρ

∂2v

∂t2. (3)

The solution of equation (3) when wave propagatealong radial direction with amplitude of displace-ment as a function of depth may be taken as:

v = V (z) J1 (kr) eiωt, (4)

ω being circular frequency of the wave where V (z)is the solution of

d2V (z)dz2

+1L

dL

dz

dV

dz− k2N

L

(1 − c2ρ

N

)= 0 (5)

1414 Sumit Kumar Vishwakarma and Shishir Gupta

where c = ω/k is the velocity of the propagationof torsional surface wave and J1 is the Bessel’sfunction of first kind and of order one.

On substituting, V = V1/√

L in equation (5), weget:

d2V1

dz2− 1

2L

{d2L

dz2− 1

2L

(dL

dz

)2}

V1

=k2N

L

(1 − c2ρ

N

). (6)

Now, the variations in directional rigidities (elasticmoduli) and density in the layer has been taken as:

N = N0ez/α, L = L0e

z/α, ρ = ρ0ez/α (7)

Using equation (7), equation (6) becomes:

d2V1

dz2− m2

1V1 = 0 (8)

where m21=k2

{1

4α2k2 + N0L0

(1− c2

c20

)}and c0=

√N0/ρ0

is the shear wave velocity in the layer.The solution of equation (8) is given by

V (z) = A1e−m1z + A2e

m1z

where A1 and A2 are arbitrary constants and hencethe displacement in the upper inhomogeneousanisotropic layer is given by

v = v0 (say) ={

A1e−(m1+

12α)z + A2e

(m1− 12α)z}

× J1 (kr)√L0

eiωt. (9)

3.2 Gravitating dry sandy mantle

The dynamical equation of motion for the initiallystressed dry sandy half-space under the effect ofgravity as given by Biot (1965) may be written as:

∂σrθ

∂r+

∂σzθ

∂z+

2σrθ

r+

∂z{(P − ρgz) ezθ}

−ρgz∂

∂r

{12

(∂v

∂r+

v

r

)}= ρ

∂2v

∂t2(10)

where v(r, z, t) is the displacement along θ direc-tion, ρ is the density, g is the acceleration due togravity and P is the compressive initial stress alongr direction. We also have N = ημ, where η is thesandy parameter and μ is the modulus of rigidity.

The inhomogeneity in the half-space is taken as:

μ=μ1 (1+a z) , ρ=ρ1, P =P1 (1+b z) . (11)

Using relation σrθ=2Nerθ and σzθ=2Nezθ in equa-tion (10), we get:

{ημ1 (1 + az) − ρgz

2

}{∂2v

∂r2− v

r2+

1r

∂v

∂r

}

+[ημ1 (1 + az) +

12{P1 + (P1b − gρ) z}

]∂2v

∂z2

+{

ημ1a +12

(P1b − ρg)}

∂v

∂z= ρ

∂2v

∂t2. (12)

We assume the solution of equation (12) in theform of

v = V (z)J1 (kr) eiωt (13)

where V (z) be solution of the equation given by

d2V

dz2+

{ημ1a + 1

2(P1b − ρg)

}[ημ1 (1 + az) + 1

2{P1 + (P1b − gρ) z}

]

dV

dz−

k2{ημ1 (1 + az) − ρgz

2

}[ημ1 (1 + az) + 1

2{P1 + (P1b − gρ) z}

]

×[

1 − ρω2

k2{ημ1 (1 + az) − ρgz

2

}

]

V = 0. (14)

Putting, V (z) = (ϕ (z)/[ημ1 (1 + az) + 1

2{P1 +

(P1b − gρ) z}]1/2) in equation (14), we get

d2ϕ

dz2+

14

{ημ1a + 1

2(P1b − gρ)

}2ϕ (z)

[ημ1 (1 + az) + 1

2{P1 + (P1b − gρ) z}

]2

−k2[ημ1 (1 + az) − ρgz

2

][ημ1 (1 + az) + 1

2{P1 + (P1b − gρ) z}

]

×[

1 − ρω2

k2{ημ1 (1 + az) − ρgz

2

}

]

ϕ (z) = 0

(15)

Now, substituting ϕ (z) = ϕ1 (δ) where

δ =2k[ημ1 (1 + az) + 1

2{P1 + (P1b − gρ) z}

][ημ1a + 1

2(P1b − gρ)

]

in equation (15), it may be reduced to

d2ϕ1 (δ)dδ2

+(

14δ2

+R

δ− A

)ϕ1 (δ) = 0 (16)

Existence of torsional surface waves in earth’s crustal layer 1415

where

R =P12μ1

+ c2

c21

2{

η(

ak

)+ 1

2

(P1μ1

bk− G)}

−12

(P12μ1

) (bk

) (η + P1

2μ1

)

{η(

ak

)+ 1

2

(P1μ1

bk− G)}2 ,

A =14−

12

(P12μ1

) (bk

)

{η(

ak

)+ 1

2

(P1μ1

bk− G)}

c = (ω/k)1/2 is the velocity of the torsional surfacewave. c1 = (μ1/ρ1)

1/2 is the velocity of the shearwave in the half-space. G = (gρ/μ1k) is Biot’sgravity parameter.

Equation (16) is known as the Whittaker’s equa-tion, whose solution may be given by (Whittakerand Watson 1990)

ϕ1 (δ) = D1 W(R/2√

A),0

(2√

A · δ)

+ D2 W−(R/2√

A),0

(−2

√A · δ)

.

Since the solution should vanish at z → ∞ (i.e., forδ → ∞), we may take the solution as:

ϕ1 (δ) = D1 W(R/2√

A),0

(2√

A · δ)

.

Expanding the Whittaker function up to linearterms, equation (13) takes the form

v = v1 (say)

=D1 e−

√Aδ(2√

A · δ) R

2√

A

[ημ1 (1 + az) + 1

2{P1 + (P1b − gρ) z}

]1/2

×

⎧⎪⎨

⎪⎩1 −

(R

2√

A− 1

2

)2

2√

⎫⎪⎬

⎪⎭J1 (kr) eiωt. (17)

4. Boundary conditions

The following boundary conditions must be satisfied

(i) At the free surface z=−H, the stress is van-ishing so that

v0 = 0 at z = −H.

(ii) The continuity of the displacement requiresthat

v0 = v1 at z = 0.

(iii) At the interface z=0, the continuity of thestress requires that

L0

∂v0

∂z= μ1

∂v1

∂zat z = 0.

Using boundary condition (i), equation (9) reducesto equation (18)

A1e(m1+

12α)H + A2e

−(m1− 12α)H = 0. (18)

Using boundary condition (ii) in equation (9) andequation (17), we get equation (19)

A1

1√L0

+ A2

1√L0

= D1 · S1 (19)

where

S1 =e−

√Aδ(2√

Aδ) R

2√

A

(ημ1 + P1

2

)1/2

⎧⎪⎨

⎪⎩1 −

(R

2√

A− 1

2

)2

2√

⎫⎪⎬

⎪⎭.

Using boundary condition (iii) in equation (9) andequation (17), we get equation (20).

−√

L0

(m1 +

12α

)A1 +

√L0

(m1 −

12α

)A2

= μ1D1S2 (20)

where

S2 = −e−√

Aδ ·2k√

A·(

ημ1 +P1

2

)−1/2

×(2√

Aδ) R

2√

A

⎧⎪⎨

⎪⎩1 −

(R

2√

A− 1

2

)2

2√

⎫⎪⎬

⎪⎭

+ 2kR e−√

(ημ1 +

P1

2

)−1/2(2√

Aδ) R

2√

A−1

×

⎧⎪⎨

⎪⎩1 −

(R

2√

A− 1

2

)2

2√

⎫⎪⎬

⎪⎭

+ e−√

Aδ · 2k ·(

ημ1 +P1

2

)−1/2 (2√

Aδ) R

2√

A

×

⎧⎪⎨

⎪⎩

(R

2√

A− 1

2

)2

2√

Aδ2

⎫⎪⎬

⎪⎭

− 12e−

√Aδ

(ημ1 +

P1

2

)−3/2 (2√

Aδ) R

2√

A

×{

ημ1a +12

(P1b − gρ)}⎧⎪⎨

⎪⎩1−

(R

2√

A− 1

2

)2

2√

⎫⎪⎬

⎪⎭

1416 Sumit Kumar Vishwakarma and Shishir Gupta

Eliminating A1, A2 and D1 using equations (18)–(20), we get

∣∣∣∣∣∣∣∣∣∣∣∣

e(m1+12α)H e−(m1− 1

2α)H 01√L0

1√L0

S1

−√

L0

(m1 +

12α

) √L0

(m1 −

12α

)μ1S2

∣∣∣∣∣∣∣∣∣∣∣∣

=0

On expanding the determinant, we get

cot

(

kH

√N0

L0

(c2

c20

− 1)− 1

4α2k2

)

=1

2αk+ μ1

L0

(S2S1k

)

√N0L0

(c2

c20− 1)− 1

4α2k2

(21)

where

S2

S1k= −2

√A+

R√Aδ

+2(

R

2√

A− 1

2

)2

δ

{2√

Aδ −(

R

2√

A− 1

2

)2}

− 12

[η(

ak

)+(

12

P1μ1

) (bk

)− 1

2G]

(η + P1

2μ1

) .

Equation (21) gives the required dispersion equa-tion of torsional surface wave in an inhomogeneousanisotropic earth’s crustal layer over a dry sandymantle when the upper boundary assumed to berigid.

5. Particular cases

Case I: When (1/α)→0, i.e., the directionalrigidities and density becomes constant, thenequation (21) reduces to

cot

(

kH

√N0

L0

(c2

c20

− 1))

=μ1

(S2S1k

)

L0

√N0L0

(c2

c20− 1) ,

which is the dispersion equation of torsional surfacewave in an anisotropic homogeneous layer underthe effect of rigid boundary.

Case II: When a → 0 and b → 0, i.e., whenthe half-space is homogeneous under the effect of

constant initial stress P1, then the equation (21)becomes

cot

(

kH

√N0

L0

(c2

c20

− 1)− 1

4α2k2

)

=1

2αk+ μ1

L0B1

√N0L0

(c2

c20− 1)− 1

4α2k2

where

B1 = −1 +12

(P12μ1

+ c2

c21

)

(η + P1

2μ1

)

+

(P12μ1

+ c2

c21

+ G2

)2

2(η + P1

2μ1

){4(η + P1

2μ1

)+ 1

G

(P12μ1

+ c2

c21

+ G2

)2}

+14

G(η + P1

2μ1

)

which is a dispersion equation of torsional surfacewave in an inhomogeneous anisotropic layer overa homogeneous isotropic half-space when upperboundary plane is rigid.

Case III: When α → ∞ and N0 = L0, i.e., thelayer is homogeneous and isotropic

cot

(

kH

√(c2

c20

− 1))

=μ1

L0

(S2S1k

)

√(c2

c20− 1) .

This gives the dispersion equation of torsional sur-face wave in a homogeneous isotropic layer over adry sandy mantle.

Case IV: When α→∞, a→0, P1→0 and N0 =L0, i.e., the layer and the half-space both arehomogeneous

cot

(

kH

√(c2

c20

− 1))

=μ1

L0

√(c2

c21− 1)

√(1 − c2

c20

) ,

which is a well known classical equation Love waveunder the effect of rigid boundary (Love 1944).

6. Numerical results and discussion

Based on the dispersion equation (21), numeri-cal results are provided to show the propagation

Existence of torsional surface waves in earth’s crustal layer 1417

Table 1. Values of various dimensionless parameters.

Figure 2 Figure 3 Figure 4 Figure 5 Figure 6 Figure 7 Figure 8

P1/2μ1 – – 0.2 0.2 0.2 0.4 0.4

a/k 0.2 0.2 – 0.2 0.2 0.2 0.2

b/k 1.5 1.5 1.5 – 1.5 1.5 1.5

αk 1.2 1.2 1.2 1.2 – 1.2 1.2

G 0.5 0.5 0.5 0.5 0.5 – 0.5

η 1.0 1.0 1.0 1.0 1.0 1.0 –

2.5 3 3.5 4 4.5 5 5.5 62

2.5

3

3.5

4

4.5

5

5.5

6

kH

c2/c

02

1 2 3 4 5

Curve no. 1 12P μ

1 0.2

2 0.4

3 0.6

4 0.8

5 1.0

Figure 2. Dimensionless phase velocity vs. dimensionlesswave number demonstrating the influence of compressiveinitial stress.

characteristics of torsional surface wave in the con-sidered layer over a dry sandy mantle under theeffect of gravity, initial stress and rigid bound-ary. The expansion of Whittaker function is takenas WR,0 (z) = e−z/2zR{1 − (R − 0.5)2/1!z}. Thenumerical data of various elastic constants andparameters have been taken from Gubbins (1990).In all the figures, curves have been plotted withvertical axis as dimensionless phase velocity (c2

0/c21)

against horizontal axis as dimensionless wave num-ber kH. It has been found that with the increase ofwave number, the phase velocity decreases rapidlyin each of the figures under the considered valuesof various parameters. The main attention is paidon the influence of sandy parameter (η) and Biot’sgravity parameter (G) along with the effect of inho-mogeneity factor αk, a/k, b/k and dimensionlessinitial stress (P1/2μ1) (as given in table 1). The val-ues of (c2

0/c21) , N0/L0 and μ1/L0 have been taken

as 0.2, 0.7 and 1.8, respectively in all the figures.Figure 2 discusses the dispersion curves for tor-

sional surface wave when compressive initial stress(P1/2μ1 > 0) has been taken into account in the

1.8 2 2.2 2.4 2.6 2.8 3 3.2 3.4

4

4.5

5

5.5

6

kH

c2 /c02 12

34

5

Curve no. 1 12P μ1 -0.1 2 -0.2 3 -0.3 4 -0.4 5 -0.5

Figure 3. Dimensionless phase velocity vs. dimensionlesswave number demonstrating the effect of tensile initialstress.

dry sandy mantle under the effect of gravity andrigid boundary. The value of P1/2μ1 for curve no.1, no. 2, no. 3, no. 4 and no. 5 has been taken as0.2, 0.4, 0.6, 0.8 and 1.0, respectively. Followingobservations and effects are obtained under theabove-considered values:

• As the compressive initial stress increases, thedimensionless phase velocity (c2

0/c21) increases at

a particular wave number.• The curves are accumulating at kH=2.5 show-

ing that although the compressive initial stressvaries, velocity remains constant at that partic-ular wave number.

• The curves being little far apart from each otherat lower phase velocity reveal that compressiveinitial stress has much dominance at large valuesof wave number.

Figure 3 shows the effect of tensile initial stress(P1/2μ1 < 0) in the dry sandy mantle under theeffect of gravity and rigid boundary. Here, the valueof tensile initial stress P1/2μ1 for curve no. 1, no. 2,no. 3, no. 4 and no. 5 have been taken as −0.1,

1418 Sumit Kumar Vishwakarma and Shishir Gupta

−0.2, −0.3, −0.4 and −0.5, respectively. Followingobservations have been made:

• It has been observed that decrease in tensileinitial stress decreases the velocity of torsionalsurface wave at the same frequency.

• Here, the curves seem converging at kH = 3.5thereby making the phase velocity constant atc2/c2

0 = 3.5 at various magnitude of tensile initialstress. Whereas its dominant effect is visible athigher phase velocity and lower wave number.

2.5 3 3.5 4 4.5 5 5.5 6

2.5

3

3.5

4

4.5

5

5.5

6

kH

c2/c

02

12345

Curveno. /a k

1 0.2

2 0.4

3 0.6

4 0.8

5 1.0

Figure 4. Dimensionless phase velocity vs. dimensionlesswave number demonstrating the influence of inhomogeneityassociated with rigidity of the half-space.

2.5 3 3.5 4 4.5 5 5.5 6

2.5

3

3.5

4

4.5

5

5.5

kH

c2/c

02

1 2 3 4 5

Curveno. /b k

1 1.52 2.0

3 2.5

4 3.0

5 3.5

Figure 5. Dimensionless phase velocity vs. dimensionlesswave number demonstrating the effect of inhomogeneityassociated with initial stress of the half-space.

Figure 4 has been plotted to have a better under-standing of the effect of the inhomogeneity param-eter (a/k) incorporated in the modulus of rigidityon the torsional wave velocity. The value of (a/k)has been varied from 0.2 to 1 (i.e., 0.2 for curve no.1, 0.4 for curve no. 2, 0.6 for curve no. 3, 0.8 forcurve no. 4 and 1.0 for curve no. 5). We observedthat

• As the dimensionless inhomogeneity factor (a/k)increases, the phase velocity of torsional surface

2.5 3 3.5 4 4.5 5 5.5 6

2

2.5

3

3.5

4

4.5

5

5.5

6

kH

c2 /c02

12

34

5

Curveno. kα

1 1.2

2 1.4

3 1.6

4 1.8

5 2.0

Figure 6. Dimensionless phase velocity vs. dimensionlesswave number demonstrating the influence of inhomogeneityassociated with the layer.

1 2 3 4 5 61.5

2

2.5

3

3.5

4

4.5

5

5.5

6

kH

c2 /c02

12

34

5

Curveno. G

1 1.2

2 1.4

3 1.6

4 1.8

5 2.0

Figure 7. Dimensionless phase velocity vs. dimensionlesswave number demonstrating the effect of Biot’s gravityparameter.

Existence of torsional surface waves in earth’s crustal layer 1419

wave at a particular frequency also increases,which justifies the fact that velocity of the sur-face wave is directly proportional to the rigidityof the medium.

• The curves shift closer to each other as the valueof (a/k) increases, reveals that it has a negligibleeffect for the higher magnitude.

2.5 3 3.5 4 4.5 5 5.5 62.5

3

3.5

4

4.5

5

5.5

6

kH

c2 /c02

1 2 3 4 5

Curveno.

η

1 1.0

2 2.0

3 2.5

4 3.5

Figure 8. Dimensionless phase velocity vs. dimension-less wave number demonstrating the influence of sandyparameter.

In figure 5, an attempt has been made to comeout with effect of inhomogeneity factor (b/k). Thevalue of (b/k) for curve no. 1, no. 2, no. 3, no. 4and no. 5 are considered as 1.5, 2.0, 2.5, 3.0 and3.5. It has been found that:

• Torsional wave velocity increases for the increas-ing value of (b/k) at a particular frequency,prominent effect of which is visible at higherfrequency.

• Similar to figure 2, here also the curvesare accumulating at a single point denotingalthough inhomogeneity parameter b/k varies,phase velocity remains constant for the samefrequency.

Figure 6 signifies the effect of inhomogeneity factorαk present in the directional rigidities and densityof the layer. The value of αk for curve no. 1, no. 2,no. 3, no. 4 and no. 5 has been taken as 1.2, 1.4,1.6, 1.8 and 2.0, respectively. Following conclusionsmay be drawn from the figure:

• These curves show that the phase velocityof torsional surface wave decreases remarkablyas the value of αk increases from 1.2 to 2.0.

• The curvature of the curves being equally apartshows the predominant influence of the inhomo-geneity parameter associated with the layer.

Figure 7 shows the study of phase velocity undera wide range of Biot’s gravity parameter G. Here

Figure 9. Snapshot of graphical user interface (GUI) developed in MATLAB 7.5.

1420 Sumit Kumar Vishwakarma and Shishir Gupta

the value of G for curve no.1, no. 2, no. 3, no. 4and no. 5 are taken as 1.2, 1.4, 1.6, 1.8 and 2.0,respectively. It has been observed that

• The phase velocity of torsional surface wave inthe layer increases significantly as the value of Gincreases in the above-mentioned range.

• The effect of dimensionless gravity parameter Galmost vanishes as it approaches kH = 6.0.

• The curves being steeper between kH = 1.0 and3.0 shows that G has a perfect influence over thephase velocity of torsional surface wave.

Figure 8 describes the effect of sandy parameterη on the velocity of torsional surface wave for thevarious values of η, i.e., 1.0, 2.0, 2.5 and 3.5 forcurve nos. 1–4, respectively. Following results maybe drawn:

• The curves reflect that in the presence of com-pressive initial stress and the rigid bound-ary plane, as the value of sandy parameter ηincreases, the phase velocity of torsional wavealso increases.

• For η = 1, the medium turn out to be perfectelastic thereby allowing torsional surface waveto propagate with least velocity as compared toother values of η (i.e., 2.0, 2.5, 3.5) for which themedium becomes dry and sandy. Hence it can beconcluded that under the above-considered valueof various parameters, the possibility of torsionalwave propagation in the layer is least when thehalf-space is elastic as compared to the case whenthe half-space is dry and sandy.

Figure 9 represents a screenshot of graphical userinterface (GUI) software in MATLAB demonstrat-ing the graph plotted in figure 2 as a sample. ThisGUI generalizes the finding of the present paperby allowing one to vary the ranges of differentdimensionless parameter and also by providing dif-ferent values to the various parameters involved.This will help one to observe the variation on thephase velocity of torsional surface wave againstdimensionless wave number.

7. Conclusion

Propagation of torsional surface wave in an inho-mogeneous anisotropic earth’s crustal layer over adry sandy mantle when upper boundary plane isrigid has been investigated analytically. The dis-persion equation thus obtained in a closed formreduces into classical equation of Love wave wheninhomogeneity parameters and initial stress isneglected thereby validating the solution of theproblem discussed. We find that as the compressiveinitial stress increases, the phase velocity increases

and as the tensile initial stress decreases the phasevelocity also decreases. It is also found that theincreasing value of inhomogeneity factor in rigid-ity and initial stress decreases the phase velocityof the torsional surface wave. The effect of Biot’sgravity parameter has also come out prominently.It has been studied that as the value of Biot’s grav-ity parameter increases, the velocity also increases.Study has also been made on sandy parameter andfound that under a rigid boundary plane, torsionalsurface wave propagates with more ease when thehalf-space is dry and sandy rather than being elas-tic. Graphical user interface software has beendeveloped in MATLAB to generalize the results offigures 2–8 so as to study the effect of compres-sive initial stress, tensile initial stress, inhomogene-ity parameter and wave number on phase velocityof torsional wave with various sets of values. Thepresent study may be useful for the study of seismicwaves generated by artificial explosions.

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MS received 8 May 2012; revised 14 March 2013; accepted 17 March 2013