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(Vidensk. Selsk. Skr. 6t0 Rsekke Naturvidenskabelig og Mathematisk afd. 3d*,
Bd. i.)
On Waves Propagated along the Plane Surface of an Elastic
Solid. By Lord RAYLEIOH, D.O.L., F.R.S.
[Head November 12th, 1885.]
It is proposed to investigate the behaviour of waves upon the plane
free surface of an infinite homogeneous isotropic elastic solid, their
character being such that the disturbance is confined to a superficial
region, of thickness comparable with the wave-length. The case is
thus analogous to tliat of deep-water waves, only that the potential
energy here depends upon elastic resilience instead of upon gravity.*
Denoting the displacements by a, /3, y, and the dilatation by 0, we
have the usual equations
=z(X + fl)f+^a *° (1)'
in which e = ^ + f.+ p. (2).
ax ay dz
If a, /i3, y all vary as eip\ equations (1) become
+/*V9+Pi>la = 0, &C (3).
* The statical problem of the deformation of an elastic solid by a harmonic appli-
cation of pressure to its surface has been treated by Prof. G. Darwin, Phil. Mag.,
Dec, 1882. [Jan. 1886.—See also Camb. Math. Trip. Ex., Jan. 20, 1875, Ques-
tion IV.]
1885.] the Plane Surface of an Elastic Solid. 5
Differentiating equations (3) in order with respect to x, y, z, and
adding, we get
(V3 + fca)0 = O (4),
in which fc8 = ppa/(x+2/*) (5)-
Again, if we put ft2 = pp2 / f» (6),
equations (3) take the form
< * + * ) . _ ( l - * ) « fa (7).
A particular solution of (7) is*
_ 1 d8
n_ 1 dd _ 1 dd ,Q,
a
-~WTx' P--T**? y-~"WTz W ;
in order to complete which it is only necessary to add complementary
terms u, v, w satisfying the system of equations
= 0 (9),
+ + 0
dx dy dz
For the purposes of the present problem we take the free surface as
the plane z = 0, and assume that, as functions of a? and y, the dis-
placements are proportional to ef/*, e = - $ . - , y - ^ . - a*).
For the complementary terms, which must also contain ev*, e & c (l5) *
whence, as before, on the assumption that the disturbance is limited
to a superficial stratum,
utzAe-*, v = B&"% w = Oe— (16),
where * s9 = / 8 +0 9 - f c f (17).
In order to satisfy (10), the coefficients in (16) must be subject to
the relation
ifA+igB-8(J=Q (18).
The complete values of a, /3, y may now be written
a = - %Le-"+Ae-\ 0 = - | f e'"+Be-', y = i? e-»+Cfe- ' . , . (19),
in which A, B, 0 are subject to (18) ; and the next step is to express
the boundary conditions for the free surface. The two components
of tangential stress must vanish, when z = 0, and these are propor-
,. , , dQ . dy dy . dational to —• + -/-, -f- + -r-,dz dy dx dz
respectively. Hence
sB^+igO, sA = 2j£+if0 (20).
Substituting from (20) in (18), we find
Cf(*8+/9+09)fc9+2r(/M-08)=O (21).
We have still to introduce the condition that the normal traction is
tero at the surface. We have, in general,
1885.] the Plane Surface of an Elastic Solid.
or, if we express X in terms of /x, h, h,
so that the condition is
or, on substitution for r2 of its value from (12),
W-2(f+g2)-2h2sO=0 (22).
By eliminating 0 between (21) and (22), we obtain the equation by
which the time of vibration is determined as a function of the wave-
lengths and of the properties of the solid. I t is
{V-2 (f+g2)} {s2+f+g2} + 4rS(/a+2) = 0,
or, by (17), {2(f+g2)-Vy=4).
Hence h?a = if { — e"n+-5433e""} eipt eVs ein
{ } eipte*ei9V [ (30).
ipt
If we suppose the motion to be in two dimensions only, we may put
g = 0; so that /3 = 0, and
in which k = -9554/, s = -2954/. ; (32).
For a progressive wave we may take simply the real parts of (31).
Thus ^8a / / = (e-'»- •5433e-1) sin (pt+fx) }
/ i 8 y / /= (e-A-l'840e-M)cos (pt+Jx) )
1885.] the Plane Surface of an Elastic Solid. 9
The velocity of propagation is p/f, or <9554v/(/*//o), in which
,/{ft I p) is the velocity of purely transverse plane waves. The sur-
face waves now under consideration move, therefore, rather more
slowly than these.
From (32), (33), we see that a vanishes for all values of x and t
when el"-0' = '5433, i.e., when/* = -8659. Thus, if \ ' be the wave-
length (2TT//), the horizontal motion vanishes at a depth equal to
*1378\'. On the other hand, there is no finite depth at which the
vertical motion vanishes.
To find the motion at the surface itself, we have only to put z — 0
in (33). "We may drop at the same time the constant multiplier
(A3//) which has no present significance. Accordingly,
o = '4567 sin (pt+fx)")Kr J J
[ (34),
y = - ' 840cos (^+ /a j ) ) .
showing that the motion takes place in elliptio orbits, whose vertical
axis is nearly the double of the horizontal axis.
The expressions for stationary vibrations may be obtained from
(30) by addition to the similar equations obtained by changing the
sign of p, and similar operations with respect to / and g. Dropping
an arbitrary multiplier, we may write
a = —/ { —e'"4-'5433e"'i>] cos pi sin fx cos gy ")
/3 = — g { — e"" +"54336""} cosptcosfx singy f (35),
y = r { e"n—l1840e""} cospt cos fx cos gy )
in which r = (fi+gi), s = t2954\/(/a + gr8) (36).
As before, the horizontal motion vanishes at a depth such that
z = -8659.
We will now examine how far the numerical results are affected when
we take into account the finite compressibility of all natural bodies.
The ratio of the elastic constants is often stated by means of the
number expressing the ratio of lateral contraction to longitudinal ex-
tension when a bar of the material is strained by forces applied to its
ends. According to a theory now generally discarded, this ratio (