Two-dimensional planar waves
edit
Two-dimensional planar pressure waves can be described in Cartesian coordinates by decomposing the wave number into x and y components,
p
(
x
,
y
,
t
)
=
P
e
j
(
ω
t
−
K
x
x
−
K
y
y
)
.
{\displaystyle \mathbf {p} (x,y,t)=\mathbf {P} e^{j(\omega t-K_{x}x-K_{y}y)}.}
Substituting into the general wave equation yields:
∇
2
p
−
1
c
o
2
∂
2
p
∂
t
2
=
0
,
{\displaystyle \nabla ^{2}\mathbf {p} -{\frac {1}{c_{o}^{2}}}{\frac {\partial ^{2}\mathbf {p} }{\partial t^{2}}}=0,}
P
(
−
K
x
2
−
K
y
2
)
+
ω
2
c
o
2
P
=
0
,
{\displaystyle \mathbf {P} (-K_{x}^{2}-K_{y}^{2})+{\frac {\omega ^{2}}{c_{o}^{2}}}\mathbf {P} =0,}
K
=
ω
c
o
=
K
x
2
+
K
y
2
.
{\displaystyle K={\frac {\omega }{c_{o}}}={\sqrt {K_{x}^{2}+K_{y}^{2}}}.}
The wave number becomes a vector quantity and may be expressed using the directional cosines,
K
→
=
K
x
ı
^
+
K
y
ȷ
^
=
K
cos
(
α
)
ı
^
+
K
cos
(
β
)
ȷ
^
.
{\displaystyle {\vec {K}}=K_{x}{\boldsymbol {\hat {\imath }}}+K_{y}{\boldsymbol {\hat {\jmath }}}=K\cos(\alpha ){\boldsymbol {\hat {\imath }}}+K\cos(\beta ){\boldsymbol {\hat {\jmath }}}.}
Obliquely incident planar waves
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Consider an obliquely incident planar wave in medium 1 which approaches the boundary at an angle
θ
i
{\displaystyle \theta _{i}}
with respect to the normal. Part of the wave is reflected back into medium 1 at an angle
θ
r
{\displaystyle \theta _{r}}
and the remaining part is transmitted to medium 2 at an angle
θ
t
{\displaystyle \theta _{t}}
.
p
1
=
P
i
e
j
(
ω
t
−
cos
θ
i
K
1
x
−
sin
θ
i
K
1
y
)
+
P
r
e
j
(
ω
t
+
cos
θ
r
K
1
x
−
sin
θ
r
K
1
y
)
{\displaystyle \mathbf {p_{1}} =\mathbf {P_{i}} e^{j(\omega t-\cos \theta _{i}K_{1}x-\sin \theta _{i}K_{1}y)}+\mathbf {P_{r}} e^{j(\omega t+\cos \theta _{r}K_{1}x-\sin \theta _{r}K_{1}y)}}
p
2
=
P
t
e
j
(
ω
t
−
cos
θ
t
K
2
x
−
sin
θ
t
K
2
y
)
{\displaystyle \mathbf {p_{2}} =\mathbf {P_{t}} e^{j(\omega t-\cos \theta _{t}K_{2}x-\sin \theta _{t}K_{2}y)}}
Reflection and transmission of obliquely incident planar wave.
Notice that the wave frequency does not change across the boundary, however the specific acoustic impedance does change from medium 1 to medium 2. The propagation speed is different in each medium, so the wave number changes across the boundary. There are two boundary conditions to be satisfied.
The acoustic pressure must be continuous at the boundary.
The particle velocity component normal to the boundary must be continuous at the boundary.
Imposition of the first boundary condition yields
p
1
(
x
=
0
)
=
p
2
(
x
=
0
)
,
{\displaystyle \mathbf {p_{1}} (x=0)=\mathbf {p_{2}} (x=0),}
P
i
e
−
j
sin
θ
i
K
1
y
+
P
r
e
−
j
sin
θ
r
K
1
y
=
P
t
e
−
j
sin
θ
t
K
2
y
.
{\displaystyle \mathbf {P_{i}} e^{-j\sin \theta _{i}K_{1}y}+\mathbf {P_{r}} e^{-j\sin \theta _{r}K_{1}y}=\mathbf {P_{t}} e^{-j\sin \theta _{t}K_{2}y}.}
For continuity to hold, the exponents must be all equal to each other
K
1
sin
θ
i
=
K
1
sin
θ
r
=
K
2
sin
θ
t
.
{\displaystyle K_{1}\sin \theta _{i}=K_{1}\sin \theta _{r}=K_{2}\sin \theta _{t}.}
This has two implications. First, the angle of incident waves is equal to the angle of reflected waves,
sin
θ
i
=
sin
θ
r
{\displaystyle \sin \theta _{i}=\sin \theta _{r}}
and second, Snell's law is recovered,
sin
θ
i
c
1
=
sin
θ
t
c
2
.
{\displaystyle {\frac {\sin \theta _{i}}{c_{1}}}={\frac {\sin \theta _{t}}{c_{2}}}.}
The first boundary condition can be expressed using the pressure reflection and transmission coefficients
1
+
R
=
T
.
{\displaystyle 1+\mathbf {R} =\mathbf {T} .}
Imposition of the second boundary condition yields
u
1
x
(
x
=
0
)
=
u
2
x
(
x
=
0
)
,
{\displaystyle \mathbf {u_{1x}} (x=0)=\mathbf {u_{2x}} (x=0),}
u
i
cos
θ
i
+
u
r
cos
θ
r
=
u
t
cos
θ
t
.
{\displaystyle \mathbf {u_{i}} \cos \theta _{i}+\mathbf {u_{r}} \cos \theta _{r}=\mathbf {u_{t}} \cos \theta _{t}.}
Using the specific acoustic impedance definition yields
P
i
r
1
cos
θ
i
−
P
r
r
1
cos
θ
r
=
P
t
r
2
cos
θ
t
.
{\displaystyle {\frac {\mathbf {P_{i}} }{r_{1}}}\cos \theta _{i}-{\frac {\mathbf {P_{r}} }{r_{1}}}\cos \theta _{r}={\frac {\mathbf {P_{t}} }{r_{2}}}\cos \theta _{t}.}
Using the reflection coefficient, the transmission coefficient and the acoustic impedance ratio leads to
1
−
R
=
cos
θ
t
cos
θ
i
T
ζ
.
{\displaystyle 1-\mathbf {R} ={\frac {\cos \theta _{t}}{\cos \theta _{i}}}{\frac {\mathbf {T} }{\zeta }}.}
Solving for the pressure reflection coefficient yields:
R
=
T
−
1
=
cos
θ
i
cos
θ
t
ζ
−
1
cos
θ
i
cos
θ
t
ζ
+
1
=
r
2
cos
θ
t
−
r
1
cos
θ
i
r
2
cos
θ
t
+
r
1
cos
θ
i
.
{\displaystyle \mathbf {R} =\mathbf {T} -1={\frac {{\frac {\cos \theta _{i}}{\cos \theta _{t}}}\zeta -1}{{\frac {\cos \theta _{i}}{\cos \theta _{t}}}\zeta +1}}={\frac {{\frac {r_{2}}{\cos \theta _{t}}}-{\frac {r_{1}}{\cos \theta _{i}}}}{{\frac {r_{2}}{\cos \theta _{t}}}+{\frac {r_{1}}{\cos \theta _{i}}}}}.}
Solving for the pressure transmission coefficient yields:
T
=
R
+
1
=
2
cos
θ
i
cos
θ
t
ζ
cos
θ
i
cos
θ
t
ζ
+
1
=
2
r
2
cos
θ
t
r
2
cos
θ
t
+
r
1
cos
θ
i
.
{\displaystyle \mathbf {T} =\mathbf {R} +1={\frac {2{\frac {\cos \theta _{i}}{\cos \theta _{t}}}\zeta }{{\frac {\cos \theta _{i}}{\cos \theta _{t}}}\zeta +1}}={\frac {2{\frac {r_{2}}{\cos \theta _{t}}}}{{\frac {r_{2}}{\cos \theta _{t}}}+{\frac {r_{1}}{\cos \theta _{i}}}}}.}
Solving for the specific acoustic impedance ratio yields
ζ
=
cos
θ
t
cos
θ
i
(
1
+
R
1
−
R
)
=
cos
θ
t
cos
θ
i
(
T
2
−
T
)
.
{\displaystyle \zeta ={\frac {\cos \theta _{t}}{\cos \theta _{i}}}{\Big (}{\frac {1+\mathbf {R} }{1-\mathbf {R} }}{\Big )}={\frac {\cos \theta _{t}}{\cos \theta _{i}}}{\Big (}{\frac {\mathbf {T} }{2-\mathbf {T} }}{\Big )}.}
Rayleigh reflection coefficient
edit
The Rayleigh reflection coefficient relates the angle of incidence from Snell's law to the angle of transmission in the equations for
R
{\displaystyle \mathbf {R} }
,
T
{\displaystyle \mathbf {T} }
and
ζ
{\displaystyle \zeta }
. From the trigonometric identity,
cos
2
θ
t
+
sin
2
θ
t
=
1
{\displaystyle \cos ^{2}\theta _{t}+\sin ^{2}\theta _{t}=1}
and using Snell's law,
cos
θ
t
=
1
−
(
c
2
c
1
sin
θ
i
)
2
.
{\displaystyle \cos \theta _{t}={\sqrt {1-{\Big (}{\frac {c_{2}}{c_{1}}}\sin \theta _{i}{\Big )}^{2}}}.}
Notice that for the angle of transmission to be real,
c
2
<
c
1
sin
θ
i
{\displaystyle c_{2}<{\frac {c_{1}}{\sin \theta _{i}}}}
must be met. Thus, there is a critical angle of incidence such that
sin
θ
c
=
c
1
c
2
.
{\displaystyle \sin {\theta _{c}}={\frac {c_{1}}{c_{2}}}.}
The Rayleigh reflection coefficient are substituted back into the equations for
R
{\displaystyle \mathbf {R} }
,
T
{\displaystyle \mathbf {T} }
and
ζ
{\displaystyle \zeta }
to obtain expression only in term of impedance and angle of incidence.
R
==
cos
θ
i
ζ
−
1
−
(
c
2
c
1
sin
θ
i
)
2
cos
θ
i
ζ
+
1
−
(
c
2
c
1
sin
θ
i
)
2
{\displaystyle \mathbf {R} =={\frac {\cos \theta _{i}\zeta -{\sqrt {1-{\Big (}{\frac {c_{2}}{c_{1}}}\sin \theta _{i}{\Big )}^{2}}}}{\cos \theta _{i}\zeta +{\sqrt {1-{\Big (}{\frac {c_{2}}{c_{1}}}\sin \theta _{i}{\Big )}^{2}}}}}}
T
=
2
cos
θ
i
ζ
cos
θ
i
ζ
+
1
−
(
c
2
c
1
sin
θ
i
)
2
{\displaystyle \mathbf {T} ={\frac {2\cos \theta _{i}\zeta }{\cos \theta _{i}\zeta +{\sqrt {1-{\Big (}{\frac {c_{2}}{c_{1}}}\sin \theta _{i}{\Big )}^{2}}}}}}
ζ
=
1
−
(
c
2
c
1
sin
θ
i
)
2
cos
θ
i
(
1
+
R
1
−
R
)
=
1
−
(
c
2
c
1
sin
θ
i
)
2
cos
θ
i
(
T
2
−
T
)
.
{\displaystyle \zeta ={\frac {\sqrt {1-{\Big (}{\frac {c_{2}}{c_{1}}}\sin \theta _{i}{\Big )}^{2}}}{\cos \theta _{i}}}{\Big (}{\frac {1+\mathbf {R} }{1-\mathbf {R} }}{\Big )}={\frac {\sqrt {1-{\Big (}{\frac {c_{2}}{c_{1}}}\sin \theta _{i}{\Big )}^{2}}}{\cos \theta _{i}}}{\Big (}{\frac {\mathbf {T} }{2-\mathbf {T} }}{\Big )}.}