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3.2 Conversion of the PO Integrals to the Canonical Form 63

and

 

 

 

 

 

Ih = F

 

eikr cosϕ) sin ξ

dξ ,

with ϕ < π ,

(3.23)

 

cos ξ + cos ϕ0

Ih = F

 

eikr cos+ϕ) sin ξ

dξ ,

with ϕ > π ,

(3.24)

 

cos ξ + cos ϕ0

where, as is shown in Figure 3.2, the integration contour F skirts above the pole

ξ = π ϕ0.

In Figures 3.3 and 3.4, we introduce two additional contours G1 and G2, related to the cases ϕ < π and ϕ > π , respectively. In the dashed regions of these figures, the relations Im cosϕ) > 0 and Im cos+ ϕ) > 0 are valid, which guarantees the convergence of integrals Is and Ih. We then apply the Cauchy residue theorem

Figure 3.3 Integration contours F and G1 for the case ϕ < π . In the shaded regions, Im cosϕ) > 0.

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64 Chapter 3 Wedge Diffraction: The Physical Optics Field

Figure 3.4 Integration contours F and G2 for the case ϕ > π . In the shaded regions, Im cos+ ϕ) > 0.

to the integrals over the closed contours F G1,2 (they are closed at the infinity, ξ = ±∞) and obtain

Is =

eikr cosϕ)

 

dξ +

2π i

 

eikr cos+ϕ0),

with 0 ≤ ϕ π ϕ0,

cos ξ

+

cos ϕ

0

sin ϕ

0

G1

 

 

 

 

 

 

(3.25)

Is =

Is =

and

Is =

G1

G2

G2

eikr cosϕ)

 

 

dξ ,

with π ϕ0 < ϕ < π ,

(3.26)

cos ξ + cos ϕ0

 

eikr cos+ϕ)

 

 

dξ ,

with π < ϕ < π + ϕ0,

(3.27)

cos ξ + cos ϕ0

 

eikr cos+ϕ)

 

 

dξ +

2π i

eikr cosϕ0),

with π + ϕ0 ϕ ≤ 2π .

cos ξ

+

cos ϕ

0

 

sin ϕ

 

 

 

 

0

 

(3.28)

 

 

 

 

 

 

 

 

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3.2 Conversion of the PO Integrals to the Canonical Form 65

In these equations, we change with integration variable ξ by ζ + ϕ in the region 0 ≤ ϕ < π , and by ζ + 2π ϕ in the region π < ϕ < 2π . As a result, the integrals in Equations (3.25) to (3.28) are transformed into the integrals over the contour D0 shown in Figure 2.6:

 

eikr cosϕ)

dξ =

 

eikr cos ζ dζ

with 0 ≤ ϕ < π

 

 

 

 

 

,

(3.29)

G1

cos ξ + cos ϕ0

D0

cos ϕ0 + cos+ ϕ)

and

 

 

 

 

 

 

 

 

eikr cos+ϕ)

dξ =

 

eikr cos ζ dζ

with π ϕ < 2π .

 

 

 

 

 

,

(3.30)

G2

cos ξ + cos ϕ0

D0

cos ϕ0 + cosϕ)

We omit similar transformations for integral Ih and present only their results:

Ih =

Ih =

Ih =

Ih =

 

eikr cos ζ sin+ ϕ)

dζ

+

2π ieikr cos+ϕ0),

 

 

with 0

ϕ

π

ϕ

,

 

cos ϕ0 + cos+ ϕ)

 

 

D0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(3.31)

 

eikr cos ζ sin+ ϕ)

dζ ,

with π

ϕ

0

ϕ < π ,

 

 

 

 

 

 

(3.32)

D0

cos ϕ0 + cos+ ϕ)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

eikr cos ζ sinϕ)

dζ ,

with π

ϕ

π

+

ϕ

,

 

 

 

 

 

 

(3.33)

 

cos ϕ0 + cosϕ)

 

 

 

 

 

 

D0

 

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

eikr cos ζ sinϕ)

dζ

+

2π ieikr cosϕ0),

 

 

with π

+

ϕ

0

ϕ

2π .

D0

cos ϕ0 + cosϕ)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(3.34)

Finally one can represent the scattered field in the following form:

(0)

 

u0eikr cos+ϕ0),

with

0 ≤ ϕ π ϕ0

us

= u0vs+(kr, ϕ, ϕ0) + 0,

 

with π

ϕ0 < ϕ < π ,

 

= u0vs(kr, ϕ, ϕ0) +

 

 

 

 

 

(0)

0,

u0eikr cosϕ0),

with π

ϕ π + ϕ0

us

with π

ϕ0 < ϕ < 2π ,

and

 

 

 

 

+

 

 

 

 

 

 

 

 

(0)

 

u0eikr cos+ϕ0),

with 0

ϕ π ϕ0

uh

= u0vh+(kr, ϕ, ϕ0) + 0,

 

with π

ϕ0 < ϕ < π ,

 

= u0vh(kr, ϕ, ϕ0) +

 

 

 

 

 

(0)

0,

u0eikr cosϕ0),

with π

ϕ π + ϕ0

uh

with π

ϕ0 < ϕ < 2π ,

 

 

 

 

 

+

 

(3.35)

(3.36)

(3.37)

(3.38)

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66 Chapter 3 Wedge Diffraction: The Physical Optics Field

 

where

 

 

 

 

 

 

 

 

 

 

 

 

 

v±(kr, ϕ, ϕ )

=

i sin ϕ0

 

 

eikr cos ζ

 

 

 

 

 

 

 

 

dζ ,

(3.39)

 

 

 

 

 

 

s

0

 

2π

D0

 

cos ϕ0 + cos± ϕ)

 

and

 

 

 

 

 

 

 

 

 

 

 

 

 

v±(kr, ϕ, ϕ

 

)

 

 

1

 

 

 

eikr cos ζ sin± ϕ)

dζ .

(3.40)

0

= ± i2π

 

 

 

h

 

 

D0

cos ϕ0 + cos± ϕ)

 

The above expressions for us(0) and uh(0) determine the PO field scattered by the face ϕ = 0 of the wedge. They are valid under the condition 0 ≤ ϕ0 < α π .

However, in the case α π < ϕ0 < π , the other face (ϕ = α) is also illuminated and generates the additional scattered field. This field is also determined by Equations (3.35) to (3.38), where one should replace ϕ by α ϕ and ϕ0 by α ϕ0. Thus, the PO field us(0) scattered in this case by both faces of the wedge is described by the following equations:

u(0)

=

u

0[

v+(kr, ϕ, ϕ )

+

v(kr, α

ϕ, α

ϕ

)

]

 

 

 

 

 

 

 

 

 

 

 

s

 

s

0

s

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u0eikr cos+ϕ0),

with 0 ≤ ϕ π ϕ0

 

π .

 

 

 

 

(3.41)

 

 

+ 0,

 

 

 

with π

ϕ0

< ϕ < α

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u(0)

=

u

0[

v+(kr, ϕ, ϕ )

+

v+(kr, α

ϕ, α

ϕ

)

]

,

with α

π < ϕ < π ,

 

 

 

s

 

s

0

s

 

 

0

 

 

 

 

 

 

 

(3.42)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u(0)

=

u

0[

v(kr, ϕ, ϕ )

+

v+(kr, α

ϕ, α

ϕ

)

]

,

with π < ϕ < 2α

π

ϕ

,

s

 

s

0

s

 

 

0

 

 

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(3.43)

and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u(0)

=

u

0[

v(kr, ϕ, ϕ )

+

v+(kr, α

ϕ, α

ϕ

)

]

 

 

 

 

 

 

 

 

 

 

 

s

 

s

0

s

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u0eikr cos(2αϕϕ0),

 

with 2α π ϕ0 < ϕ < α.

 

 

(3.44)

Similar equations are valid for the field uh(0) in the case α π < ϕ0 < π :

 

 

 

 

 

uh(0) = u0[vh+(kr, ϕ, ϕ0) + vh(kr, α ϕ, α ϕ0)]

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u0eikr cos+ϕ0),

with 0

ϕ π ϕ0

 

π ,

 

 

 

 

(3.45)

 

 

+ 0,

 

 

 

with π

ϕ0 < ϕ < α

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

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cos ϕ + cos ϕ0

 

3.3 Ray Asymptotics for the PO Diffracted Field 67

uh(0) = u0[vh+(kr, ϕ, ϕ0) + vh+(kr, α ϕ, α ϕ0)],

with α π < ϕ < π ,

(3.46)

 

 

 

uh(0) = u0[vh(kr, ϕ, ϕ0) + vh+(kr, α ϕ, α ϕ0)],

with π < ϕ < 2α π ϕ0,

 

 

 

(3.47)

uh(0) = u0[vh(kr, ϕ, ϕ0) + vh+(kr, α ϕ, α ϕ0)]

 

 

+ u0eikr cos(2αϕϕ0),

with 2α π ϕ0 < ϕ < α.

(3.48)

As is seen in Equations (3.41) to (3.48), the PO scattered field consists of the reflected plane waves and the diffracted part described by functions vs± and vh±. Simple asymptotic expressions for the functions vs,h± and for the diffracted field are derived in the next section.

3.3 RAY ASYMPTOTICS FOR THE PO DIFFRACTED FIELD

The relationships us = Ez and uh = Hz exist between the acoustic and electromagnetic

fields studied in this section.

Again, as in Section 2.4, we introduce in the integrals (3.39) and (3.40) the new variable s = 2eiπ/4 sin ζ2 and transform functions vs,h± as

v±(kr, ϕ, ϕ )

=

sin ϕ0

ei(kr+π/4)

 

 

 

 

s

0

2

π

v±(kr, ϕ, ϕ )

 

1

 

 

ei(kr+π/4)

 

 

 

 

 

 

 

 

= √

 

 

 

h

0

2

π

ekrs2 ds

−∞ [cos ϕ0 + cos± ϕ)] cos ζ , 2

sin± ϕ)ekrs2 ds

−∞ [cos ϕ0 + cos± ϕ)] cos ζ . 2

Then the standard saddle point technique leads to the asymptotic expressions

v±(kr, ϕ, ϕ )

 

 

sin ϕ0

 

ei(kr+π/4)

,

 

cos ϕ + cos ϕ0

 

 

 

s

0

 

2π kr

 

 

 

and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

v±(kr, ϕ, ϕ )

sin ϕ

 

 

 

ei(kr+π/4)

.

 

 

 

 

 

h

0

 

 

 

 

2π kr

 

(3.49)

(3.50)

(3.51)

(3.52)

These asymptotics are valid under the conditions kr| cos± ϕ0)/2| 1, that is, away from the geometrical optics boundaries, where the diffracted field has a ray structure and can be interpreted in terms of edge diffracted rays.

TEAM LinG


68 Chapter 3 Wedge Diffraction: The Physical Optics Field

In view of Equations (3.51) and (3.52), the ray asymptotics for the diffracted part of the fields (3.41) to (3.44) and (3.45) to (3.48) can be written in the following form:

(0)d

u0 f

(0)

 

ei(kr+π/4)

 

us

 

 

, ϕ0)

 

 

 

 

 

(3.53)

 

 

2π kr

 

and

 

 

 

 

 

 

 

 

 

 

 

(0)d

u0 g

(0)

 

ei(kr+π/4)

 

uh

 

, ϕ0)

 

 

.

(3.54)

 

2π kr

 

 

 

 

 

 

 

 

 

 

 

 

The directivity patterns of these diffracted rays are different for the situations with one or two illuminated faces. In the case 0 < ϕ0 < α π , when only the face ϕ = 0 is illuminated by the incident wave,

f (0), ϕ0) =

 

sin ϕ0

 

 

g(0), ϕ0) = −

sin ϕ

 

 

 

 

 

,

 

 

 

 

 

.

cos ϕ + cos ϕ0

 

cos ϕ + cos ϕ0

However, if both faces are illuminated (α π < ϕ0 < π ),

 

 

f (0), ϕ

)

 

 

 

sin ϕ0

 

 

 

sinϕ0)

 

 

 

= cos ϕ + cos ϕ0

+ cosϕ) + cosϕ0)

 

 

0

 

 

 

and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

g(0), ϕ

)

 

 

 

sin ϕ

 

 

 

sinϕ)

.

 

= − cos ϕ + cos ϕ0

cosϕ) + cosϕ0)

 

0

 

 

 

(3.55)

(3.56)

(3.57)

It is seen that these functions are singular at the boundaries of reflected plane waves, where ϕ = π ± ϕ0 or ϕ = 2α π ϕ0. The asymptotics of the PO diffracted field, which are uniformly valid around the wedge, can be easily derived by the application of the Pauli technique demonstrated in Sections 2.5 and 2.6. We do not consider them here, because our main purpose in the canonical wedge diffraction problem is the calculation of the field generated by the nonuniform component of the surface sources.

PROBLEMS

3.1 Analyze the accuracy of the PO approximation. Compute and plot the relative error

δf (0), ϕ0, α) = |F(ϕ, ϕ0, α) − 1| · 100%,

where

F(ϕ, ϕ0, α) = f (0), ϕ0)/f (ϕ, ϕ0, α).

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