Through-Wall Imaging With UWB Radar System - KEMT FEI TUKE
Through-Wall Imaging With UWB Radar System - KEMT FEI TUKE
Through-Wall Imaging With UWB Radar System - KEMT FEI TUKE
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2.5 <strong>Radar</strong> <strong>Imaging</strong> Methods Overview 21<br />
where ∇ 2 φ = � ∇. � ∇φ and ∂φ<br />
∂n = � ∇φ.�n. In the case when φ = φ1φ2, the φ ′ =<br />
φ2φ ′ 1 + φ1φ ′ 2 and (2.5.11) becomes:<br />
or<br />
�b<br />
a<br />
�b<br />
a<br />
[φ2φ ′ 1 + φ1φ ′ 2]dx = φ1φ2| b<br />
a<br />
φ2φ ′ 1dx = φ1φ2| b<br />
a −<br />
�b<br />
a<br />
(2.5.14)<br />
φ1φ ′ 2dx. (2.5.15)<br />
An analogous formula in higher dimensions arises by substituting A = φ2 � ∇φ1 into<br />
(2.5.12). Using the identity � ∇.a� ∇b = � ∇a. � ∇b + a∇2b leads to:<br />
� �<br />
�∇φ2. � ∇φ1 + φ2∇ 2 � �<br />
φ1 dvol =<br />
∂φ1<br />
φ2 dsurf.<br />
∂n<br />
(2.5.16)<br />
V<br />
Similar result can be obtained when A = φ1 � ∇2φ2: � �<br />
�∇φ1. � ∇φ2 + φ1∇ 2 � �<br />
φ2 dvol =<br />
V<br />
V<br />
Finally, subtracting (2.5.17) from (2.5.16) yields to:<br />
�<br />
�<br />
φ2∇ 2 φ1 − φ1∇ 2 �<br />
�<br />
φ2 dvol =<br />
�<br />
∂φ1<br />
φ2<br />
∂n<br />
∂V<br />
∂V<br />
∂V<br />
φ1<br />
− φ1<br />
∂φ2<br />
dsurf. (2.5.17)<br />
∂n<br />
�<br />
∂φ2<br />
dsurf. (2.5.18)<br />
∂n<br />
(2.5.18) is known as Green’s theorem that represents fundamental of the Kirchhoff<br />
migration theory. It is a multidimensional generalization of the integration by<br />
formula from elementary calculus and is valuable for its ability to solve certain<br />
partial differential equation. φ1 and φ2 in (2.5.18) may be chosen as desired to<br />
conveniently expressed solutions to a given problem. Typically, in the solution to<br />
a partial differential equation like the wave equation, one function is chosen to be<br />
the solution to the problem at hand and the other is chosen to be the solution to<br />
the more simple reference problem. The reference problem is usually selected to<br />
have a known analytic solution and this solution is called a Green’s function [96].<br />
In general, the scalar wavefield ψ is a solution to the Helmholtz scalar wave<br />
equation: � ∇ 2 + k 2 � ψ = 0 (2.5.19)<br />
where ∇ 2 is the Laplacian and k is the wavevector. When the wave travels through<br />
the medium from point x0 to the point x this Helmholtz scalar wave equation can<br />
be expressed with the aid of Green’s function G (x0, x) as:<br />
� ∇ 2 + k 2 � G (x0, x) = δ (x0 − x) (2.5.20)