Asymptotic forms of the solution of the inverse problem for the helmholtz equation

1988 ◽  
Vol 28 (6) ◽  
pp. 152-158 ◽  
Author(s):  
A.S. Barashkov
2011 ◽  
Vol 19 (6) ◽  
pp. 839-854 ◽  
Author(s):  
M. Tadi ◽  
A.K. Nandakumaran ◽  
S.S. Sritharan

2003 ◽  
Vol 184 (1) ◽  
pp. 122-148 ◽  
Author(s):  
Yuriy A. Gryazin ◽  
Michael V. Klibanov ◽  
Thomas R. Lucas

2013 ◽  
Vol 2013 ◽  
pp. 1-15 ◽  
Author(s):  
Edwin A. Marengo

The inverse problem of estimating the smallest region of localization (minimum source region) of a source or scatterer that can produce a given radiation or scattered field is investigated with the help of the multipole expansion. The results are derived in the framework of the scalar Helmholtz equation. The proposed approach allows the estimation of possibly nonconvex minimum source regions. The derived method is illustrated with an example relevant to inverse scattering.


1985 ◽  
Vol 1 (4) ◽  
pp. 357-370 ◽  
Author(s):  
R Magnanini ◽  
G Papi

1993 ◽  
Vol 66 (4) ◽  
pp. 2363-2368
Author(s):  
A. G. Nakonechnyi ◽  
Kh. M. Meredov

2020 ◽  
Vol 0 (0) ◽  
Author(s):  
T. S. Kalmenov ◽  
S. I. Kabanikhin ◽  
Aidana Les

AbstractThe study of a time-periodic solution of the multidimensional wave equation {\frac{\partial^{2}}{\partial t^{2}}\widetilde{u}-\Delta_{x}\widetilde{u}=% \widetilde{f}(x,t)}, {\widetilde{u}(x,t)=e^{ikt}u(x)}, over the whole space {\mathbb{R}^{3}} leads to the condition of the Sommerfeld radiation at infinity. This is a problem that describes the motion of scattering stationary waves from a source that is in a bounded area. The inverse problem of finding this source is equivalent to reducing the Sommerfeld problem to a boundary value problem for the Helmholtz equation in a finite domain. Therefore, the Sommerfeld problem is a special inverse problem. It should be noted that in the work of Bezmenov [I. V. Bezmenov, Transfer of Sommerfeld radiation conditions to an artificial boundary of the region based on the variational principle, Sb. Math. 185 1995, 3, 3–24] approximate forms of such boundary conditions were found. In [T. S. Kalmenov and D. Suragan, Transfer of Sommerfeld radiation conditions to the boundary of a limited area, J. Comput. Math. Math. Phys. 52 2012, 6, 1063–1068], for a complex parameter λ, an explicit form of these boundary conditions was found through the boundary condition of the Helmholtz potential given by the integral in the finite domain Ω:($*$)u(x,\lambda)=\int_{\Omega}\varepsilon(x-\xi,\lambda)\rho(\xi,\lambda)\,d\xi{}where {\varepsilon(x-\xi,\lambda)} are fundamental solutions of the Helmholtz equation,-\Delta_{x}\varepsilon(x)-\lambda\varepsilon=\delta(x),{\rho(\xi,\lambda)} is a density of the potential, λ is a complex number, and δ is the Dirac delta function. These boundary conditions have the property that stationary waves coming from the region Ω to {\partial\Omega} pass {\partial\Omega} without reflection, i.e. are transparent boundary conditions. In the present work, in the general case, in {\mathbb{R}^{n}}, {n\geq 3}, we have proved the problem of reducing the Sommerfeld problem to a boundary value problem in a finite domain. Under the necessary conditions for the Helmholtz potential (*), its density {\rho(\xi,\lambda)} has also been found.


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