TY - GEN
T1 - Method of Generalized Debye Sources in Problems of EM Scattering by Conducting Bodies
AU - Chernokozhin, Evgeny
AU - Boag, Amir
N1 - Publisher Copyright: © 2024 IEEE.
PY - 2024
Y1 - 2024
N2 - In 2010, Epstein and Greengard proposed an approach to solving time harmonic Maxwell's equations that is free both from spurious resonances and the low-frequency breakdown (C. L. Epstein and L. Greengard, "Debye sources and the numerical solution of the time harmonic Maxwell equations," Commun. Pure Appl. Math., vol. LXIII, pp. 0413–0463, 2010). Their approach generalizes the Debye potentials, which are traditionally used in spherically symmetric problems, to closed surfaces of arbitrary shape. The electromagnetic field is represented via two fictitious surface charges r and q (generalized Debye sources, scalars) and two fictitious surface currents j and m (vectors). The latter, in turn, are expressed via two other scalar functions, Ψ and Ψm. In the case of perfectly conducting scatterers, the problem reduces to a system of two Fredholm integral equations of the second kind, expressing the equality to zero of the normal component of the total magnetic field and of the surface divergence of the total tangential electric field on the scatterer's surface S, and two surface differential equations—Poisson's equations with the Laplace–Beltrami operator Δτ on S: ΔτΨ = ikr, ΔτΨm = -ikq, where k is the wavenumber.
AB - In 2010, Epstein and Greengard proposed an approach to solving time harmonic Maxwell's equations that is free both from spurious resonances and the low-frequency breakdown (C. L. Epstein and L. Greengard, "Debye sources and the numerical solution of the time harmonic Maxwell equations," Commun. Pure Appl. Math., vol. LXIII, pp. 0413–0463, 2010). Their approach generalizes the Debye potentials, which are traditionally used in spherically symmetric problems, to closed surfaces of arbitrary shape. The electromagnetic field is represented via two fictitious surface charges r and q (generalized Debye sources, scalars) and two fictitious surface currents j and m (vectors). The latter, in turn, are expressed via two other scalar functions, Ψ and Ψm. In the case of perfectly conducting scatterers, the problem reduces to a system of two Fredholm integral equations of the second kind, expressing the equality to zero of the normal component of the total magnetic field and of the surface divergence of the total tangential electric field on the scatterer's surface S, and two surface differential equations—Poisson's equations with the Laplace–Beltrami operator Δτ on S: ΔτΨ = ikr, ΔτΨm = -ikq, where k is the wavenumber.
UR - http://www.scopus.com/inward/record.url?scp=85203147073&partnerID=8YFLogxK
U2 - https://doi.org/10.23919/INC-USNC-URSI61303.2024.10632467
DO - https://doi.org/10.23919/INC-USNC-URSI61303.2024.10632467
M3 - منشور من مؤتمر
T3 - 2024 IEEE INC-USNC-URSI Radio Science Meeting (Joint with AP-S Symposium), INC-USNC-URSI 2024 - Proceedings
SP - 117
BT - 2024 IEEE INC-USNC-URSI Radio Science Meeting (Joint with AP-S Symposium), INC-USNC-URSI 2024 - Proceedings
PB - Institute of Electrical and Electronics Engineers Inc.
T2 - 2024 IEEE INC-USNC-URSI Radio Science Meeting (Joint with AP-S Symposium), INC-USNC-URSI 2024
Y2 - 14 July 2024 through 19 July 2024
ER -