%{ Copyright © 2020 Alexey A. Shcherbakov. All rights reserved. This file is part of GratingFMM. GratingFMM is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 2 of the License, or (at your option) any later version. GratingFMM is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with GratingFMM. If not, see . %} %% description: % calculate a matrix of diffraction efficiencies in case of the % diffraction by 2D gratings being periodic in x and y dimensions %% input: % xno, yno: numbers of Fourier harmonics in x and y dimensions % V_inc: incident field amplitude matrix of size (2*no,2) % V_dif: diffracted field amplitude matrix of size (2*no,2) % kx0, ky0: incident plane wave wavevector x and y projections (Bloch wavevector projections) % kgx, kgy: wavelength-to-period ratios (grating vectors) % eps1, eps2: substrate and superstrate permittivities %% output: % V_eff: efficiency matrix of size (2*no,2) if the if the incident field has % propagating harmonics, otherwise (if the incident field is purely evanescent) % the matrix of partial powers carried by each diffraction order % first index of V_inc, V_dif, V_eff indicates diffraction harmonics % with indices 1:no being TE orders and no+1:2*no being TM orders % (0-th order index is ind_0 = (ceil(xno/2)-1)*yno+ceil(yno/2)) % second index of V_inc, V_dif, V_eff indicates whether the diffraction orders % are in the substrate (V(:,1)) or in the superstrate (V(:,2)) %% implementation function [V_eff] = fmmtd_efficiency(xno, yno, V_inc, V_dif, kx0, ky0, kgx, kgy, eps1, eps2) no = xno*yno; ib1 = 1:no; ib2 = no+1:2*no; [kz1, kz2] = fmmtd_kxyz(xno, yno, kx0, ky0, kgx, kgy, eps1, eps2); kz1 = transpose(kz1); kz2 = transpose(kz2); P_inc = sum( abs(V_inc(ib1,1).^2).*real(kz1) + abs(V_inc(ib1,2).^2).*real(kz2) ) ... + sum( abs(V_inc(ib2,1).^2).*real(kz1/eps1) + abs(V_inc(ib2,2).^2).*real(kz2/eps2) ); V_eff = zeros(2*no,2); V_eff(ib1,1) = abs(V_dif(ib1,1).^2).*real(kz1); V_eff(ib1,2) = abs(V_dif(ib1,2).^2).*real(kz2); V_eff(ib2,1) = abs(V_dif(ib2,1).^2).*real(kz1/eps1); V_eff(ib2,2) = abs(V_dif(ib2,2).^2).*real(kz2/eps2); if abs(P_inc) > 1e-15 V_eff = (1/P_inc)*V_eff; else V_eff = 0.5*V_eff; end end % % END %