作业帮 > 综合 > 作业

英语翻译% This code solves the NLS equation with the split-step

来源:学生作业帮 编辑:大师作文网作业帮 分类:综合作业 时间:2024/11/13 20:13:14
英语翻译
% This code solves the NLS equation with the split-step method
% idu/dz - sgn(beta2)/2 d^2u/d(tau)^2 + N^2*|u|^2*u = 0
% Specify input parameters
clear all;
distance=10; % fiber length
beta2 = -1; % dispersion of fober
N = 1; % nonlinear parameter
mshape = 1; % pulse shape mshap=0 for sech,mshape>0 for super-Gausssian
chirp0 = 0; % input pulse chirp (default value)
%%%%%%%%%%% set simulation parameters
nt = 1024; Tmax = 32; % FFT points and window size
step_num = round(20*distance*N^2); % No.of z steps to
deltaz = distance/step_num; % step size in z
dtau = (2*Tmax)/nt; % step size in tau
%%%%%%%%% tau and omega arrays
tau = (-nt/2:nt/2-1)*dtau; % temporal grid
omega = (pi/Tmax)*[(0:nt/2-1) (-nt/2:-1)]; % frequency grid
%%%%%%%%% Input Field profile
if mshape==0
uu = sech(tau).*exp(-0.5i*chirp0*tau.^2); % soliton
else % super-Gaussian
uu = exp(-0.5*(1+i*chirp0).*tau.^(2*mshape));
end
%%%%%%%%% Plot input pulse shape and spectrum
temp = fftshift(ifft(uu)).*(nt*dtau)/sqrt(2*pi); % spectrum
figure(1);
subplot(2,1,1);
plot(tau,abs(uu).^2,'r','linewidth',2); hold on;
axis([-5 5 0 inf]);
xlabel('Normalized Time');
ylabel('Normalized Power');
subplot(2,1,2);
plot(fftshift(omega)/(2*pi),abs(temp).^2,'b','linewidth',2);
hold on;
axis([-.5 .5 0 inf]);
xlabel('Normalized Frequency');
ylabel('Spectral Power');
%%%%%%%%% store dispersive phase shifts to speedup code
dispersion = exp(i*0.5*beta2*omega.^2*deltaz); % phase factor
hhz = i*N^2*deltaz; % nonlinear phase factor
%%%%%%%% [ Beginning of MAIN Loop] %%%%%%%%%%%
%%%%%%%% scheme:1/2N -> D -> 1/2N; first half step nonlinear
temp = uu.*exp(abs(uu).^2.*hhz/2); % note hhz/2
for n=1:step_num
f_temp = ifft(temp).*dispersion;
uu = fft(f_temp);
temp = uu.*exp(abs(uu).^2.*hhz);
end
uu = temp.*exp(-abs(uu).^2.*hhz/2); % Final field
temp = fftshift(ifft(uu)).*(nt*dtau)/sqrt(2*pi); %Final spectrum
%%%%%%%% [ End of MAIN Loop ] %%%%%%%%%%%%%
%%%%%%%% Plot output pulse shape and spectrum
figure(2);
subplot(2,1,1);
plot(tau,abs(uu).^2 ,'c','linewidth',2);
hold on;
axis([-5 5 0 inf]);
xlabel('Normalized Time');
ylabel('Normalized Power');
subplot(2,1,2);
plot(fftshift(omega)/(2*pi),abs(temp).^2,'k','linewidth',2);
hold on;
axis([-.5 .5 0 inf]);
xlabel('Normalized Frequency');
ylabel('Spectral Power');
英语翻译% This code solves the NLS equation with the split-step
我是光学工程硕士研究生,希望我能给你帮助.
学习光信息,要学好高等数学、概率论与数理统计、线性代数、复变函数,这是数学基础,包括积分微分统计等等.
光学基础包括电动力学,数学物理方法,量子力学,这是光学的基础.包括麦克斯韦方程,这是基础.
光学专业知识包括:光学、信息光学、导波光学、红外光学、激光原理、光电子.
另外光电不分家的,电学也要学习,包括电路基础、模拟电路、数字电路等.
软件方面有MATLAB、zmax、beamprop等.
还有什么问题可以直接问我.
加油↖(^ω^)↗