📄 berest.m
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%qpsk_berest.m
% File: psk_berest.m
function [peideal,pesystem]=psk_berest(xx,yy,ebn0db,eb,tb,nbw)
% ebn0db is an array of Eb/No values in db (specified at the receiver
%input); tb is the bit duration and nbw is the noise BW
% xx is the reference (ideal) input; yy is the filtered output;
nx=length(xx);
% For comparision purposes , set the noise BW of the ideal receiver
% (integrate and dump) to be equal to rs/2.
nbwideal=1/(2*tb); % noise bandwidth
for m=1:length(ebn0db)
peideal(m)=0.0; pesystem(m)=0.0; %initialize
% find n0 and the variance of the noise.
ebn0(m)=10^(ebn0db(m)/10); % dB to linear
n0=eb/ebn0(m); % noise power
sigma=sqrt(n0*nbw*2); %variance
sigma1=sqrt(n0*nbwideal*2);%
% Multiply the input constellation/signal by a scale factor so that input
% constellation and the constellations/signal at the input to receive
% filter have the same ave power a=sqrt(2*eb/(2*tb)).
b=sqrt(2*eb/tb)/sqrt(sum(abs(xx).^2)/nx);
d1=b*abs(xx);
d3=abs(yy);
peideal(m)=sum(q(d1/sigma1));
pesystem(m)=sum(q(d3/sigma));
end
peideal=peideal/nx;
pesystem=pesystem/nx;
% End of function file.
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