Add new functions
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123
Functions/Metrics/calc_ngmi.m
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123
Functions/Metrics/calc_ngmi.m
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function [GMI,NGMI] = calc_ngmi(test_signal,reference_signal,options)
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% Silas implementation of (N)GMI calculation according to: J. Cho, L. Schmalen, und P. J. Winzer,
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% „Normalized Generalized Mutual Information as a Forward Error Correction Threshold for Probabilistically Shaped QAM“,
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% in 2017 European Conference on Optical Communication (ECOC), Sep. 2017, doi: 10.1109/ECOC.2017.8345872.
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% This implementation assumes the same normal distributed noise for each
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% channel (sigma2 is calculated once for the whole signal)
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arguments(Input)
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test_signal;
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reference_signal;
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options.skip_front = 0;
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options.skip_end = 0;
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options.returnErrorLocation = 0;
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end
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options.skip_end = abs(options.skip_end);
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options.skip_front = abs(options.skip_front);
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assert((options.skip_end+options.skip_front)<length(test_signal),"You can not skip more bits than overall length of data! Set skip_front or skip_end to lower value or check data_in");
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if isa(reference_signal,'Signal')
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reference_signal = reference_signal.signal;
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end
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if isa(test_signal,'Signal')
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test_signal = test_signal.signal;
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end
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% TRIM
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[test_signal,reference_signal]=trimseq(test_signal,reference_signal,options.skip_front,options.skip_end);
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% CALC EVM
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[GMI,NGMI] = calc_ngmi_(test_signal,reference_signal);
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function [GMI,NGMI] = calc_ngmi_(test_signal,reference_signal)
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assert(length(test_signal) == length(reference_signal),"Sequence length does not match");
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%%% implemented according to [1] J. Cho, L. Schmalen, und P. J. Winzer,
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% „Normalized Generalized Mutual Information as a Forward Error Correction Threshold for Probabilistically Shaped QAM“,
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% in 2017 European Conference on Optical Communication (ECOC), Sep. 2017, S. 1–3. doi: 10.1109/ECOC.2017.8345872.
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error_vector = (test_signal-reference_signal);
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sigma2 = var(error_vector); %noise variance
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%%% Separate Classes
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constellation = unique(reference_signal);
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received_sd = NaN(numel(constellation),length(reference_signal));
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lvlcol = cbrewer2('Set1',numel(constellation));
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for lvl = 1:numel(constellation)
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%Separate the equalized signal into the
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%respective levels based on the actually
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%transmitted level!
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received_sd(lvl,reference_signal==constellation(lvl)) = test_signal(reference_signal==constellation(lvl));
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end
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N = length(test_signal); % Number of received samples
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M = length(constellation); %P
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m = log2(M); %bits per symbol
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entries = sum(~isnan(received_sd),2)';
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P_X = entries./N;
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% Parameters
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symbols = constellation'; % PAM-4 symbols
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gray_bits = PAMmapper(M,0).demap_(constellation); % Gray coding (bits per symbol)
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% Conditional probability function for AWGN
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q_Y_given_X = @(y, x) (1 / sqrt(2 * pi * sigma2)) * exp(-(y - x).^2 / (2 * sigma2));
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% Entropy term
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H_X = -sum(P_X .* log2(P_X)); % Entropy of input distribution
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% GMI computation
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noise_impact_term = 0;
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for k = 1:N
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y_k = test_signal(k); % Current received sample
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[~, closest_symbol_idx] = min(abs(symbols - y_k)); % Closest symbol index
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closest_symbol = symbols(closest_symbol_idx); % Closest symbol
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for i = 1:m
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% Extract i-th bit for each symbol
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bit_mask = gray_bits(:, i); % Binary column for i-th bit of all symbols
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matching_symbols = symbols(bit_mask == gray_bits(closest_symbol_idx, i));
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% Numerator: Sum over x in x_{b_{k, i}}
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numerator = sum(q_Y_given_X(y_k, matching_symbols) .* P_X(ismember(symbols, matching_symbols)));
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% Denominator: Sum over all x
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denominator = sum(q_Y_given_X(y_k, symbols) .* P_X);
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% Logarithmic contribution
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noise_impact_term = noise_impact_term + log2(numerator / denominator);
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end
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end
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% Normalize the noise impact term by N
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noise_impact_term = noise_impact_term / N;
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% GMI
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GMI = H_X + noise_impact_term;
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NGMI = GMI / m;
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end
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function [data_,reference_]=trimseq(data,reference,skipstart,skip_end)
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data_ = data(skipstart+1:end-skip_end,:);
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delta_bits = length(reference) - length(data);
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skip_end = delta_bits + skip_end;
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reference_ = reference(skipstart+1:end-skip_end,:);
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end
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end
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