From f02dfce6e6c34b3d8a7b8a0e784b506178e331fa Mon Sep 17 00:00:00 2001 From: "erdgeist@erdgeist.org" Date: Thu, 4 Jul 2019 23:26:09 +0200 Subject: stripdown of version 0.9 --- newamp1.c | 625 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ 1 file changed, 625 insertions(+) create mode 100644 newamp1.c (limited to 'newamp1.c') diff --git a/newamp1.c b/newamp1.c new file mode 100644 index 0000000..575620a --- /dev/null +++ b/newamp1.c @@ -0,0 +1,625 @@ +/*---------------------------------------------------------------------------*\ + + FILE........: newamp1.c + AUTHOR......: David Rowe + DATE CREATED: Jan 2017 + + Quantisation functions for the sinusoidal coder, using "newamp1" + algorithm that resamples variable rate L [Am} to a fixed rate K then + VQs. + +\*---------------------------------------------------------------------------*/ + +/* + Copyright David Rowe 2017 + + All rights reserved. + + This program is free software; you can redistribute it and/or modify + it under the terms of the GNU Lesser General Public License version 2.1, as + published by the Free Software Foundation. This program 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 Lesser General Public License + along with this program; if not, see . + +*/ + +#include +#include +#include +#include +#include + +#include "defines.h" +#include "phase.h" +#include "quantise.h" +#include "mbest.h" +#include "newamp1.h" + +#define NEWAMP1_VQ_MBEST_DEPTH 5 /* how many candidates we keep for each stage of mbest search */ + +/*---------------------------------------------------------------------------*\ + + FUNCTION....: interp_para() + AUTHOR......: David Rowe + DATE CREATED: Jan 2017 + + General 2nd order parabolic interpolator. Used splines orginally, + but this is much simpler and we don't need much accuracy. Given two + vectors of points xp and yp, find interpolated values y at points x. + +\*---------------------------------------------------------------------------*/ + +void interp_para(float y[], float xp[], float yp[], int np, float x[], int n) +{ + assert(np >= 3); + + int k,i; + float xi, x1, y1, x2, y2, x3, y3, a, b; + + k = 0; + for (i=0; iL; m++) { + AmdB[m] = 20.0*log10f(model->A[m]+1E-16); + if (AmdB[m] > AmdB_peak) { + AmdB_peak = AmdB[m]; + } + rate_L_sample_freqs_kHz[m] = m*model->Wo*(c2const->Fs/2000.0)/M_PI; + //printf("m: %d AmdB: %f AmdB_peak: %f sf: %f\n", m, AmdB[m], AmdB_peak, rate_L_sample_freqs_kHz[m]); + } + + /* clip between peak and peak -50dB, to reduce dynamic range */ + + for(m=1; m<=model->L; m++) { + if (AmdB[m] < (AmdB_peak-50.0)) { + AmdB[m] = AmdB_peak-50.0; + } + } + + interp_para(rate_K_vec, &rate_L_sample_freqs_kHz[1], &AmdB[1], model->L, rate_K_sample_freqs_kHz, K); +} + + +/*---------------------------------------------------------------------------*\ + + FUNCTION....: rate_K_mbest_encode + AUTHOR......: David Rowe + DATE CREATED: Jan 2017 + + Two stage rate K newamp1 VQ quantiser using mbest search. + +\*---------------------------------------------------------------------------*/ + +float rate_K_mbest_encode(int *indexes, float *x, float *xq, int ndim, int mbest_entries) +{ + int i, j, n1, n2; + const float *codebook1 = newamp1vq_cb[0].cb; + const float *codebook2 = newamp1vq_cb[1].cb; + struct MBEST *mbest_stage1, *mbest_stage2; + float target[ndim]; + float w[ndim]; + int index[MBEST_STAGES]; + float mse, tmp; + + /* codebook is compiled for a fixed K */ + + assert(ndim == newamp1vq_cb[0].k); + + /* equal weights, could be argued mel freq axis gives freq dep weighting */ + + for(i=0; ilist[j].index[0]; + for(i=0; ilist[0].index[1]; + n2 = mbest_stage2->list[0].index[0]; + mse = 0.0; + for (i=0;iL; m++) { + rate_L_sample_freqs_kHz[m] = m*model->Wo*(c2const->Fs/2000.0)/M_PI; + } + + interp_para(&AmdB[1], rate_K_sample_freqs_kHz_term, rate_K_vec_term, K+2, &rate_L_sample_freqs_kHz[1], model->L); + for(m=1; m<=model->L; m++) { + model->A[m] = POW10F(AmdB[m]/20.0); + // printf("m: %d f: %f AdB: %f A: %f\n", m, rate_L_sample_freqs_kHz[m], AmdB[m], model->A[m]); + } +} + + +/*---------------------------------------------------------------------------*\ + + FUNCTION....: determine_phase + AUTHOR......: David Rowe + DATE CREATED: Jan 2017 + + Given a magnitude spectrum determine a phase spectrum, used for + phase synthesis with newamp1. + +\*---------------------------------------------------------------------------*/ + +void determine_phase(C2CONST *c2const, COMP H[], MODEL *model, int Nfft, codec2_fft_cfg fwd_cfg, codec2_fft_cfg inv_cfg) +{ + int i,m,b; + int Ns = Nfft/2+1; + float Gdbfk[Ns], sample_freqs_kHz[Ns], phase[Ns]; + float AmdB[MAX_AMP+1], rate_L_sample_freqs_kHz[MAX_AMP+1]; + + for(m=1; m<=model->L; m++) { + assert(model->A[m] != 0.0); + AmdB[m] = 20.0*log10f(model->A[m]); + rate_L_sample_freqs_kHz[m] = (float)m*model->Wo*(c2const->Fs/2000.0)/M_PI; + } + + for(i=0; iFs/1000.0)*(float)i/Nfft; + } + + interp_para(Gdbfk, &rate_L_sample_freqs_kHz[1], &AmdB[1], model->L, sample_freqs_kHz, Ns); + mag_to_phase(phase, Gdbfk, Nfft, fwd_cfg, inv_cfg); + + for(m=1; m<=model->L; m++) { + b = floorf(0.5+m*model->Wo*Nfft/(2.0*M_PI)); + H[m].real = cosf(phase[b]); H[m].imag = sinf(phase[b]); + } +} + + +/*---------------------------------------------------------------------------*\ + + FUNCTION....: newamp1_model_to_indexes + AUTHOR......: David Rowe + DATE CREATED: Jan 2017 + + newamp1 encoder for amplitdues {Am}. Given the rate L model + parameters, outputs VQ and energy quantiser indexes. + +\*---------------------------------------------------------------------------*/ + +void newamp1_model_to_indexes(C2CONST *c2const, + int indexes[], + MODEL *model, + float rate_K_vec[], + float rate_K_sample_freqs_kHz[], + int K, + float *mean, + float rate_K_vec_no_mean[], + float rate_K_vec_no_mean_[], + float *se + ) +{ + int k; + + /* convert variable rate L to fixed rate K */ + + resample_const_rate_f(c2const, model, rate_K_vec, rate_K_sample_freqs_kHz, K); + + /* remove mean and two stage VQ */ + + float sum = 0.0; + for(k=0; kvoiced) { + int index = encode_log_Wo(c2const, model->Wo, 6); + if (index == 0) { + index = 1; + } + indexes[3] = index; + } + else { + indexes[3] = 0; + } + + } + + +/*---------------------------------------------------------------------------*\ + + FUNCTION....: newamp1_interpolate + AUTHOR......: David Rowe + DATE CREATED: Jan 2017 + +\*---------------------------------------------------------------------------*/ + +void newamp1_interpolate(float interpolated_surface_[], float left_vec[], float right_vec[], int K) +{ + int i, k; + int M = 4; + float c; + + /* (linearly) interpolate 25Hz amplitude vectors back to 100Hz */ + + for(i=0,c=1.0; i