/* ugens8.h: Copyright (C) 1991, 1998, 2000 Dan Ellis, Richard Karpen, Richard Dobson This file is part of Csound. The Csound Library is free software; you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation; either version 2.1 of the License, or (at your option) any later version. Csound 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 Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with Csound; if not, write to the Free Software Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA */ /* UGENS8.H */ #ifndef _UGENS8_H_ #define _UGENS8_H_ #define PVFRAMSIZE 8192 /* i.e. max FFT point size */ #define PVFFTSIZE (2*PVFRAMSIZE) /* 2x for real + imag */ #define PVDATASIZE (1+PVFRAMSIZE/2) /* Need 1/2 channels + mid */ #define PVWINLEN (4097) /* time window 1st half */ /* PVDATASIZE reflects the fact that for n point _real_ time data, the fourier * transform will only have n degrees of freedom, although it has 2n values * (n bins x {re,im} or {mag,phase}). This constraint is reflected by the top * n/2-1 bins (bins n/2+1 .. n-1) being complex conjugates of bins 1..n/2-1. * Bins 0 and n/2 do not have conjugate images, but they ARE always real, * so only contribute one degree of freedom each. So the number of degrees of * freedom in the complex FFT is {re,im}*(n/2 - 1) +2 = n , as expected. * Thus we only need to store and process these independent values. However, * for convenience, and because our analysis system records the phase of * bins 0 and n/2 as 0 or pi rather than making the magnitude negative, we * allow these 2 bins to have imaginary components too, so that FFT frames are * stored as Magnitude & phase for bins 0..n/2 = 2*(n/2 + 1) or n+2 values. * These are the n+2 channels interleaved in the PVOC analysis file, and * then stored and processed wherever you see PVDATA/FRDA (frame data) */ #define pvfrsiz(p) (p->frSiz) #define pvffsiz(p) (2* p->frSiz) #define pvdasiz(p) (1 + (p->frSiz)/2) /* as above, based on */ #define pvfdsiz(p) (2 + p->frSiz) /* ACTUAL frameSize in use */ typedef struct { OPDS h; MYFLT *rslt, *ktimpnt, *kfmod, *ifilno, *ispecwp, *imode; MYFLT *ifreqlim, *igatefun; int32 mems; int32 kcnt, baseFr, maxFr, frSiz, prFlg, opBpos; /* RWD 8:2001 for pvocex: need these too */ int32 frInc, chans; MYFLT frPktim, frPrtim, scale, asr, lastPex; MYFLT PvMaxAmp; float *frPtr, *pvcopy; FUNC *AmpGateFunc; AUXCH auxch; MYFLT *lastPhase; /* [PVDATASIZE] Keep track of cum. phase */ MYFLT *fftBuf; /* [PVFFTSIZE] FFT works on Real & Imag */ MYFLT *dsBuf; /* [PVFFTSIZE] Output of downsampling may be 2x */ MYFLT *outBuf; /* [PVFFTSIZE] Output buffer over win length */ MYFLT *window; /* [PVWINLEN] Store 1/2 window */ MYFLT *dsputil_env; AUXCH memenv; PVOC_GLOBALS *pp; } PVOC; #endif

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