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| 1 /* Copyright (c) 2007-2008 CSIRO |
| 2 Copyright (c) 2007-2009 Xiph.Org Foundation |
| 3 Written by Jean-Marc Valin */ |
| 4 /* |
| 5 Redistribution and use in source and binary forms, with or without |
| 6 modification, are permitted provided that the following conditions |
| 7 are met: |
| 8 |
| 9 - Redistributions of source code must retain the above copyright |
| 10 notice, this list of conditions and the following disclaimer. |
| 11 |
| 12 - Redistributions in binary form must reproduce the above copyright |
| 13 notice, this list of conditions and the following disclaimer in the |
| 14 documentation and/or other materials provided with the distribution. |
| 15 |
| 16 THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS |
| 17 ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT |
| 18 LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR |
| 19 A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT OWNER |
| 20 OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, |
| 21 EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, |
| 22 PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR |
| 23 PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF |
| 24 LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING |
| 25 NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS |
| 26 SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. |
| 27 */ |
| 28 |
| 29 #ifdef HAVE_CONFIG_H |
| 30 #include "config.h" |
| 31 #endif |
| 32 |
| 33 #include "mathops.h" |
| 34 #include "cwrs.h" |
| 35 #include "vq.h" |
| 36 #include "arch.h" |
| 37 #include "os_support.h" |
| 38 #include "bands.h" |
| 39 #include "rate.h" |
| 40 |
| 41 static void exp_rotation1(celt_norm *X, int len, int stride, opus_val16 c, opus_
val16 s) |
| 42 { |
| 43 int i; |
| 44 celt_norm *Xptr; |
| 45 Xptr = X; |
| 46 for (i=0;i<len-stride;i++) |
| 47 { |
| 48 celt_norm x1, x2; |
| 49 x1 = Xptr[0]; |
| 50 x2 = Xptr[stride]; |
| 51 Xptr[stride] = EXTRACT16(SHR32(MULT16_16(c,x2) + MULT16_16(s,x1), 15)); |
| 52 *Xptr++ = EXTRACT16(SHR32(MULT16_16(c,x1) - MULT16_16(s,x2), 15)); |
| 53 } |
| 54 Xptr = &X[len-2*stride-1]; |
| 55 for (i=len-2*stride-1;i>=0;i--) |
| 56 { |
| 57 celt_norm x1, x2; |
| 58 x1 = Xptr[0]; |
| 59 x2 = Xptr[stride]; |
| 60 Xptr[stride] = EXTRACT16(SHR32(MULT16_16(c,x2) + MULT16_16(s,x1), 15)); |
| 61 *Xptr-- = EXTRACT16(SHR32(MULT16_16(c,x1) - MULT16_16(s,x2), 15)); |
| 62 } |
| 63 } |
| 64 |
| 65 static void exp_rotation(celt_norm *X, int len, int dir, int stride, int K, int
spread) |
| 66 { |
| 67 static const int SPREAD_FACTOR[3]={15,10,5}; |
| 68 int i; |
| 69 opus_val16 c, s; |
| 70 opus_val16 gain, theta; |
| 71 int stride2=0; |
| 72 int factor; |
| 73 |
| 74 if (2*K>=len || spread==SPREAD_NONE) |
| 75 return; |
| 76 factor = SPREAD_FACTOR[spread-1]; |
| 77 |
| 78 gain = celt_div((opus_val32)MULT16_16(Q15_ONE,len),(opus_val32)(len+factor*K)
); |
| 79 theta = HALF16(MULT16_16_Q15(gain,gain)); |
| 80 |
| 81 c = celt_cos_norm(EXTEND32(theta)); |
| 82 s = celt_cos_norm(EXTEND32(SUB16(Q15ONE,theta))); /* sin(theta) */ |
| 83 |
| 84 if (len>=8*stride) |
| 85 { |
| 86 stride2 = 1; |
| 87 /* This is just a simple (equivalent) way of computing sqrt(len/stride) wi
th rounding. |
| 88 It's basically incrementing long as (stride2+0.5)^2 < len/stride. */ |
| 89 while ((stride2*stride2+stride2)*stride + (stride>>2) < len) |
| 90 stride2++; |
| 91 } |
| 92 /*NOTE: As a minor optimization, we could be passing around log2(B), not B, f
or both this and for |
| 93 extract_collapse_mask().*/ |
| 94 len /= stride; |
| 95 for (i=0;i<stride;i++) |
| 96 { |
| 97 if (dir < 0) |
| 98 { |
| 99 if (stride2) |
| 100 exp_rotation1(X+i*len, len, stride2, s, c); |
| 101 exp_rotation1(X+i*len, len, 1, c, s); |
| 102 } else { |
| 103 exp_rotation1(X+i*len, len, 1, c, -s); |
| 104 if (stride2) |
| 105 exp_rotation1(X+i*len, len, stride2, s, -c); |
| 106 } |
| 107 } |
| 108 } |
| 109 |
| 110 /** Takes the pitch vector and the decoded residual vector, computes the gain |
| 111 that will give ||p+g*y||=1 and mixes the residual with the pitch. */ |
| 112 static void normalise_residual(int * OPUS_RESTRICT iy, celt_norm * OPUS_RESTRICT
X, |
| 113 int N, opus_val32 Ryy, opus_val16 gain) |
| 114 { |
| 115 int i; |
| 116 #ifdef FIXED_POINT |
| 117 int k; |
| 118 #endif |
| 119 opus_val32 t; |
| 120 opus_val16 g; |
| 121 |
| 122 #ifdef FIXED_POINT |
| 123 k = celt_ilog2(Ryy)>>1; |
| 124 #endif |
| 125 t = VSHR32(Ryy, 2*(k-7)); |
| 126 g = MULT16_16_P15(celt_rsqrt_norm(t),gain); |
| 127 |
| 128 i=0; |
| 129 do |
| 130 X[i] = EXTRACT16(PSHR32(MULT16_16(g, iy[i]), k+1)); |
| 131 while (++i < N); |
| 132 } |
| 133 |
| 134 static unsigned extract_collapse_mask(int *iy, int N, int B) |
| 135 { |
| 136 unsigned collapse_mask; |
| 137 int N0; |
| 138 int i; |
| 139 if (B<=1) |
| 140 return 1; |
| 141 /*NOTE: As a minor optimization, we could be passing around log2(B), not B, f
or both this and for |
| 142 exp_rotation().*/ |
| 143 N0 = N/B; |
| 144 collapse_mask = 0; |
| 145 i=0; do { |
| 146 int j; |
| 147 j=0; do { |
| 148 collapse_mask |= (iy[i*N0+j]!=0)<<i; |
| 149 } while (++j<N0); |
| 150 } while (++i<B); |
| 151 return collapse_mask; |
| 152 } |
| 153 |
| 154 unsigned alg_quant(celt_norm *X, int N, int K, int spread, int B, ec_enc *enc |
| 155 #ifdef RESYNTH |
| 156 , opus_val16 gain |
| 157 #endif |
| 158 ) |
| 159 { |
| 160 VARDECL(celt_norm, y); |
| 161 VARDECL(int, iy); |
| 162 VARDECL(opus_val16, signx); |
| 163 int i, j; |
| 164 opus_val16 s; |
| 165 int pulsesLeft; |
| 166 opus_val32 sum; |
| 167 opus_val32 xy; |
| 168 opus_val16 yy; |
| 169 unsigned collapse_mask; |
| 170 SAVE_STACK; |
| 171 |
| 172 celt_assert2(K>0, "alg_quant() needs at least one pulse"); |
| 173 celt_assert2(N>1, "alg_quant() needs at least two dimensions"); |
| 174 |
| 175 ALLOC(y, N, celt_norm); |
| 176 ALLOC(iy, N, int); |
| 177 ALLOC(signx, N, opus_val16); |
| 178 |
| 179 exp_rotation(X, N, 1, B, K, spread); |
| 180 |
| 181 /* Get rid of the sign */ |
| 182 sum = 0; |
| 183 j=0; do { |
| 184 if (X[j]>0) |
| 185 signx[j]=1; |
| 186 else { |
| 187 signx[j]=-1; |
| 188 X[j]=-X[j]; |
| 189 } |
| 190 iy[j] = 0; |
| 191 y[j] = 0; |
| 192 } while (++j<N); |
| 193 |
| 194 xy = yy = 0; |
| 195 |
| 196 pulsesLeft = K; |
| 197 |
| 198 /* Do a pre-search by projecting on the pyramid */ |
| 199 if (K > (N>>1)) |
| 200 { |
| 201 opus_val16 rcp; |
| 202 j=0; do { |
| 203 sum += X[j]; |
| 204 } while (++j<N); |
| 205 |
| 206 /* If X is too small, just replace it with a pulse at 0 */ |
| 207 #ifdef FIXED_POINT |
| 208 if (sum <= K) |
| 209 #else |
| 210 /* Prevents infinities and NaNs from causing too many pulses |
| 211 to be allocated. 64 is an approximation of infinity here. */ |
| 212 if (!(sum > EPSILON && sum < 64)) |
| 213 #endif |
| 214 { |
| 215 X[0] = QCONST16(1.f,14); |
| 216 j=1; do |
| 217 X[j]=0; |
| 218 while (++j<N); |
| 219 sum = QCONST16(1.f,14); |
| 220 } |
| 221 rcp = EXTRACT16(MULT16_32_Q16(K-1, celt_rcp(sum))); |
| 222 j=0; do { |
| 223 #ifdef FIXED_POINT |
| 224 /* It's really important to round *towards zero* here */ |
| 225 iy[j] = MULT16_16_Q15(X[j],rcp); |
| 226 #else |
| 227 iy[j] = (int)floor(rcp*X[j]); |
| 228 #endif |
| 229 y[j] = (celt_norm)iy[j]; |
| 230 yy = MAC16_16(yy, y[j],y[j]); |
| 231 xy = MAC16_16(xy, X[j],y[j]); |
| 232 y[j] *= 2; |
| 233 pulsesLeft -= iy[j]; |
| 234 } while (++j<N); |
| 235 } |
| 236 celt_assert2(pulsesLeft>=1, "Allocated too many pulses in the quick pass"); |
| 237 |
| 238 /* This should never happen, but just in case it does (e.g. on silence) |
| 239 we fill the first bin with pulses. */ |
| 240 #ifdef FIXED_POINT_DEBUG |
| 241 celt_assert2(pulsesLeft<=N+3, "Not enough pulses in the quick pass"); |
| 242 #endif |
| 243 if (pulsesLeft > N+3) |
| 244 { |
| 245 opus_val16 tmp = (opus_val16)pulsesLeft; |
| 246 yy = MAC16_16(yy, tmp, tmp); |
| 247 yy = MAC16_16(yy, tmp, y[0]); |
| 248 iy[0] += pulsesLeft; |
| 249 pulsesLeft=0; |
| 250 } |
| 251 |
| 252 s = 1; |
| 253 for (i=0;i<pulsesLeft;i++) |
| 254 { |
| 255 int best_id; |
| 256 opus_val32 best_num = -VERY_LARGE16; |
| 257 opus_val16 best_den = 0; |
| 258 #ifdef FIXED_POINT |
| 259 int rshift; |
| 260 #endif |
| 261 #ifdef FIXED_POINT |
| 262 rshift = 1+celt_ilog2(K-pulsesLeft+i+1); |
| 263 #endif |
| 264 best_id = 0; |
| 265 /* The squared magnitude term gets added anyway, so we might as well |
| 266 add it outside the loop */ |
| 267 yy = ADD32(yy, 1); |
| 268 j=0; |
| 269 do { |
| 270 opus_val16 Rxy, Ryy; |
| 271 /* Temporary sums of the new pulse(s) */ |
| 272 Rxy = EXTRACT16(SHR32(ADD32(xy, EXTEND32(X[j])),rshift)); |
| 273 /* We're multiplying y[j] by two so we don't have to do it here */ |
| 274 Ryy = ADD16(yy, y[j]); |
| 275 |
| 276 /* Approximate score: we maximise Rxy/sqrt(Ryy) (we're guaranteed that |
| 277 Rxy is positive because the sign is pre-computed) */ |
| 278 Rxy = MULT16_16_Q15(Rxy,Rxy); |
| 279 /* The idea is to check for num/den >= best_num/best_den, but that way |
| 280 we can do it without any division */ |
| 281 /* OPT: Make sure to use conditional moves here */ |
| 282 if (MULT16_16(best_den, Rxy) > MULT16_16(Ryy, best_num)) |
| 283 { |
| 284 best_den = Ryy; |
| 285 best_num = Rxy; |
| 286 best_id = j; |
| 287 } |
| 288 } while (++j<N); |
| 289 |
| 290 /* Updating the sums of the new pulse(s) */ |
| 291 xy = ADD32(xy, EXTEND32(X[best_id])); |
| 292 /* We're multiplying y[j] by two so we don't have to do it here */ |
| 293 yy = ADD16(yy, y[best_id]); |
| 294 |
| 295 /* Only now that we've made the final choice, update y/iy */ |
| 296 /* Multiplying y[j] by 2 so we don't have to do it everywhere else */ |
| 297 y[best_id] += 2*s; |
| 298 iy[best_id]++; |
| 299 } |
| 300 |
| 301 /* Put the original sign back */ |
| 302 j=0; |
| 303 do { |
| 304 X[j] = MULT16_16(signx[j],X[j]); |
| 305 if (signx[j] < 0) |
| 306 iy[j] = -iy[j]; |
| 307 } while (++j<N); |
| 308 encode_pulses(iy, N, K, enc); |
| 309 |
| 310 #ifdef RESYNTH |
| 311 normalise_residual(iy, X, N, yy, gain); |
| 312 exp_rotation(X, N, -1, B, K, spread); |
| 313 #endif |
| 314 |
| 315 collapse_mask = extract_collapse_mask(iy, N, B); |
| 316 RESTORE_STACK; |
| 317 return collapse_mask; |
| 318 } |
| 319 |
| 320 /** Decode pulse vector and combine the result with the pitch vector to produce |
| 321 the final normalised signal in the current band. */ |
| 322 unsigned alg_unquant(celt_norm *X, int N, int K, int spread, int B, |
| 323 ec_dec *dec, opus_val16 gain) |
| 324 { |
| 325 int i; |
| 326 opus_val32 Ryy; |
| 327 unsigned collapse_mask; |
| 328 VARDECL(int, iy); |
| 329 SAVE_STACK; |
| 330 |
| 331 celt_assert2(K>0, "alg_unquant() needs at least one pulse"); |
| 332 celt_assert2(N>1, "alg_unquant() needs at least two dimensions"); |
| 333 ALLOC(iy, N, int); |
| 334 decode_pulses(iy, N, K, dec); |
| 335 Ryy = 0; |
| 336 i=0; |
| 337 do { |
| 338 Ryy = MAC16_16(Ryy, iy[i], iy[i]); |
| 339 } while (++i < N); |
| 340 normalise_residual(iy, X, N, Ryy, gain); |
| 341 exp_rotation(X, N, -1, B, K, spread); |
| 342 collapse_mask = extract_collapse_mask(iy, N, B); |
| 343 RESTORE_STACK; |
| 344 return collapse_mask; |
| 345 } |
| 346 |
| 347 void renormalise_vector(celt_norm *X, int N, opus_val16 gain) |
| 348 { |
| 349 int i; |
| 350 #ifdef FIXED_POINT |
| 351 int k; |
| 352 #endif |
| 353 opus_val32 E = EPSILON; |
| 354 opus_val16 g; |
| 355 opus_val32 t; |
| 356 celt_norm *xptr = X; |
| 357 for (i=0;i<N;i++) |
| 358 { |
| 359 E = MAC16_16(E, *xptr, *xptr); |
| 360 xptr++; |
| 361 } |
| 362 #ifdef FIXED_POINT |
| 363 k = celt_ilog2(E)>>1; |
| 364 #endif |
| 365 t = VSHR32(E, 2*(k-7)); |
| 366 g = MULT16_16_P15(celt_rsqrt_norm(t),gain); |
| 367 |
| 368 xptr = X; |
| 369 for (i=0;i<N;i++) |
| 370 { |
| 371 *xptr = EXTRACT16(PSHR32(MULT16_16(g, *xptr), k+1)); |
| 372 xptr++; |
| 373 } |
| 374 /*return celt_sqrt(E);*/ |
| 375 } |
| 376 |
| 377 int stereo_itheta(celt_norm *X, celt_norm *Y, int stereo, int N) |
| 378 { |
| 379 int i; |
| 380 int itheta; |
| 381 opus_val16 mid, side; |
| 382 opus_val32 Emid, Eside; |
| 383 |
| 384 Emid = Eside = EPSILON; |
| 385 if (stereo) |
| 386 { |
| 387 for (i=0;i<N;i++) |
| 388 { |
| 389 celt_norm m, s; |
| 390 m = ADD16(SHR16(X[i],1),SHR16(Y[i],1)); |
| 391 s = SUB16(SHR16(X[i],1),SHR16(Y[i],1)); |
| 392 Emid = MAC16_16(Emid, m, m); |
| 393 Eside = MAC16_16(Eside, s, s); |
| 394 } |
| 395 } else { |
| 396 for (i=0;i<N;i++) |
| 397 { |
| 398 celt_norm m, s; |
| 399 m = X[i]; |
| 400 s = Y[i]; |
| 401 Emid = MAC16_16(Emid, m, m); |
| 402 Eside = MAC16_16(Eside, s, s); |
| 403 } |
| 404 } |
| 405 mid = celt_sqrt(Emid); |
| 406 side = celt_sqrt(Eside); |
| 407 #ifdef FIXED_POINT |
| 408 /* 0.63662 = 2/pi */ |
| 409 itheta = MULT16_16_Q15(QCONST16(0.63662f,15),celt_atan2p(side, mid)); |
| 410 #else |
| 411 itheta = (int)floor(.5f+16384*0.63662f*atan2(side,mid)); |
| 412 #endif |
| 413 |
| 414 return itheta; |
| 415 } |
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