Mercurial > hg > sv-dependency-builds
comparison src/fftw-3.3.3/mpi/choose-radix.c @ 10:37bf6b4a2645
Add FFTW3
author | Chris Cannam |
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date | Wed, 20 Mar 2013 15:35:50 +0000 |
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1 /* | |
2 * Copyright (c) 2003, 2007-11 Matteo Frigo | |
3 * Copyright (c) 2003, 2007-11 Massachusetts Institute of Technology | |
4 * | |
5 * This program is free software; you can redistribute it and/or modify | |
6 * it under the terms of the GNU General Public License as published by | |
7 * the Free Software Foundation; either version 2 of the License, or | |
8 * (at your option) any later version. | |
9 * | |
10 * This program is distributed in the hope that it will be useful, | |
11 * but WITHOUT ANY WARRANTY; without even the implied warranty of | |
12 * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the | |
13 * GNU General Public License for more details. | |
14 * | |
15 * You should have received a copy of the GNU General Public License | |
16 * along with this program; if not, write to the Free Software | |
17 * Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA | |
18 * | |
19 */ | |
20 | |
21 #include "ifftw-mpi.h" | |
22 | |
23 /* Return the radix r for a 1d MPI transform of a distributed dimension d, | |
24 with the given flags and transform size. That is, decomposes d.n | |
25 as r * m, Cooley-Tukey style. Also computes the block sizes rblock | |
26 and mblock. Returns 0 if such a decomposition is not feasible. | |
27 This is unfortunately somewhat complicated. | |
28 | |
29 A distributed Cooley-Tukey algorithm works as follows (see dft-rank1.c): | |
30 | |
31 d.n is initially distributed as an m x r array with block size mblock[IB]. | |
32 Then it is internally transposed to an r x m array with block size | |
33 rblock[IB]. Then it is internally transposed to m x r again with block | |
34 size mblock[OB]. Finally, it is transposed to r x m with block size | |
35 rblock[IB]. | |
36 | |
37 If flags & SCRAMBLED_IN, then the first transpose is skipped (the array | |
38 starts out as r x m). If flags & SCRAMBLED_OUT, then the last transpose | |
39 is skipped (the array ends up as m x r). To make sure the forward | |
40 and backward transforms use the same "scrambling" format, we swap r | |
41 and m when sign != FFT_SIGN. | |
42 | |
43 There are some downsides to this, especially in the case where | |
44 either m or r is not divisible by n_pes. For one thing, it means | |
45 that in general we can't use the same block size for the input and | |
46 output. For another thing, it means that we can't in general honor | |
47 a user's "requested" block sizes in d.b[]. Therefore, for simplicity, | |
48 we simply ignore d.b[] for now. | |
49 */ | |
50 INT XM(choose_radix)(ddim d, int n_pes, unsigned flags, int sign, | |
51 INT rblock[2], INT mblock[2]) | |
52 { | |
53 INT r, m; | |
54 | |
55 UNUSED(flags); /* we would need this if we paid attention to d.b[*] */ | |
56 | |
57 /* If n_pes is a factor of d.n, then choose r to be d.n / n_pes. | |
58 This not only ensures that the input (the m dimension) is | |
59 equally distributed if possible, and at the r dimension is | |
60 maximally equally distributed (if d.n/n_pes >= n_pes), it also | |
61 makes one of the local transpositions in the algorithm | |
62 trivial. */ | |
63 if (d.n % n_pes == 0 /* it's good if n_pes divides d.n ...*/ | |
64 && d.n / n_pes >= n_pes /* .. unless we can't use n_pes processes */) | |
65 r = d.n / n_pes; | |
66 else { /* n_pes does not divide d.n, pick a factor close to sqrt(d.n) */ | |
67 for (r = X(isqrt)(d.n); d.n % r != 0; ++r) | |
68 ; | |
69 } | |
70 if (r == 1 || r == d.n) return 0; /* punt if we can't reduce size */ | |
71 | |
72 if (sign != FFT_SIGN) { /* swap {m,r} so that scrambling is reversible */ | |
73 m = r; | |
74 r = d.n / m; | |
75 } | |
76 else | |
77 m = d.n / r; | |
78 | |
79 rblock[IB] = rblock[OB] = XM(default_block)(r, n_pes); | |
80 mblock[IB] = mblock[OB] = XM(default_block)(m, n_pes); | |
81 | |
82 return r; | |
83 } |