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Diffstat (limited to 'newlib/libm/machine/spu/headers/cos_sin.h')
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diff --git a/newlib/libm/machine/spu/headers/cos_sin.h b/newlib/libm/machine/spu/headers/cos_sin.h
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+/* -------------------------------------------------------------- */
+/* (C)Copyright 2006,2007, */
+/* International Business Machines Corporation, */
+/* Sony Computer Entertainment, Incorporated, */
+/* Toshiba Corporation, */
+/* */
+/* All Rights Reserved. */
+/* */
+/* Redistribution and use in source and binary forms, with or */
+/* without modification, are permitted provided that the */
+/* following conditions are met: */
+/* */
+/* - Redistributions of source code must retain the above copyright*/
+/* notice, this list of conditions and the following disclaimer. */
+/* */
+/* - Redistributions in binary form must reproduce the above */
+/* copyright notice, this list of conditions and the following */
+/* disclaimer in the documentation and/or other materials */
+/* provided with the distribution. */
+/* */
+/* - Neither the name of IBM Corporation nor the names of its */
+/* contributors may be used to endorse or promote products */
+/* derived from this software without specific prior written */
+/* permission. */
+/* Redistributions of source code must retain the above copyright */
+/* notice, this list of conditions and the following disclaimer. */
+/* */
+/* Redistributions in binary form must reproduce the above */
+/* copyright notice, this list of conditions and the following */
+/* disclaimer in the documentation and/or other materials */
+/* provided with the distribution. */
+/* */
+/* Neither the name of IBM Corporation nor the names of its */
+/* contributors may be used to endorse or promote products */
+/* derived from this software without specific prior written */
+/* permission. */
+/* */
+/* THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND */
+/* CONTRIBUTORS "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, */
+/* INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF */
+/* MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE */
+/* DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT OWNER OR */
+/* CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, */
+/* SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT */
+/* NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; */
+/* LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) */
+/* HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN */
+/* CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR */
+/* OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, */
+/* EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */
+/* -------------------------------------------------------------- */
+/* PROLOG END TAG zYx */
+#ifdef __SPU__
+#ifndef _COS_SIN_H_
+#define _COS_SIN_H_ 1
+
+#define M_PI_OVER_4_HI_32 0x3fe921fb
+
+#define M_PI_OVER_4 0.78539816339744827900
+#define M_FOUR_OVER_PI 1.27323954478442180616
+
+#define M_PI_OVER_2 1.57079632679489655800
+#define M_PI_OVER_2_HI 1.57079632673412561417
+#define M_PI_OVER_2_LO 0.0000000000607710050650619224932
+
+#define M_PI_OVER_2F_HI 1.570312500000000000
+#define M_PI_OVER_2F_LO 0.000483826794896558
+
+/* The following coefficients correspond to the Taylor series
+ * coefficients for cos and sin.
+ */
+#define COS_14 -0.00000000001138218794258068723867
+#define COS_12 0.000000002087614008917893178252
+#define COS_10 -0.0000002755731724204127572108
+#define COS_08 0.00002480158729870839541888
+#define COS_06 -0.001388888888888735934799
+#define COS_04 0.04166666666666666534980
+#define COS_02 -0.5000000000000000000000
+#define COS_00 1.0
+
+#define SIN_15 -0.00000000000076471637318198164759
+#define SIN_13 0.00000000016059043836821614599
+#define SIN_11 -0.000000025052108385441718775
+#define SIN_09 0.0000027557319223985890653
+#define SIN_07 -0.0001984126984126984127
+#define SIN_05 0.008333333333333333333
+#define SIN_03 -0.16666666666666666666
+#define SIN_01 1.0
+
+
+/* Compute the following for each floating point element of x.
+ * x = fmod(x, PI/4);
+ * ix = (int)x * PI/4;
+ * This allows one to compute cos / sin over the limited range
+ * and select the sign and correct result based upon the octant
+ * of the original angle (as defined by the ix result).
+ *
+ * Expected Inputs Types:
+ * x = vec_float4
+ * ix = vec_int4
+ */
+#define MOD_PI_OVER_FOUR_F(_x, _ix) { \
+ vec_float4 fx; \
+ \
+ _ix = spu_convts(spu_mul(_x, spu_splats((float)M_FOUR_OVER_PI)), 0); \
+ _ix = spu_add(_ix, spu_add(spu_rlmaska((vec_int4)_x, -31), 1)); \
+ \
+ fx = spu_convtf(spu_rlmaska(_ix, -1), 0); \
+ _x = spu_nmsub(fx, spu_splats((float)M_PI_OVER_2F_HI), _x); \
+ _x = spu_nmsub(fx, spu_splats((float)M_PI_OVER_2F_LO), _x); \
+ }
+
+/* Double precision MOD_PI_OVER_FOUR
+ *
+ * Expected Inputs Types:
+ * x = vec_double2
+ * ix = vec_int4
+ */
+#define MOD_PI_OVER_FOUR(_x, _ix) { \
+ vec_float4 fx; \
+ vec_double2 dix; \
+ \
+ fx = spu_roundtf(spu_mul(_x, spu_splats(M_FOUR_OVER_PI))); \
+ _ix = spu_convts(fx, 0); \
+ _ix = spu_add(_ix, spu_add(spu_rlmaska((vec_int4)fx, -31), 1)); \
+ \
+ dix = spu_extend(spu_convtf(spu_rlmaska(_ix, -1), 0)); \
+ _x = spu_nmsub(spu_splats(M_PI_OVER_2_HI), dix, _x); \
+ _x = spu_nmsub(spu_splats(M_PI_OVER_2_LO), dix, _x); \
+ }
+
+
+/* Compute the cos(x) and sin(x) for the range reduced angle x.
+ * In order to compute these trig functions to full single precision
+ * accuracy, we solve the Taylor series.
+ *
+ * c = cos(x) = 1 - x^2/2! + x^4/4! - x^6/6! + x^8/8! - x^10/10!
+ * s = sin(x) = x - x^3/4! + x^5/5! - x^7/7! + x^9/9! - x^11/11!
+ *
+ * Expected Inputs Types:
+ * x = vec_float4
+ * c = vec_float4
+ * s = vec_float4
+ */
+
+#define COMPUTE_COS_SIN_F(_x, _c, _s) { \
+ vec_float4 x2, x4, x6; \
+ vec_float4 cos_hi, cos_lo; \
+ vec_float4 sin_hi, sin_lo; \
+ \
+ x2 = spu_mul(_x, _x); \
+ x4 = spu_mul(x2, x2); \
+ x6 = spu_mul(x2, x4); \
+ \
+ cos_hi = spu_madd(spu_splats((float)COS_10), x2, spu_splats((float)COS_08)); \
+ cos_lo = spu_madd(spu_splats((float)COS_04), x2, spu_splats((float)COS_02)); \
+ cos_hi = spu_madd(cos_hi, x2, spu_splats((float)COS_06)); \
+ cos_lo = spu_madd(cos_lo, x2, spu_splats((float)COS_00)); \
+ _c = spu_madd(cos_hi, x6, cos_lo); \
+ \
+ sin_hi = spu_madd(spu_splats((float)SIN_11), x2, spu_splats((float)SIN_09)); \
+ sin_lo = spu_madd(spu_splats((float)SIN_05), x2, spu_splats((float)SIN_03)); \
+ sin_hi = spu_madd(sin_hi, x2, spu_splats((float)SIN_07)); \
+ sin_lo = spu_madd(sin_lo, x2, spu_splats((float)SIN_01)); \
+ _s = spu_madd(sin_hi, x6, sin_lo); \
+ _s = spu_mul(_s, _x); \
+ }
+
+
+/* Compute the cos(x) and sin(x) for the range reduced angle x.
+ * This version computes the cosine and sine to double precision
+ * accuracy using the Taylor series:
+ *
+ * c = cos(x) = 1 - x^2/2! + x^4/4! - x^6/6! + x^8/8! - x^10/10! + x^12/12! - x^14/14!
+ * s = sin(x) = x - x^3/4! + x^5/5! - x^7/7! + x^9/9! - x^11/11! + x^13/13! - x^15/15!
+ *
+ * Expected Inputs Types:
+ * x = vec_double2
+ * c = vec_double2
+ * s = vec_double2
+ */
+
+#define COMPUTE_COS_SIN(_x, _c, _s) { \
+ vec_double2 x2, x4, x8; \
+ vec_double2 cos_hi, cos_lo; \
+ vec_double2 sin_hi, sin_lo; \
+ \
+ x2 = spu_mul(_x, _x); \
+ x4 = spu_mul(x2, x2); \
+ x8 = spu_mul(x4, x4); \
+ \
+ cos_hi = spu_madd(spu_splats(COS_14), x2, spu_splats(COS_12)); \
+ cos_lo = spu_madd(spu_splats(COS_06), x2, spu_splats(COS_04)); \
+ cos_hi = spu_madd(cos_hi, x2, spu_splats(COS_10)); \
+ cos_lo = spu_madd(cos_lo, x2, spu_splats(COS_02)); \
+ cos_hi = spu_madd(cos_hi, x2, spu_splats(COS_08)); \
+ cos_lo = spu_madd(cos_lo, x2, spu_splats(COS_00)); \
+ _c = spu_madd(cos_hi, x8, cos_lo); \
+ \
+ sin_hi = spu_madd(spu_splats(SIN_15), x2, spu_splats(SIN_13)); \
+ sin_lo = spu_madd(spu_splats(SIN_07), x2, spu_splats(SIN_05)); \
+ sin_hi = spu_madd(sin_hi, x2, spu_splats(SIN_11)); \
+ sin_lo = spu_madd(sin_lo, x2, spu_splats(SIN_03)); \
+ sin_hi = spu_madd(sin_hi, x2, spu_splats(SIN_09)); \
+ sin_lo = spu_madd(sin_lo, x2, spu_splats(SIN_01)); \
+ _s = spu_madd(sin_hi, x8, sin_lo); \
+ _s = spu_mul(_s, _x); \
+ }
+
+
+
+
+#endif /* _COS_SIN_H_ */
+#endif /* __SPU__ */
+
+