mirror of
https://github.com/brl/mutter.git
synced 2024-12-23 19:42:05 +00:00
f6dce7f9e5
* clutter/x11/clutter-backend-x11.c: * clutter/clutter-event.h: * clutter/clutter-feature.h: * clutter/clutter-fixed.c: * clutter/clutter-model.h: Fix documentation. * clutter/eglnative/clutter-backend-egl.[ch]: * clutter/eglnative/clutter-event-egl.c: Add the same solution used for the SDL backend in order to get the time of an event. This should fix the motion event throttling and the click count on button press. * tests/test-pixmap.c (create_pixmap), (main): Fix preprocessor directives.
1274 lines
35 KiB
C
1274 lines
35 KiB
C
/*
|
|
* Clutter.
|
|
*
|
|
* An OpenGL based 'interactive canvas' library.
|
|
*
|
|
* Authored By Tomas Frydrych <tf@openedhand.com>
|
|
*
|
|
* Copyright (C) 2006, 2007 OpenedHand
|
|
*
|
|
* This 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 of the License, or (at your option) any later version.
|
|
*
|
|
* This library 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 this library; if not, write to the
|
|
* Free Software Foundation, Inc., 59 Temple Place - Suite 330,
|
|
* Boston, MA 02111-1307, USA.
|
|
*/
|
|
|
|
#ifdef HAVE_CONFIG_H
|
|
#include "config.h"
|
|
#endif
|
|
|
|
#include <glib-object.h>
|
|
#include <gobject/gvaluecollector.h>
|
|
|
|
#include "clutter-fixed.h"
|
|
#include "clutter-private.h"
|
|
|
|
/**
|
|
* SECTION:clutter-fixed
|
|
* @short_description: Fixed Point API
|
|
*
|
|
* Clutter has a fixed point API targeted at platforms without a
|
|
* floating point unit, such as embedded devices. On such platforms
|
|
* this API should be preferred to the floating point one as it does
|
|
* not trigger the slow path of software emulation, relying on integer
|
|
* math for fixed-to-floating and floating-to-fixed conversion.
|
|
*
|
|
* It is no recommened for use on platforms with a floating point unit
|
|
* (eg desktop systems) nor for use in bindings.
|
|
*
|
|
* Basic rules of Fixed Point arithmethic:
|
|
*
|
|
* <itemizedlist>
|
|
* <listitem>
|
|
* <para>Two fixed point numbers can be directly added and
|
|
* subtracted.</para>
|
|
* </listitem>
|
|
* <listitem>
|
|
* <para>To add other numerical type to a fixed point number it has to
|
|
* be first converted to fixed point.</para>
|
|
* </listitem>
|
|
* <listitem>
|
|
* <para>A fixed point number can be directly multiplied or divided by
|
|
* an integer.</para>
|
|
* </listitem>
|
|
* <listitem>
|
|
* <para>Two fixed point numbers can only be multiplied and divided by the
|
|
* provided #CLUTTER_FIXED_MUL and #CLUTTER_FIXED_DIV macros.</para>
|
|
* </listitem>
|
|
* </itemizedlist>
|
|
*/
|
|
|
|
/* pre-computed sin table for 1st quadrant
|
|
*
|
|
* Currently contains 257 entries.
|
|
*
|
|
* The current error (compared to system sin) is about
|
|
* 0.5% for values near the start of the table where the
|
|
* curve is steep, but improving rapidly. If this precission
|
|
* is not enough, we can increase the size of the table
|
|
*/
|
|
static ClutterFixed sin_tbl [] =
|
|
{
|
|
0x00000000L, 0x00000192L, 0x00000324L, 0x000004B6L,
|
|
0x00000648L, 0x000007DAL, 0x0000096CL, 0x00000AFEL,
|
|
0x00000C90L, 0x00000E21L, 0x00000FB3L, 0x00001144L,
|
|
0x000012D5L, 0x00001466L, 0x000015F7L, 0x00001787L,
|
|
0x00001918L, 0x00001AA8L, 0x00001C38L, 0x00001DC7L,
|
|
0x00001F56L, 0x000020E5L, 0x00002274L, 0x00002402L,
|
|
0x00002590L, 0x0000271EL, 0x000028ABL, 0x00002A38L,
|
|
0x00002BC4L, 0x00002D50L, 0x00002EDCL, 0x00003067L,
|
|
0x000031F1L, 0x0000337CL, 0x00003505L, 0x0000368EL,
|
|
0x00003817L, 0x0000399FL, 0x00003B27L, 0x00003CAEL,
|
|
0x00003E34L, 0x00003FBAL, 0x0000413FL, 0x000042C3L,
|
|
0x00004447L, 0x000045CBL, 0x0000474DL, 0x000048CFL,
|
|
0x00004A50L, 0x00004BD1L, 0x00004D50L, 0x00004ECFL,
|
|
0x0000504DL, 0x000051CBL, 0x00005348L, 0x000054C3L,
|
|
0x0000563EL, 0x000057B9L, 0x00005932L, 0x00005AAAL,
|
|
0x00005C22L, 0x00005D99L, 0x00005F0FL, 0x00006084L,
|
|
0x000061F8L, 0x0000636BL, 0x000064DDL, 0x0000664EL,
|
|
0x000067BEL, 0x0000692DL, 0x00006A9BL, 0x00006C08L,
|
|
0x00006D74L, 0x00006EDFL, 0x00007049L, 0x000071B2L,
|
|
0x0000731AL, 0x00007480L, 0x000075E6L, 0x0000774AL,
|
|
0x000078ADL, 0x00007A10L, 0x00007B70L, 0x00007CD0L,
|
|
0x00007E2FL, 0x00007F8CL, 0x000080E8L, 0x00008243L,
|
|
0x0000839CL, 0x000084F5L, 0x0000864CL, 0x000087A1L,
|
|
0x000088F6L, 0x00008A49L, 0x00008B9AL, 0x00008CEBL,
|
|
0x00008E3AL, 0x00008F88L, 0x000090D4L, 0x0000921FL,
|
|
0x00009368L, 0x000094B0L, 0x000095F7L, 0x0000973CL,
|
|
0x00009880L, 0x000099C2L, 0x00009B03L, 0x00009C42L,
|
|
0x00009D80L, 0x00009EBCL, 0x00009FF7L, 0x0000A130L,
|
|
0x0000A268L, 0x0000A39EL, 0x0000A4D2L, 0x0000A605L,
|
|
0x0000A736L, 0x0000A866L, 0x0000A994L, 0x0000AAC1L,
|
|
0x0000ABEBL, 0x0000AD14L, 0x0000AE3CL, 0x0000AF62L,
|
|
0x0000B086L, 0x0000B1A8L, 0x0000B2C9L, 0x0000B3E8L,
|
|
0x0000B505L, 0x0000B620L, 0x0000B73AL, 0x0000B852L,
|
|
0x0000B968L, 0x0000BA7DL, 0x0000BB8FL, 0x0000BCA0L,
|
|
0x0000BDAFL, 0x0000BEBCL, 0x0000BFC7L, 0x0000C0D1L,
|
|
0x0000C1D8L, 0x0000C2DEL, 0x0000C3E2L, 0x0000C4E4L,
|
|
0x0000C5E4L, 0x0000C6E2L, 0x0000C7DEL, 0x0000C8D9L,
|
|
0x0000C9D1L, 0x0000CAC7L, 0x0000CBBCL, 0x0000CCAEL,
|
|
0x0000CD9FL, 0x0000CE8EL, 0x0000CF7AL, 0x0000D065L,
|
|
0x0000D14DL, 0x0000D234L, 0x0000D318L, 0x0000D3FBL,
|
|
0x0000D4DBL, 0x0000D5BAL, 0x0000D696L, 0x0000D770L,
|
|
0x0000D848L, 0x0000D91EL, 0x0000D9F2L, 0x0000DAC4L,
|
|
0x0000DB94L, 0x0000DC62L, 0x0000DD2DL, 0x0000DDF7L,
|
|
0x0000DEBEL, 0x0000DF83L, 0x0000E046L, 0x0000E107L,
|
|
0x0000E1C6L, 0x0000E282L, 0x0000E33CL, 0x0000E3F4L,
|
|
0x0000E4AAL, 0x0000E55EL, 0x0000E610L, 0x0000E6BFL,
|
|
0x0000E76CL, 0x0000E817L, 0x0000E8BFL, 0x0000E966L,
|
|
0x0000EA0AL, 0x0000EAABL, 0x0000EB4BL, 0x0000EBE8L,
|
|
0x0000EC83L, 0x0000ED1CL, 0x0000EDB3L, 0x0000EE47L,
|
|
0x0000EED9L, 0x0000EF68L, 0x0000EFF5L, 0x0000F080L,
|
|
0x0000F109L, 0x0000F18FL, 0x0000F213L, 0x0000F295L,
|
|
0x0000F314L, 0x0000F391L, 0x0000F40CL, 0x0000F484L,
|
|
0x0000F4FAL, 0x0000F56EL, 0x0000F5DFL, 0x0000F64EL,
|
|
0x0000F6BAL, 0x0000F724L, 0x0000F78CL, 0x0000F7F1L,
|
|
0x0000F854L, 0x0000F8B4L, 0x0000F913L, 0x0000F96EL,
|
|
0x0000F9C8L, 0x0000FA1FL, 0x0000FA73L, 0x0000FAC5L,
|
|
0x0000FB15L, 0x0000FB62L, 0x0000FBADL, 0x0000FBF5L,
|
|
0x0000FC3BL, 0x0000FC7FL, 0x0000FCC0L, 0x0000FCFEL,
|
|
0x0000FD3BL, 0x0000FD74L, 0x0000FDACL, 0x0000FDE1L,
|
|
0x0000FE13L, 0x0000FE43L, 0x0000FE71L, 0x0000FE9CL,
|
|
0x0000FEC4L, 0x0000FEEBL, 0x0000FF0EL, 0x0000FF30L,
|
|
0x0000FF4EL, 0x0000FF6BL, 0x0000FF85L, 0x0000FF9CL,
|
|
0x0000FFB1L, 0x0000FFC4L, 0x0000FFD4L, 0x0000FFE1L,
|
|
0x0000FFECL, 0x0000FFF5L, 0x0000FFFBL, 0x0000FFFFL,
|
|
0x00010000L,
|
|
};
|
|
|
|
/* the difference of the angle for two adjacent values in the table
|
|
* expressed as ClutterFixed number
|
|
*/
|
|
#define CFX_SIN_STEP 0x00000192
|
|
|
|
/* <private> */
|
|
const double _magic = 68719476736.0 * 1.5;
|
|
|
|
/* Where in the 64 bits of double is the mantisa */
|
|
#if (__FLOAT_WORD_ORDER == 1234)
|
|
#define _CFX_MAN 0
|
|
#elif (__FLOAT_WORD_ORDER == 4321)
|
|
#define _CFX_MAN 1
|
|
#else
|
|
#define CFX_NO_FAST_CONVERSIONS
|
|
#endif
|
|
|
|
/*
|
|
* clutter_double_to_fixed :
|
|
* @value: value to be converted
|
|
*
|
|
* A fast conversion from double precision floating to fixed point
|
|
*
|
|
* Return value: Fixed point representation of the value
|
|
*
|
|
* Since: 0.2
|
|
*/
|
|
ClutterFixed
|
|
clutter_double_to_fixed (double val)
|
|
{
|
|
#ifdef CFX_NO_FAST_CONVERSIONS
|
|
return (ClutterFixed)(val * (double)CFX_ONE);
|
|
#else
|
|
union
|
|
{
|
|
double d;
|
|
unsigned int i[2];
|
|
} dbl;
|
|
|
|
dbl.d = val;
|
|
dbl.d = dbl.d + _magic;
|
|
return dbl.i[_CFX_MAN];
|
|
#endif
|
|
}
|
|
|
|
/*
|
|
* clutter_double_to_int :
|
|
* @value: value to be converted
|
|
*
|
|
* A fast conversion from doulbe precision floatint point to int;
|
|
* used this instead of casting double/float to int.
|
|
*
|
|
* Return value: Integer part of the double
|
|
*
|
|
* Since: 0.2
|
|
*/
|
|
gint
|
|
clutter_double_to_int (double val)
|
|
{
|
|
#ifdef CFX_NO_FAST_CONVERSIONS
|
|
return (gint)(val);
|
|
#else
|
|
union
|
|
{
|
|
double d;
|
|
unsigned int i[2];
|
|
} dbl;
|
|
|
|
dbl.d = val;
|
|
dbl.d = dbl.d + _magic;
|
|
return ((int)dbl.i[_CFX_MAN]) >> 16;
|
|
#endif
|
|
}
|
|
|
|
guint
|
|
clutter_double_to_uint (double val)
|
|
{
|
|
#ifdef CFX_NO_FAST_CONVERSIONS
|
|
return (guint)(val);
|
|
#else
|
|
union
|
|
{
|
|
double d;
|
|
unsigned int i[2];
|
|
} dbl;
|
|
|
|
dbl.d = val;
|
|
dbl.d = dbl.d + _magic;
|
|
return (dbl.i[_CFX_MAN]) >> 16;
|
|
#endif
|
|
}
|
|
|
|
#undef _CFX_MAN
|
|
|
|
/**
|
|
* clutter_sinx:
|
|
* @angle: a #ClutterFixed angle in radians
|
|
*
|
|
* Fixed point implementation of sine function
|
|
*
|
|
* Return value: #ClutterFixed sine value.
|
|
*
|
|
* Since: 0.2
|
|
*/
|
|
ClutterFixed
|
|
clutter_sinx (ClutterFixed angle)
|
|
{
|
|
int sign = 1, indx1, indx2;
|
|
ClutterFixed low, high, d1, d2;
|
|
|
|
/* convert negative angle to positive + sign */
|
|
if ((int)angle < 0)
|
|
{
|
|
sign = 1 + ~sign;
|
|
angle = 1 + ~angle;
|
|
}
|
|
|
|
/* reduce to <0, 2*pi) */
|
|
if (angle >= CFX_2PI)
|
|
{
|
|
ClutterFixed f = CLUTTER_FIXED_DIV (angle, CFX_2PI);
|
|
angle = angle - f;
|
|
}
|
|
|
|
/* reduce to first quadrant and sign */
|
|
if (angle > CFX_PI)
|
|
{
|
|
sign = 1 + ~sign;
|
|
if (angle > CFX_PI + CFX_PI_2)
|
|
{
|
|
/* fourth qudrant */
|
|
angle = CFX_2PI - angle;
|
|
}
|
|
else
|
|
{
|
|
/* third quadrant */
|
|
angle -= CFX_PI;
|
|
}
|
|
}
|
|
else
|
|
{
|
|
if (angle > CFX_PI_2)
|
|
{
|
|
/* second quadrant */
|
|
angle = CFX_PI - angle;
|
|
}
|
|
}
|
|
|
|
/* Calculate indices of the two nearest values in our table
|
|
* and return weighted average
|
|
*
|
|
* Handle the end of the table gracefully
|
|
*/
|
|
indx1 = CLUTTER_FIXED_DIV (angle, CFX_SIN_STEP);
|
|
indx1 = CLUTTER_FIXED_TO_INT (indx1);
|
|
|
|
if (indx1 == sizeof (sin_tbl)/sizeof (ClutterFixed) - 1)
|
|
{
|
|
indx2 = indx1;
|
|
indx1 = indx2 - 1;
|
|
}
|
|
else
|
|
{
|
|
indx2 = indx1 + 1;
|
|
}
|
|
|
|
low = sin_tbl[indx1];
|
|
high = sin_tbl[indx2];
|
|
|
|
d1 = angle - indx1 * CFX_SIN_STEP;
|
|
d2 = indx2 * CFX_SIN_STEP - angle;
|
|
|
|
angle = ((low * d2 + high * d1) / (CFX_SIN_STEP));
|
|
|
|
if (sign < 0)
|
|
angle = (1 + ~angle);
|
|
|
|
return angle;
|
|
}
|
|
|
|
/**
|
|
* clutter_sini:
|
|
* @angle: a #ClutterAngle
|
|
*
|
|
* Very fast fixed point implementation of sine function.
|
|
*
|
|
* ClutterAngle is an integer such that 1024 represents
|
|
* full circle.
|
|
*
|
|
* Return value: #ClutterFixed sine value.
|
|
*
|
|
* Since: 0.2
|
|
*/
|
|
ClutterFixed
|
|
clutter_sini (ClutterAngle angle)
|
|
{
|
|
int sign = 1;
|
|
ClutterFixed result;
|
|
|
|
/* reduce negative angle to positive + sign */
|
|
if (angle < 0)
|
|
{
|
|
sign = 1 + ~sign;
|
|
angle = 1 + ~angle;
|
|
}
|
|
|
|
/* reduce to <0, 2*pi) */
|
|
angle &= 0x3ff;
|
|
|
|
/* reduce to first quadrant and sign */
|
|
if (angle > 512)
|
|
{
|
|
sign = 1 + ~sign;
|
|
if (angle > 768)
|
|
{
|
|
/* fourth qudrant */
|
|
angle = 1024 - angle;
|
|
}
|
|
else
|
|
{
|
|
/* third quadrant */
|
|
angle -= 512;
|
|
}
|
|
}
|
|
else
|
|
{
|
|
if (angle > 256)
|
|
{
|
|
/* second quadrant */
|
|
angle = 512 - angle;
|
|
}
|
|
}
|
|
|
|
result = sin_tbl[angle];
|
|
|
|
if (sign < 0)
|
|
result = (1 + ~result);
|
|
|
|
return result;
|
|
}
|
|
|
|
/* pre-computed tan table for 1st quadrant
|
|
*
|
|
* Currently contains 257 entries.
|
|
*
|
|
*/
|
|
static ClutterFixed tan_tbl [] =
|
|
{
|
|
0x00000000L, 0x00000192L, 0x00000324L, 0x000004b7L,
|
|
0x00000649L, 0x000007dbL, 0x0000096eL, 0x00000b01L,
|
|
0x00000c94L, 0x00000e27L, 0x00000fbaL, 0x0000114eL,
|
|
0x000012e2L, 0x00001477L, 0x0000160cL, 0x000017a1L,
|
|
0x00001937L, 0x00001acdL, 0x00001c64L, 0x00001dfbL,
|
|
0x00001f93L, 0x0000212cL, 0x000022c5L, 0x0000245fL,
|
|
0x000025f9L, 0x00002795L, 0x00002931L, 0x00002aceL,
|
|
0x00002c6cL, 0x00002e0aL, 0x00002faaL, 0x0000314aL,
|
|
0x000032ecL, 0x0000348eL, 0x00003632L, 0x000037d7L,
|
|
0x0000397dL, 0x00003b24L, 0x00003cccL, 0x00003e75L,
|
|
0x00004020L, 0x000041ccL, 0x00004379L, 0x00004528L,
|
|
0x000046d8L, 0x0000488aL, 0x00004a3dL, 0x00004bf2L,
|
|
0x00004da8L, 0x00004f60L, 0x0000511aL, 0x000052d5L,
|
|
0x00005492L, 0x00005651L, 0x00005812L, 0x000059d5L,
|
|
0x00005b99L, 0x00005d60L, 0x00005f28L, 0x000060f3L,
|
|
0x000062c0L, 0x0000648fL, 0x00006660L, 0x00006834L,
|
|
0x00006a0aL, 0x00006be2L, 0x00006dbdL, 0x00006f9aL,
|
|
0x0000717aL, 0x0000735dL, 0x00007542L, 0x0000772aL,
|
|
0x00007914L, 0x00007b02L, 0x00007cf2L, 0x00007ee6L,
|
|
0x000080dcL, 0x000082d6L, 0x000084d2L, 0x000086d2L,
|
|
0x000088d6L, 0x00008adcL, 0x00008ce7L, 0x00008ef4L,
|
|
0x00009106L, 0x0000931bL, 0x00009534L, 0x00009750L,
|
|
0x00009971L, 0x00009b95L, 0x00009dbeL, 0x00009febL,
|
|
0x0000a21cL, 0x0000a452L, 0x0000a68cL, 0x0000a8caL,
|
|
0x0000ab0eL, 0x0000ad56L, 0x0000afa3L, 0x0000b1f5L,
|
|
0x0000b44cL, 0x0000b6a8L, 0x0000b909L, 0x0000bb70L,
|
|
0x0000bdddL, 0x0000c04fL, 0x0000c2c7L, 0x0000c545L,
|
|
0x0000c7c9L, 0x0000ca53L, 0x0000cce3L, 0x0000cf7aL,
|
|
0x0000d218L, 0x0000d4bcL, 0x0000d768L, 0x0000da1aL,
|
|
0x0000dcd4L, 0x0000df95L, 0x0000e25eL, 0x0000e52eL,
|
|
0x0000e806L, 0x0000eae7L, 0x0000edd0L, 0x0000f0c1L,
|
|
0x0000f3bbL, 0x0000f6bfL, 0x0000f9cbL, 0x0000fce1L,
|
|
0x00010000L, 0x00010329L, 0x0001065dL, 0x0001099aL,
|
|
0x00010ce3L, 0x00011036L, 0x00011394L, 0x000116feL,
|
|
0x00011a74L, 0x00011df6L, 0x00012184L, 0x0001251fL,
|
|
0x000128c6L, 0x00012c7cL, 0x0001303fL, 0x00013410L,
|
|
0x000137f0L, 0x00013bdfL, 0x00013fddL, 0x000143ebL,
|
|
0x00014809L, 0x00014c37L, 0x00015077L, 0x000154c9L,
|
|
0x0001592dL, 0x00015da4L, 0x0001622eL, 0x000166ccL,
|
|
0x00016b7eL, 0x00017045L, 0x00017523L, 0x00017a17L,
|
|
0x00017f22L, 0x00018444L, 0x00018980L, 0x00018ed5L,
|
|
0x00019445L, 0x000199cfL, 0x00019f76L, 0x0001a53aL,
|
|
0x0001ab1cL, 0x0001b11dL, 0x0001b73fL, 0x0001bd82L,
|
|
0x0001c3e7L, 0x0001ca71L, 0x0001d11fL, 0x0001d7f4L,
|
|
0x0001def1L, 0x0001e618L, 0x0001ed6aL, 0x0001f4e8L,
|
|
0x0001fc96L, 0x00020473L, 0x00020c84L, 0x000214c9L,
|
|
0x00021d44L, 0x000225f9L, 0x00022ee9L, 0x00023818L,
|
|
0x00024187L, 0x00024b3aL, 0x00025534L, 0x00025f78L,
|
|
0x00026a0aL, 0x000274edL, 0x00028026L, 0x00028bb8L,
|
|
0x000297a8L, 0x0002a3fbL, 0x0002b0b5L, 0x0002bdddL,
|
|
0x0002cb79L, 0x0002d98eL, 0x0002e823L, 0x0002f740L,
|
|
0x000306ecL, 0x00031730L, 0x00032816L, 0x000339a6L,
|
|
0x00034bebL, 0x00035ef2L, 0x000372c6L, 0x00038776L,
|
|
0x00039d11L, 0x0003b3a6L, 0x0003cb48L, 0x0003e40aL,
|
|
0x0003fe02L, 0x00041949L, 0x000435f7L, 0x0004542bL,
|
|
0x00047405L, 0x000495a9L, 0x0004b940L, 0x0004def6L,
|
|
0x00050700L, 0x00053196L, 0x00055ef9L, 0x00058f75L,
|
|
0x0005c35dL, 0x0005fb14L, 0x00063709L, 0x000677c0L,
|
|
0x0006bdd0L, 0x000709ecL, 0x00075ce6L, 0x0007b7bbL,
|
|
0x00081b98L, 0x000889e9L, 0x0009046eL, 0x00098d4dL,
|
|
0x000a2736L, 0x000ad593L, 0x000b9cc6L, 0x000c828aL,
|
|
0x000d8e82L, 0x000ecb1bL, 0x001046eaL, 0x00121703L,
|
|
0x00145b00L, 0x0017448dL, 0x001b2672L, 0x002095afL,
|
|
0x0028bc49L, 0x0036519aL, 0x00517bb6L, 0x00a2f8fdL,
|
|
0x46d3eab2L,
|
|
};
|
|
|
|
/**
|
|
* clutter_tani:
|
|
* @angle: a #ClutterAngle
|
|
*
|
|
* Very fast fixed point implementation of tan function.
|
|
*
|
|
* ClutterAngle is an integer such that 1024 represents
|
|
* full circle.
|
|
*
|
|
* Return value: #ClutterFixed sine value.
|
|
*
|
|
* Since: 0.3
|
|
*/
|
|
ClutterFixed
|
|
clutter_tani (ClutterAngle angle)
|
|
{
|
|
int sign = 1;
|
|
ClutterFixed result;
|
|
|
|
/* reduce negative angle to positive + sign */
|
|
if (angle < 0)
|
|
{
|
|
sign = 1 + ~sign;
|
|
angle = 1 + ~angle;
|
|
}
|
|
|
|
/* reduce to <0, pi) */
|
|
angle &= 0x1ff;
|
|
|
|
/* reduce to first quadrant and sign */
|
|
if (angle > 256)
|
|
{
|
|
sign = 1 + ~sign;
|
|
angle = 512 - angle;
|
|
}
|
|
|
|
result = tan_tbl[angle];
|
|
|
|
if (sign < 0)
|
|
result = (1 + ~result);
|
|
|
|
return result;
|
|
}
|
|
|
|
ClutterFixed sqrt_tbl [] =
|
|
{
|
|
0x00000000L, 0x00010000L, 0x00016A0AL, 0x0001BB68L,
|
|
0x00020000L, 0x00023C6FL, 0x00027312L, 0x0002A550L,
|
|
0x0002D414L, 0x00030000L, 0x0003298BL, 0x0003510EL,
|
|
0x000376CFL, 0x00039B05L, 0x0003BDDDL, 0x0003DF7CL,
|
|
0x00040000L, 0x00041F84L, 0x00043E1EL, 0x00045BE1L,
|
|
0x000478DEL, 0x00049524L, 0x0004B0BFL, 0x0004CBBCL,
|
|
0x0004E624L, 0x00050000L, 0x00051959L, 0x00053237L,
|
|
0x00054AA0L, 0x0005629AL, 0x00057A2BL, 0x00059159L,
|
|
0x0005A828L, 0x0005BE9CL, 0x0005D4B9L, 0x0005EA84L,
|
|
0x00060000L, 0x00061530L, 0x00062A17L, 0x00063EB8L,
|
|
0x00065316L, 0x00066733L, 0x00067B12L, 0x00068EB4L,
|
|
0x0006A21DL, 0x0006B54DL, 0x0006C847L, 0x0006DB0CL,
|
|
0x0006ED9FL, 0x00070000L, 0x00071232L, 0x00072435L,
|
|
0x0007360BL, 0x000747B5L, 0x00075935L, 0x00076A8CL,
|
|
0x00077BBBL, 0x00078CC2L, 0x00079DA3L, 0x0007AE60L,
|
|
0x0007BEF8L, 0x0007CF6DL, 0x0007DFBFL, 0x0007EFF0L,
|
|
0x00080000L, 0x00080FF0L, 0x00081FC1L, 0x00082F73L,
|
|
0x00083F08L, 0x00084E7FL, 0x00085DDAL, 0x00086D18L,
|
|
0x00087C3BL, 0x00088B44L, 0x00089A32L, 0x0008A906L,
|
|
0x0008B7C2L, 0x0008C664L, 0x0008D4EEL, 0x0008E361L,
|
|
0x0008F1BCL, 0x00090000L, 0x00090E2EL, 0x00091C45L,
|
|
0x00092A47L, 0x00093834L, 0x0009460CL, 0x000953CFL,
|
|
0x0009617EL, 0x00096F19L, 0x00097CA1L, 0x00098A16L,
|
|
0x00099777L, 0x0009A4C6L, 0x0009B203L, 0x0009BF2EL,
|
|
0x0009CC47L, 0x0009D94FL, 0x0009E645L, 0x0009F32BL,
|
|
0x000A0000L, 0x000A0CC5L, 0x000A1979L, 0x000A261EL,
|
|
0x000A32B3L, 0x000A3F38L, 0x000A4BAEL, 0x000A5816L,
|
|
0x000A646EL, 0x000A70B8L, 0x000A7CF3L, 0x000A8921L,
|
|
0x000A9540L, 0x000AA151L, 0x000AAD55L, 0x000AB94BL,
|
|
0x000AC534L, 0x000AD110L, 0x000ADCDFL, 0x000AE8A1L,
|
|
0x000AF457L, 0x000B0000L, 0x000B0B9DL, 0x000B172DL,
|
|
0x000B22B2L, 0x000B2E2BL, 0x000B3998L, 0x000B44F9L,
|
|
0x000B504FL, 0x000B5B9AL, 0x000B66D9L, 0x000B720EL,
|
|
0x000B7D37L, 0x000B8856L, 0x000B936AL, 0x000B9E74L,
|
|
0x000BA973L, 0x000BB467L, 0x000BBF52L, 0x000BCA32L,
|
|
0x000BD508L, 0x000BDFD5L, 0x000BEA98L, 0x000BF551L,
|
|
0x000C0000L, 0x000C0AA6L, 0x000C1543L, 0x000C1FD6L,
|
|
0x000C2A60L, 0x000C34E1L, 0x000C3F59L, 0x000C49C8L,
|
|
0x000C542EL, 0x000C5E8CL, 0x000C68E0L, 0x000C732DL,
|
|
0x000C7D70L, 0x000C87ACL, 0x000C91DFL, 0x000C9C0AL,
|
|
0x000CA62CL, 0x000CB047L, 0x000CBA59L, 0x000CC464L,
|
|
0x000CCE66L, 0x000CD861L, 0x000CE254L, 0x000CEC40L,
|
|
0x000CF624L, 0x000D0000L, 0x000D09D5L, 0x000D13A2L,
|
|
0x000D1D69L, 0x000D2727L, 0x000D30DFL, 0x000D3A90L,
|
|
0x000D4439L, 0x000D4DDCL, 0x000D5777L, 0x000D610CL,
|
|
0x000D6A9AL, 0x000D7421L, 0x000D7DA1L, 0x000D871BL,
|
|
0x000D908EL, 0x000D99FAL, 0x000DA360L, 0x000DACBFL,
|
|
0x000DB618L, 0x000DBF6BL, 0x000DC8B7L, 0x000DD1FEL,
|
|
0x000DDB3DL, 0x000DE477L, 0x000DEDABL, 0x000DF6D8L,
|
|
0x000E0000L, 0x000E0922L, 0x000E123DL, 0x000E1B53L,
|
|
0x000E2463L, 0x000E2D6DL, 0x000E3672L, 0x000E3F70L,
|
|
0x000E4869L, 0x000E515DL, 0x000E5A4BL, 0x000E6333L,
|
|
0x000E6C16L, 0x000E74F3L, 0x000E7DCBL, 0x000E869DL,
|
|
0x000E8F6BL, 0x000E9832L, 0x000EA0F5L, 0x000EA9B2L,
|
|
0x000EB26BL, 0x000EBB1EL, 0x000EC3CBL, 0x000ECC74L,
|
|
0x000ED518L, 0x000EDDB7L, 0x000EE650L, 0x000EEEE5L,
|
|
0x000EF775L, 0x000F0000L, 0x000F0886L, 0x000F1107L,
|
|
0x000F1984L, 0x000F21FCL, 0x000F2A6FL, 0x000F32DDL,
|
|
0x000F3B47L, 0x000F43ACL, 0x000F4C0CL, 0x000F5468L,
|
|
0x000F5CBFL, 0x000F6512L, 0x000F6D60L, 0x000F75AAL,
|
|
0x000F7DEFL, 0x000F8630L, 0x000F8E6DL, 0x000F96A5L,
|
|
0x000F9ED9L, 0x000FA709L, 0x000FAF34L, 0x000FB75BL,
|
|
0x000FBF7EL, 0x000FC79DL, 0x000FCFB7L, 0x000FD7CEL,
|
|
0x000FDFE0L, 0x000FE7EEL, 0x000FEFF8L, 0x000FF7FEL,
|
|
0x00100000L,
|
|
};
|
|
|
|
/**
|
|
* clutter_sqrtx:
|
|
* @x: a #ClutterFixed
|
|
*
|
|
* A fixed point implementation of squre root
|
|
*
|
|
* Return value: #ClutterFixed square root.
|
|
*
|
|
* Since: 0.2
|
|
*/
|
|
ClutterFixed
|
|
clutter_sqrtx (ClutterFixed x)
|
|
{
|
|
/* The idea for this comes from the Alegro library, exploiting the
|
|
* fact that,
|
|
* sqrt (x) = sqrt (x/d) * sqrt (d);
|
|
*
|
|
* For d == 2^(n):
|
|
*
|
|
* sqrt (x) = sqrt (x/2^(2n)) * 2^n
|
|
*
|
|
* By locating suitable n for given x such that x >> 2n is in <0,255>
|
|
* we can use a LUT of precomputed values.
|
|
*
|
|
* This algorithm provides both good performance and precission;
|
|
* on ARM this function is about 5 times faster than c-lib sqrt, whilst
|
|
* producing errors < 1%.
|
|
*
|
|
*/
|
|
int t = 0;
|
|
int sh = 0;
|
|
unsigned int mask = 0x40000000;
|
|
unsigned fract = x & 0x0000ffff;
|
|
unsigned int d1, d2;
|
|
ClutterFixed v1, v2;
|
|
|
|
if (x <= 0)
|
|
return 0;
|
|
|
|
if (x > CFX_255 || x < CFX_ONE)
|
|
{
|
|
/*
|
|
* Find the highest bit set
|
|
*/
|
|
#if __arm__
|
|
/* This actually requires at least arm v5, but gcc does not seem
|
|
* to set the architecture defines correctly, and it is I think
|
|
* very unlikely that anyone will want to use clutter on anything
|
|
* less than v5.
|
|
*/
|
|
int bit;
|
|
__asm__ ("clz %0, %1\n"
|
|
"rsb %0, %0, #31\n"
|
|
:"=r"(bit)
|
|
:"r" (x));
|
|
|
|
/* make even (2n) */
|
|
bit &= 0xfffffffe;
|
|
#else
|
|
/* TODO -- add i386 branch using bshr
|
|
*
|
|
* NB: it's been said that the bshr instruction is poorly implemented
|
|
* and that it is possible to write a faster code in C using binary
|
|
* search -- at some point we should explore this
|
|
*/
|
|
int bit = 30;
|
|
while (bit >= 0)
|
|
{
|
|
if (x & mask)
|
|
break;
|
|
|
|
mask = (mask >> 1 | mask >> 2);
|
|
bit -= 2;
|
|
}
|
|
#endif
|
|
|
|
/* now bit indicates the highest bit set; there are two scenarios
|
|
*
|
|
* 1) bit < 23: Our number is smaller so we shift it left to maximase
|
|
* precision (< 16 really, since <16,23> never goes
|
|
* through here.
|
|
*
|
|
* 2) bit > 23: our number is above the table, so we shift right
|
|
*/
|
|
|
|
sh = ((bit - 22) >> 1);
|
|
if (bit >= 8)
|
|
t = (x >> (16 - 22 + bit));
|
|
else
|
|
t = (x << (22 - 16 - bit));
|
|
}
|
|
else
|
|
{
|
|
t = CLUTTER_FIXED_TO_INT (x);
|
|
}
|
|
|
|
/* Do a weighted average of the two nearest values */
|
|
v1 = sqrt_tbl[t];
|
|
v2 = sqrt_tbl[t+1];
|
|
|
|
/*
|
|
* 12 is fairly arbitrary -- we want integer that is not too big to cost
|
|
* us precission
|
|
*/
|
|
d1 = (unsigned)(fract) >> 12;
|
|
d2 = ((unsigned)CFX_ONE >> 12) - d1;
|
|
|
|
x = ((v1*d2) + (v2*d1))/(CFX_ONE >> 12);
|
|
|
|
if (sh > 0)
|
|
x = x << sh;
|
|
else if (sh < 0)
|
|
x = (x >> (1 + ~sh));
|
|
|
|
return x;
|
|
}
|
|
|
|
/**
|
|
* clutter_sqrti:
|
|
* @x: integer value
|
|
*
|
|
* Very fast fixed point implementation of square root for integers.
|
|
*
|
|
* This function is at least 6x faster than clib sqrt() on x86, and (this is
|
|
* not a typo!) about 500x faster on ARM without FPU. It's error is < 5%
|
|
* for arguments < #CLUTTER_SQRTI_ARG_5_PERCENT and < 10% for arguments <
|
|
* #CLUTTER_SQRTI_ARG_10_PERCENT. The maximum argument that can be passed to
|
|
* this function is CLUTTER_SQRTI_ARG_MAX.
|
|
*
|
|
* Return value: integer square root.
|
|
*
|
|
*
|
|
* Since: 0.2
|
|
*/
|
|
gint
|
|
clutter_sqrti (gint number)
|
|
{
|
|
#if defined __SSE2__
|
|
/* The GCC built-in with SSE2 (sqrtsd) is up to twice as fast as
|
|
* the pure integer code below. It is also more accurate.
|
|
*/
|
|
return __builtin_sqrt (number);
|
|
#else
|
|
/* This is a fixed point implementation of the Quake III sqrt algorithm,
|
|
* described, for example, at
|
|
* http://www.codemaestro.com/reviews/review00000105.html
|
|
*
|
|
* While the original QIII is extremely fast, the use of floating division
|
|
* and multiplication makes it perform very on arm processors without FPU.
|
|
*
|
|
* The key to successfully replacing the floating point operations with
|
|
* fixed point is in the choice of the fixed point format. The QIII
|
|
* algorithm does not calculate the square root, but its reciprocal ('y'
|
|
* below), which is only at the end turned to the inverse value. In order
|
|
* for the algorithm to produce satisfactory results, the reciprocal value
|
|
* must be represented with sufficient precission; the 16.16 we use
|
|
* elsewhere in clutter is not good enough, and 10.22 is used instead.
|
|
*/
|
|
ClutterFixed x;
|
|
guint32 y_1; /* 10.22 fixed point */
|
|
guint32 f = 0x600000; /* '1.5' as 10.22 fixed */
|
|
|
|
union
|
|
{
|
|
float f;
|
|
guint32 i;
|
|
} flt, flt2;
|
|
|
|
flt.f = number;
|
|
|
|
x = CLUTTER_INT_TO_FIXED (number) / 2;
|
|
|
|
/* The QIII initial estimate */
|
|
flt.i = 0x5f3759df - ( flt.i >> 1 );
|
|
|
|
/* Now, we convert the float to 10.22 fixed. We exploit the mechanism
|
|
* described at http://www.d6.com/users/checker/pdfs/gdmfp.pdf.
|
|
*
|
|
* We want 22 bit fraction; a single precission float uses 23 bit
|
|
* mantisa, so we only need to add 2^(23-22) (no need for the 1.5
|
|
* multiplier as we are only dealing with positive numbers).
|
|
*
|
|
* Note: we have to use two separate variables here -- for some reason,
|
|
* if we try to use just the flt variable, gcc on ARM optimises the whole
|
|
* addition out, and it all goes pear shape, since without it, the bits
|
|
* in the float will not be correctly aligned.
|
|
*/
|
|
flt2.f = flt.f + 2.0;
|
|
flt2.i &= 0x7FFFFF;
|
|
|
|
/* Now we correct the estimate */
|
|
y_1 = (flt2.i >> 11) * (flt2.i >> 11);
|
|
y_1 = (y_1 >> 8) * (x >> 8);
|
|
|
|
y_1 = f - y_1;
|
|
flt2.i = (flt2.i >> 11) * (y_1 >> 11);
|
|
|
|
/* If the original argument is less than 342, we do another
|
|
* iteration to improve precission (for arguments >= 342, the single
|
|
* iteration produces generally better results).
|
|
*/
|
|
if (x < 171)
|
|
{
|
|
y_1 = (flt2.i >> 11) * (flt2.i >> 11);
|
|
y_1 = (y_1 >> 8) * (x >> 8);
|
|
|
|
y_1 = f - y_1;
|
|
flt2.i = (flt2.i >> 11) * (y_1 >> 11);
|
|
}
|
|
|
|
/* Invert, round and convert from 10.22 to an integer
|
|
* 0x1e3c68 is a magical rounding constant that produces slightly
|
|
* better results than 0x200000.
|
|
*/
|
|
return (number * flt2.i + 0x1e3c68) >> 22;
|
|
#endif
|
|
}
|
|
|
|
/**
|
|
* clutter_qmulx:
|
|
* @op1: #ClutterFixed
|
|
* @op2: #ClutterFixed
|
|
*
|
|
* Multiplies two fixed values using 64bit arithmetic; this provides
|
|
* significantly better precission than the #CLUTTER_FIXED_MUL macro,
|
|
* but at performance cost (about 2.7 times slowdown on ARMv5e, and 2 times
|
|
* on x86).
|
|
*
|
|
* Return value: the result of the operation
|
|
*
|
|
* Since: 0.4
|
|
*/
|
|
ClutterFixed
|
|
clutter_qmulx (ClutterFixed op1, ClutterFixed op2)
|
|
{
|
|
#ifdef __arm__
|
|
/* This provides about 12% speedeup on the gcc -O2 optimised
|
|
* C version
|
|
*
|
|
* Based on code found in the following thread:
|
|
* http://lists.mplayerhq.hu/pipermail/ffmpeg-devel/2006-August/014405.html
|
|
*/
|
|
int res_low, res_hi;
|
|
|
|
__asm__ ("smull %0, %1, %2, %3 \n"
|
|
"mov %0, %0, lsr %4 \n"
|
|
"add %1, %0, %1, lsl %5 \n"
|
|
: "=r"(res_hi), "=r"(res_low)\
|
|
: "r"(op1), "r"(op2), "i"(CFX_Q), "i"(32-CFX_Q));
|
|
|
|
return (ClutterFixed) res_low;
|
|
#else
|
|
long long r = (long long) op1 * (long long) op2;
|
|
|
|
return (unsigned int)(r >> CFX_Q);
|
|
#endif
|
|
}
|
|
|
|
/**
|
|
* clutter_qdivx:
|
|
* @op1: #ClutterFixed
|
|
* @op2: #ClutterFixed
|
|
*
|
|
* Return value: #ClutterFixed.
|
|
*
|
|
* Divides two fixed values using 64bit arithmetic; this provides
|
|
* significantly better precission than the #CLUTTER_FIXED_DIV macro,
|
|
* but at performance cost.
|
|
*
|
|
* Since: 0.4
|
|
*/
|
|
ClutterFixed
|
|
clutter_qdivx (ClutterFixed op1, ClutterFixed op2)
|
|
{
|
|
return (ClutterFixed)((((gint64)op1) << CFX_Q) / op2);
|
|
}
|
|
|
|
/*
|
|
* The log2x() and pow2x() functions
|
|
*
|
|
* The implementation of the log2x() and pow2x() exploits the well-documented
|
|
* fact that the exponent part of IEEE floating number provides a good estimate
|
|
* of log2 of that number, while the mantisa serves as a good error-correction.
|
|
*
|
|
* The implemenation here uses a quadratic error correction as described by
|
|
* Ian Stephenson at http://www.dctsystems.co.uk/Software/power.html.
|
|
*/
|
|
|
|
/**
|
|
* clutter_log2x :
|
|
* @x: value to calculate base 2 logarithm from
|
|
*
|
|
* Calculates base 2 logarithm.
|
|
*
|
|
* This function is some 2.5 times faster on x86, and over 12 times faster on
|
|
* fpu-less arm, than using libc log().
|
|
*
|
|
* Return value: base 2 logarithm.
|
|
*
|
|
* Since: 0.4
|
|
*/
|
|
ClutterFixed
|
|
clutter_log2x (guint x)
|
|
{
|
|
/* Note: we could easily have a version for ClutterFixed x, but the int
|
|
* precission is enough for the current purposes.
|
|
*/
|
|
union
|
|
{
|
|
float f;
|
|
ClutterFixed i;
|
|
} flt;
|
|
|
|
ClutterFixed magic = 0x58bb;
|
|
ClutterFixed y;
|
|
|
|
/*
|
|
* Convert x to float, then extract exponent.
|
|
*
|
|
* We want the result to be 16.16 fixed, so we shift (23-16) bits only
|
|
*/
|
|
flt.f = x;
|
|
flt.i >>= 7;
|
|
flt.i -= CLUTTER_INT_TO_FIXED (127);
|
|
|
|
y = CLUTTER_FIXED_FRACTION (flt.i);
|
|
|
|
y = CFX_MUL ((y - CFX_MUL (y, y)), magic);
|
|
|
|
return flt.i + y;
|
|
}
|
|
|
|
/**
|
|
* clutter_pow2x :
|
|
* @x: exponent
|
|
*
|
|
* Calculates 2 to x power.
|
|
*
|
|
* This function is around 11 times faster on x86, and around 22 times faster
|
|
* on fpu-less arm than libc pow(2, x).
|
|
*
|
|
* Return value: 2 in x power.
|
|
*
|
|
* Since: 0.4
|
|
*/
|
|
guint
|
|
clutter_pow2x (ClutterFixed x)
|
|
{
|
|
/* Note: we could easily have a version that produces ClutterFixed result,
|
|
* but the the range would be limited to x < 15, and the int precission
|
|
* is enough for the current purposes.
|
|
*/
|
|
|
|
union
|
|
{
|
|
float f;
|
|
guint32 i;
|
|
} flt;
|
|
|
|
ClutterFixed magic = 0x56f7;
|
|
ClutterFixed y;
|
|
|
|
flt.i = x;
|
|
|
|
/*
|
|
* Reverse of the log2x function -- convert the fixed value to a suitable
|
|
* floating point exponent, and mantisa adjusted with quadratic error
|
|
* correction y.
|
|
*/
|
|
y = CLUTTER_FIXED_FRACTION (x);
|
|
y = CFX_MUL ((y - CFX_MUL (y, y)), magic);
|
|
|
|
/* Shift the exponent into it's position in the floating point
|
|
* representation; as our number is not int but 16.16 fixed, shift only
|
|
* by (23 - 16)
|
|
*/
|
|
flt.i += (CLUTTER_INT_TO_FIXED (127) - y);
|
|
flt.i <<= 7;
|
|
|
|
return CLUTTER_FLOAT_TO_UINT (flt.f);
|
|
}
|
|
|
|
|
|
/**
|
|
* clutter_powx :
|
|
* @x: base
|
|
* @y: #ClutterFixed exponent
|
|
*
|
|
* Calculates x to y power. (Note, if x is a constant it will be faster to
|
|
* calculate the power as clutter_pow2x (CLUTTER_FIXED_MUL(y, log2 (x)))
|
|
*
|
|
* Return value: x in y power.
|
|
*
|
|
* Since: 0.4
|
|
*/
|
|
guint
|
|
clutter_powx (guint x, ClutterFixed y)
|
|
{
|
|
return clutter_pow2x (CFX_MUL (y, clutter_log2x (x)));
|
|
}
|
|
|
|
static GTypeInfo _info = {
|
|
0,
|
|
NULL,
|
|
NULL,
|
|
NULL,
|
|
NULL,
|
|
NULL,
|
|
0,
|
|
0,
|
|
NULL,
|
|
NULL,
|
|
};
|
|
|
|
static GTypeFundamentalInfo _finfo = { 0, };
|
|
|
|
static void
|
|
clutter_value_init_fixed (GValue *value)
|
|
{
|
|
value->data[0].v_int = 0;
|
|
}
|
|
|
|
static void
|
|
clutter_value_copy_fixed (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_int = src->data[0].v_int;
|
|
}
|
|
|
|
static gchar *
|
|
clutter_value_collect_fixed (GValue *value,
|
|
guint n_collect_values,
|
|
GTypeCValue *collect_values,
|
|
guint collect_flags)
|
|
{
|
|
value->data[0].v_int = collect_values[0].v_int;
|
|
|
|
return NULL;
|
|
}
|
|
|
|
static gchar *
|
|
clutter_value_lcopy_fixed (const GValue *value,
|
|
guint n_collect_values,
|
|
GTypeCValue *collect_values,
|
|
guint collect_flags)
|
|
{
|
|
gint32 *fixed_p = collect_values[0].v_pointer;
|
|
|
|
if (!fixed_p)
|
|
return g_strdup_printf ("value location for `%s' passed as NULL",
|
|
G_VALUE_TYPE_NAME (value));
|
|
|
|
*fixed_p = value->data[0].v_int;
|
|
|
|
return NULL;
|
|
}
|
|
|
|
static void
|
|
clutter_value_transform_fixed_int (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_int = CLUTTER_FIXED_TO_INT (src->data[0].v_int);
|
|
}
|
|
|
|
static void
|
|
clutter_value_transform_fixed_double (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_double = CLUTTER_FIXED_TO_DOUBLE (src->data[0].v_int);
|
|
}
|
|
|
|
static void
|
|
clutter_value_transform_fixed_float (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_float = CLUTTER_FIXED_TO_FLOAT (src->data[0].v_int);
|
|
}
|
|
|
|
static void
|
|
clutter_value_transform_int_fixed (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_int = CLUTTER_INT_TO_FIXED (src->data[0].v_int);
|
|
}
|
|
|
|
static void
|
|
clutter_value_transform_double_fixed (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_int = CLUTTER_FLOAT_TO_FIXED (src->data[0].v_double);
|
|
}
|
|
|
|
static void
|
|
clutter_value_transform_float_fixed (const GValue *src,
|
|
GValue *dest)
|
|
{
|
|
dest->data[0].v_int = CLUTTER_FLOAT_TO_FIXED (src->data[0].v_float);
|
|
}
|
|
|
|
|
|
static const GTypeValueTable _clutter_fixed_value_table = {
|
|
clutter_value_init_fixed,
|
|
NULL,
|
|
clutter_value_copy_fixed,
|
|
NULL,
|
|
"i",
|
|
clutter_value_collect_fixed,
|
|
"p",
|
|
clutter_value_lcopy_fixed
|
|
};
|
|
|
|
GType
|
|
clutter_fixed_get_type (void)
|
|
{
|
|
static GType _clutter_fixed_type = 0;
|
|
|
|
if (G_UNLIKELY (_clutter_fixed_type == 0))
|
|
{
|
|
_info.value_table = & _clutter_fixed_value_table;
|
|
_clutter_fixed_type =
|
|
g_type_register_fundamental (g_type_fundamental_next (),
|
|
I_("ClutterFixed"),
|
|
&_info, &_finfo, 0);
|
|
|
|
g_value_register_transform_func (_clutter_fixed_type, G_TYPE_INT,
|
|
clutter_value_transform_fixed_int);
|
|
g_value_register_transform_func (G_TYPE_INT, _clutter_fixed_type,
|
|
clutter_value_transform_int_fixed);
|
|
g_value_register_transform_func (_clutter_fixed_type, G_TYPE_FLOAT,
|
|
clutter_value_transform_fixed_float);
|
|
g_value_register_transform_func (G_TYPE_FLOAT, _clutter_fixed_type,
|
|
clutter_value_transform_float_fixed);
|
|
g_value_register_transform_func (_clutter_fixed_type, G_TYPE_DOUBLE,
|
|
clutter_value_transform_fixed_double);
|
|
g_value_register_transform_func (G_TYPE_DOUBLE, _clutter_fixed_type,
|
|
clutter_value_transform_double_fixed);
|
|
}
|
|
|
|
return _clutter_fixed_type;
|
|
}
|
|
|
|
/**
|
|
* clutter_value_set_fixed:
|
|
* @value: a #GValue initialized to #CLUTTER_TYPE_FIXED
|
|
* @fixed_: the fixed point value to set
|
|
*
|
|
* Sets @value to @fixed_.
|
|
*
|
|
* Since: 0.8
|
|
*/
|
|
void
|
|
clutter_value_set_fixed (GValue *value,
|
|
ClutterFixed fixed_)
|
|
{
|
|
g_return_if_fail (CLUTTER_VALUE_HOLDS_FIXED (value));
|
|
|
|
value->data[0].v_int = fixed_;
|
|
}
|
|
|
|
/**
|
|
* clutter_value_get_fixed:
|
|
* @value: a #GValue initialized to #CLUTTER_TYPE_FIXED
|
|
*
|
|
* Gets the fixed point value stored inside @value.
|
|
*
|
|
* Return value: the value inside the passed #GValue
|
|
*
|
|
* Since: 0.8
|
|
*/
|
|
ClutterFixed
|
|
clutter_value_get_fixed (const GValue *value)
|
|
{
|
|
g_return_val_if_fail (CLUTTER_VALUE_HOLDS_FIXED (value), 0);
|
|
|
|
return value->data[0].v_int;
|
|
}
|
|
|
|
static void
|
|
param_fixed_init (GParamSpec *pspec)
|
|
{
|
|
ClutterParamSpecFixed *fspec = CLUTTER_PARAM_SPEC_FIXED (pspec);
|
|
|
|
fspec->minimum = CLUTTER_MINFIXED;
|
|
fspec->maximum = CLUTTER_MAXFIXED;
|
|
fspec->default_value = 0;
|
|
}
|
|
|
|
static void
|
|
param_fixed_set_default (GParamSpec *pspec,
|
|
GValue *value)
|
|
{
|
|
value->data[0].v_int = CLUTTER_PARAM_SPEC_FIXED (pspec)->default_value;
|
|
}
|
|
|
|
static gboolean
|
|
param_fixed_validate (GParamSpec *pspec,
|
|
GValue *value)
|
|
{
|
|
ClutterParamSpecFixed *fspec = CLUTTER_PARAM_SPEC_FIXED (pspec);
|
|
gint oval = CLUTTER_FIXED_TO_INT (value->data[0].v_int);
|
|
gint min, max, val;
|
|
|
|
g_assert (CLUTTER_IS_PARAM_SPEC_FIXED (pspec));
|
|
|
|
/* we compare the integer part of the value because the minimum
|
|
* and maximum values cover just that part of the representation
|
|
*/
|
|
|
|
min = fspec->minimum;
|
|
max = fspec->maximum;
|
|
val = CLUTTER_FIXED_TO_INT (value->data[0].v_int);
|
|
|
|
val = CLAMP (val, min, max);
|
|
if (val != oval)
|
|
{
|
|
value->data[0].v_int = val;
|
|
return TRUE;
|
|
}
|
|
|
|
return FALSE;
|
|
}
|
|
|
|
static gint
|
|
param_fixed_values_cmp (GParamSpec *pspec,
|
|
const GValue *value1,
|
|
const GValue *value2)
|
|
{
|
|
if (value1->data[0].v_int < value2->data[0].v_int)
|
|
return -1;
|
|
else
|
|
return value1->data[0].v_int > value2->data[0].v_int;
|
|
}
|
|
|
|
GType
|
|
clutter_param_fixed_get_type (void)
|
|
{
|
|
static GType pspec_type = 0;
|
|
|
|
if (G_UNLIKELY (pspec_type == 0))
|
|
{
|
|
const GParamSpecTypeInfo pspec_info = {
|
|
sizeof (ClutterParamSpecFixed),
|
|
16,
|
|
param_fixed_init,
|
|
CLUTTER_TYPE_FIXED,
|
|
NULL,
|
|
param_fixed_set_default,
|
|
param_fixed_validate,
|
|
param_fixed_values_cmp,
|
|
};
|
|
|
|
pspec_type = g_param_type_register_static (I_("ClutterParamSpecFixed"),
|
|
&pspec_info);
|
|
}
|
|
|
|
return pspec_type;
|
|
}
|
|
|
|
/**
|
|
* clutter_param_spec_fixed:
|
|
* @name: name of the property
|
|
* @nick: short name
|
|
* @blurb: description (can be translatable)
|
|
* @minimum: lower boundary
|
|
* @maximum: higher boundary
|
|
* @default_value: default value
|
|
* @flags: flags for the param spec
|
|
*
|
|
* Creates a #GParamSpec for properties using #ClutterFixed values
|
|
*
|
|
* Return value: the newly created #GParamSpec
|
|
*
|
|
* Since: 0.8
|
|
*/
|
|
GParamSpec *
|
|
clutter_param_spec_fixed (const gchar *name,
|
|
const gchar *nick,
|
|
const gchar *blurb,
|
|
ClutterUnit minimum,
|
|
ClutterUnit maximum,
|
|
ClutterUnit default_value,
|
|
GParamFlags flags)
|
|
{
|
|
ClutterParamSpecFixed *fspec;
|
|
|
|
g_return_val_if_fail (default_value >= minimum && default_value <= maximum,
|
|
NULL);
|
|
|
|
fspec = g_param_spec_internal (CLUTTER_TYPE_PARAM_FIXED,
|
|
name, nick, blurb,
|
|
flags);
|
|
fspec->minimum = minimum;
|
|
fspec->maximum = maximum;
|
|
fspec->default_value = default_value;
|
|
|
|
return G_PARAM_SPEC (fspec);
|
|
}
|