|
|
|
// -*- C++;indent-tabs-mode: t; tab-width: 4; c-basic-offset: 4; -*-
|
|
|
|
|
|
|
|
/**
|
|
|
|
* KImageIO Routines to read (and perhaps in the future, write) images
|
|
|
|
* in the high dynamic range EXR format.
|
|
|
|
* Copyright (c) 2003, Brad Hards <bradh@frogmouth.net>
|
|
|
|
*
|
|
|
|
* This library is distributed under the conditions of the GNU LGPL.
|
|
|
|
*
|
|
|
|
* $Id$
|
|
|
|
*/
|
|
|
|
|
|
|
|
#include "config.h"
|
|
|
|
|
|
|
|
#ifdef HAVE_EXR
|
|
|
|
|
|
|
|
#include <ImfRgbaFile.h>
|
|
|
|
#include <ImfStandardAttributes.h>
|
|
|
|
#include <ImathBox.h>
|
|
|
|
#include <ImfInputFile.h>
|
|
|
|
#include <ImfBoxAttribute.h>
|
|
|
|
#include <ImfChannelListAttribute.h>
|
|
|
|
#include <ImfCompressionAttribute.h>
|
|
|
|
#include <ImfFloatAttribute.h>
|
|
|
|
#include <ImfIntAttribute.h>
|
|
|
|
#include <ImfLineOrderAttribute.h>
|
|
|
|
#include <ImfStringAttribute.h>
|
|
|
|
#include <ImfVecAttribute.h>
|
|
|
|
#include <ImfArray.h>
|
|
|
|
#include <ImfConvert.h>
|
|
|
|
|
|
|
|
#include <iostream>
|
|
|
|
|
|
|
|
#include <stdlib.h>
|
|
|
|
|
|
|
|
#include <kurl.h>
|
|
|
|
#include <kprocess.h>
|
|
|
|
#include <klocale.h>
|
|
|
|
#include <kgenericfactory.h>
|
|
|
|
#include <kdebug.h>
|
|
|
|
|
|
|
|
#include <tqimage.h>
|
|
|
|
#include <tqcstring.h>
|
|
|
|
#include <tqfile.h>
|
|
|
|
#include <tqdatetime.h>
|
|
|
|
#include <tqdict.h>
|
|
|
|
#include <tqvalidator.h>
|
|
|
|
#include <tqcolor.h>
|
|
|
|
|
|
|
|
#include "exr.h"
|
|
|
|
|
|
|
|
using namespace Imf;
|
|
|
|
|
|
|
|
/* this does a conversion from the ILM Half (equal to Nvidia Half)
|
|
|
|
* format into the normal 32 bit pixel format. Process is from the
|
|
|
|
* ILM code.
|
|
|
|
*/
|
|
|
|
QRgb RgbaToQrgba(struct Rgba imagePixel)
|
|
|
|
{
|
|
|
|
float r,g,b,a;
|
|
|
|
|
|
|
|
// 1) Compensate for fogging by subtracting defog
|
|
|
|
// from the raw pixel values.
|
|
|
|
// Response: We work with defog of 0.0, so this is a no-op
|
|
|
|
|
|
|
|
// 2) Multiply the defogged pixel values by
|
|
|
|
// 2^(exposure + 2.47393).
|
|
|
|
// Response: We work with exposure of 0.0.
|
|
|
|
// (2^2.47393) is 5.55555
|
|
|
|
r = imagePixel.r * 5.55555;
|
|
|
|
g = imagePixel.g * 5.55555;
|
|
|
|
b = imagePixel.b * 5.55555;
|
|
|
|
a = imagePixel.a * 5.55555;
|
|
|
|
|
|
|
|
// 3) Values, which are now 1.0, are called "middle gray".
|
|
|
|
// If defog and exposure are both set to 0.0, then
|
|
|
|
// middle gray corresponds to a raw pixel value of 0.18.
|
|
|
|
// In step 6, middle gray values will be mapped to an
|
|
|
|
// intensity 3.5 f-stops below the display's maximum
|
|
|
|
// intensity.
|
|
|
|
// Response: no apparent content.
|
|
|
|
|
|
|
|
// 4) Apply a knee function. The knee function has two
|
|
|
|
// parameters, kneeLow and kneeHigh. Pixel values
|
|
|
|
// below 2^kneeLow are not changed by the knee
|
|
|
|
// function. Pixel values above kneeLow are lowered
|
|
|
|
// according to a logarithmic curve, such that the
|
|
|
|
// value 2^kneeHigh is mapped to 2^3.5 (in step 6,
|
|
|
|
// this value will be mapped to the the display's
|
|
|
|
// maximum intensity).
|
|
|
|
// Response: kneeLow = 0.0 (2^0.0 => 1); kneeHigh = 5.0 (2^5 =>32)
|
|
|
|
if (r > 1.0)
|
|
|
|
r = 1.0 + Imath::Math<float>::log ((r-1.0) * 0.184874 + 1) / 0.184874;
|
|
|
|
if (g > 1.0)
|
|
|
|
g = 1.0 + Imath::Math<float>::log ((g-1.0) * 0.184874 + 1) / 0.184874;
|
|
|
|
if (b > 1.0)
|
|
|
|
b = 1.0 + Imath::Math<float>::log ((b-1.0) * 0.184874 + 1) / 0.184874;
|
|
|
|
if (a > 1.0)
|
|
|
|
a = 1.0 + Imath::Math<float>::log ((a-1.0) * 0.184874 + 1) / 0.184874;
|
|
|
|
//
|
|
|
|
// 5) Gamma-correct the pixel values, assuming that the
|
|
|
|
// screen's gamma is 0.4545 (or 1/2.2).
|
|
|
|
r = Imath::Math<float>::pow (r, 0.4545);
|
|
|
|
g = Imath::Math<float>::pow (g, 0.4545);
|
|
|
|
b = Imath::Math<float>::pow (b, 0.4545);
|
|
|
|
a = Imath::Math<float>::pow (a, 0.4545);
|
|
|
|
|
|
|
|
// 6) Scale the values such that pixels middle gray
|
|
|
|
// pixels are mapped to 84.66 (or 3.5 f-stops below
|
|
|
|
// the display's maximum intensity).
|
|
|
|
//
|
|
|
|
// 7) Clamp the values to [0, 255].
|
|
|
|
return tqRgba( char (Imath::clamp ( r * 84.66f, 0.f, 255.f ) ),
|
|
|
|
char (Imath::clamp ( g * 84.66f, 0.f, 255.f ) ),
|
|
|
|
char (Imath::clamp ( b * 84.66f, 0.f, 255.f ) ),
|
|
|
|
char (Imath::clamp ( a * 84.66f, 0.f, 255.f ) ) );
|
|
|
|
}
|
|
|
|
|
|
|
|
KDE_EXPORT void kimgio_exr_read( TQImageIO *io )
|
|
|
|
{
|
|
|
|
try
|
|
|
|
{
|
|
|
|
int width, height;
|
|
|
|
|
|
|
|
// This won't work if io is not TQFile !
|
|
|
|
RgbaInputFile file (TQFile::encodeName(io->fileName()));
|
|
|
|
Imath::Box2i dw = file.dataWindow();
|
|
|
|
|
|
|
|
width = dw.max.x - dw.min.x + 1;
|
|
|
|
height = dw.max.y - dw.min.y + 1;
|
|
|
|
|
|
|
|
Array2D<Rgba> pixels;
|
|
|
|
pixels.resizeErase (height, width);
|
|
|
|
|
|
|
|
file.setFrameBuffer (&pixels[0][0] - dw.min.x - dw.min.y * width, 1, width);
|
|
|
|
file.readPixels (dw.min.y, dw.max.y);
|
|
|
|
|
|
|
|
TQImage image(width, height, 32, 0, TQImage::BigEndian);
|
|
|
|
if( image.isNull())
|
|
|
|
return;
|
|
|
|
|
|
|
|
// somehow copy pixels into image
|
|
|
|
for ( int y=0; y < height; y++ ) {
|
|
|
|
for ( int x=0; x < width; x++ ) {
|
|
|
|
// copy pixels(x,y) into image(x,y)
|
|
|
|
image.setPixel( x, y, RgbaToQrgba( pixels[y][x] ) );
|
|
|
|
}
|
|
|
|
}
|
|
|
|
|
|
|
|
io->setImage( image );
|
|
|
|
io->seStatus( 0 );
|
|
|
|
}
|
|
|
|
catch (const std::exception &exc)
|
|
|
|
{
|
|
|
|
kdDebug(399) << exc.what() << endl;
|
|
|
|
return;
|
|
|
|
}
|
|
|
|
}
|
|
|
|
|
|
|
|
|
|
|
|
KDE_EXPORT void kimgio_exr_write(TQImageIO *)
|
|
|
|
{
|
|
|
|
// TODO: stub
|
|
|
|
}
|
|
|
|
|
|
|
|
|
|
|
|
#endif
|