2012-08-02 21:59:40 +02:00
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/*
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Copyright (c) 2012, Jan Schlicht <jan.schlicht@gmail.com>
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Permission to use, copy, modify, and/or distribute this software for any purpose
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with or without fee is hereby granted, provided that the above copyright notice
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and this permission notice appear in all copies.
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THE SOFTWARE IS PROVIDED "AS IS" AND THE AUTHOR DISCLAIMS ALL WARRANTIES WITH
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REGARD TO THIS SOFTWARE INCLUDING ALL IMPLIED WARRANTIES OF MERCHANTABILITY AND
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FITNESS. IN NO EVENT SHALL THE AUTHOR BE LIABLE FOR ANY SPECIAL, DIRECT,
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INDIRECT, OR CONSEQUENTIAL DAMAGES OR ANY DAMAGES WHATSOEVER RESULTING FROM LOSS
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OF USE, DATA OR PROFITS, WHETHER IN AN ACTION OF CONTRACT, NEGLIGENCE OR OTHER
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TORTIOUS ACTION, ARISING OUT OF OR IN CONNECTION WITH THE USE OR PERFORMANCE OF
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THIS SOFTWARE.
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*/
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package resize
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import (
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"image"
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"image/color"
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2012-09-14 23:12:05 +02:00
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"math"
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2012-08-02 21:59:40 +02:00
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)
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2012-12-11 20:18:23 +01:00
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// restrict an input float32 to the range of uint16 values
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2012-08-02 21:59:40 +02:00
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func clampToUint16(x float32) (y uint16) {
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y = uint16(x)
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if x < 0 {
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y = 0
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2012-09-14 23:12:05 +02:00
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} else if x > float32(0xfffe) {
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2012-12-10 18:56:53 +01:00
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// "else if x > float32(0xffff)" will cause overflows!
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2012-08-02 21:59:40 +02:00
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y = 0xffff
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}
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return
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}
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2012-12-11 20:18:23 +01:00
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func boolToUint(b bool) (i uint) {
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if b {
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i = 0
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} else {
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i = 1
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}
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return
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}
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// describe a resampling filter
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type filterModel struct {
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// for optimized access to image points
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converter
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// instead of blurring an image before downscaling to avoid aliasing,
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// to filter is scaled by a factor which leads to a similar effect
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factor [2]float32
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// resampling is done by convolution with a (scaled) kernel
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kernel func(float32) float32
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// temporaries used by Interpolate
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tempRow, tempCol []colorArray
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}
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func (f *filterModel) convolution1d(x float32, p []colorArray, isRow bool) colorArray {
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var k float32
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var sum float32 = 0
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c := colorArray{0.0, 0.0, 0.0, 0.0}
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2012-12-11 20:18:23 +01:00
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index := boolToUint(isRow)
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for j := range p {
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k = f.kernel((x - float32(j)) / f.factor[index])
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sum += k
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for i := range c {
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c[i] += p[j][i] * k
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}
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}
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// normalize values
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for i := range c {
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c[i] = c[i] / sum
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}
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return c
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}
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2012-09-15 20:24:14 +02:00
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func (f *filterModel) Interpolate(x, y float32) color.RGBA64 {
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xf, yf := int(x)-len(f.tempRow)/2+1, int(y)-len(f.tempCol)/2+1
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x -= float32(xf)
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y -= float32(yf)
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for i := 0; i < len(f.tempCol); i++ {
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for j := 0; j < len(f.tempRow); j++ {
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f.tempRow[j] = f.at(xf+j, yf+i)
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}
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f.tempCol[i] = f.convolution1d(x, f.tempRow, true)
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}
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2012-09-19 21:03:56 +02:00
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c := f.convolution1d(y, f.tempCol, false)
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return color.RGBA64{
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clampToUint16(c[0]),
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clampToUint16(c[1]),
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clampToUint16(c[2]),
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clampToUint16(c[3]),
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}
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2012-09-04 18:49:04 +02:00
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}
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2012-09-21 20:02:25 +02:00
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// createFilter tries to find an optimized converter for the given input image
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// and initializes all filterModel members to their defaults
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func createFilter(img image.Image, factor [2]float32, size int, kernel func(float32) float32) (f Filter) {
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sizeX := size * (int(math.Ceil(float64(factor[0]))))
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sizeY := size * (int(math.Ceil(float64(factor[1]))))
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switch img.(type) {
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default:
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f = &filterModel{
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&genericConverter{img},
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factor, kernel,
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make([]colorArray, sizeX), make([]colorArray, sizeY),
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}
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case *image.RGBA:
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f = &filterModel{
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&rgbaConverter{img.(*image.RGBA)},
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factor, kernel,
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make([]colorArray, sizeX), make([]colorArray, sizeY),
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}
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case *image.RGBA64:
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f = &filterModel{
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&rgba64Converter{img.(*image.RGBA64)},
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factor, kernel,
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make([]colorArray, sizeX), make([]colorArray, sizeY),
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}
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case *image.Gray:
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f = &filterModel{
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&grayConverter{img.(*image.Gray)},
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factor, kernel,
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make([]colorArray, sizeX), make([]colorArray, sizeY),
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}
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case *image.Gray16:
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f = &filterModel{
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&gray16Converter{img.(*image.Gray16)},
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factor, kernel,
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make([]colorArray, sizeX), make([]colorArray, sizeY),
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}
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case *image.YCbCr:
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f = &filterModel{
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&ycbcrConverter{img.(*image.YCbCr)},
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factor, kernel,
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make([]colorArray, sizeX), make([]colorArray, sizeY),
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}
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}
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return
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}
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2012-09-16 09:20:11 +02:00
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// Nearest-neighbor interpolation
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func NearestNeighbor(img image.Image, factor [2]float32) Filter {
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return createFilter(img, factor, 2, func(x float32) (y float32) {
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if x >= -0.5 && x < 0.5 {
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y = 1
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} else {
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y = 0
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}
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return
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})
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}
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2012-09-16 09:20:11 +02:00
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// Bilinear interpolation
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func Bilinear(img image.Image, factor [2]float32) Filter {
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return createFilter(img, factor, 2, func(x float32) (y float32) {
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absX := float32(math.Abs(float64(x)))
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if absX <= 1 {
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y = 1 - absX
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} else {
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y = 0
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}
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return
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})
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}
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2012-09-16 09:20:11 +02:00
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// Bicubic interpolation (with cubic hermite spline)
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func Bicubic(img image.Image, factor [2]float32) Filter {
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return createFilter(img, factor, 4, func(x float32) (y float32) {
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absX := float32(math.Abs(float64(x)))
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if absX <= 1 {
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y = absX*absX*(1.5*absX-2.5) + 1
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} else if absX <= 2 {
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y = absX*(absX*(2.5-0.5*absX)-4) + 2
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} else {
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y = 0
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}
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return
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})
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}
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2012-09-21 20:02:25 +02:00
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// Mitchell-Netravali interpolation
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func MitchellNetravali(img image.Image, factor [2]float32) Filter {
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return createFilter(img, factor, 4, func(x float32) (y float32) {
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2012-09-19 19:32:00 +02:00
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absX := float32(math.Abs(float64(x)))
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if absX <= 1 {
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y = absX*absX*(7*absX-12) + 16.0/3
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} else if absX <= 2 {
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y = -(absX - 2) * (absX - 2) / 3 * (7*absX - 8)
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2012-12-10 18:56:53 +01:00
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} else {
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y = 0
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2012-09-19 19:32:00 +02:00
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}
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return
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2012-09-19 21:03:56 +02:00
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})
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2012-09-19 19:32:00 +02:00
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}
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func lanczosKernel(a uint) func(float32) float32 {
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return func(x float32) (y float32) {
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if x > -float32(a) && x < float32(a) {
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y = float32(Sinc(float64(x))) * float32(Sinc(float64(x/float32(a))))
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} else {
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y = 0
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}
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return
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2012-09-19 19:32:00 +02:00
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}
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}
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2012-09-21 20:02:25 +02:00
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// Lanczos interpolation (a=2)
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func Lanczos2(img image.Image, factor [2]float32) Filter {
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return createFilter(img, factor, 4, lanczosKernel(2))
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}
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2012-09-21 20:02:25 +02:00
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// Lanczos interpolation (a=3)
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func Lanczos3(img image.Image, factor [2]float32) Filter {
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return createFilter(img, factor, 6, lanczosKernel(3))
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2012-08-02 21:59:40 +02:00
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}
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