C# 클래스 BitMiracle.LibJpeg.Classic.Internal.my_2pass_cquantizer

This module implements the well-known Heckbert paradigm for color quantization. Most of the ideas used here can be traced back to Heckbert's seminal paper Heckbert, Paul. "Color Image Quantization for Frame Buffer Display", Proc. SIGGRAPH '82, Computer Graphics v.16 #3 (July 1982), pp 297-304. In the first pass over the image, we accumulate a histogram showing the usage count of each possible color. To keep the histogram to a reasonable size, we reduce the precision of the input; typical practice is to retain 5 or 6 bits per color, so that 8 or 4 different input values are counted in the same histogram cell. Next, the color-selection step begins with a box representing the whole color space, and repeatedly splits the "largest" remaining box until we have as many boxes as desired colors. Then the mean color in each remaining box becomes one of the possible output colors. The second pass over the image maps each input pixel to the closest output color (optionally after applying a Floyd-Steinberg dithering correction). This mapping is logically trivial, but making it go fast enough requires considerable care. Heckbert-style quantizers vary a good deal in their policies for choosing the "largest" box and deciding where to cut it. The particular policies used here have proved out well in experimental comparisons, but better ones may yet be found. In earlier versions of the IJG code, this module quantized in YCbCr color space, processing the raw upsampled data without a color conversion step. This allowed the color conversion math to be done only once per colormap entry, not once per pixel. However, that optimization precluded other useful optimizations (such as merging color conversion with upsampling) and it also interfered with desired capabilities such as quantizing to an externally-supplied colormap. We have therefore abandoned that approach. The present code works in the post-conversion color space, typically RGB. To improve the visual quality of the results, we actually work in scaled RGB space, giving G distances more weight than R, and R in turn more than B. To do everything in integer math, we must use integer scale factors. The 2/3/1 scale factors used here correspond loosely to the relative weights of the colors in the NTSC grayscale equation. If you want to use this code to quantize a non-RGB color space, you'll probably need to change these scale factors. First we have the histogram data structure and routines for creating it. The number of bits of precision can be adjusted by changing these symbols. We recommend keeping 6 bits for G and 5 each for R and B. If you have plenty of memory and cycles, 6 bits all around gives marginally better results; if you are short of memory, 5 bits all around will save some space but degrade the results. To maintain a fully accurate histogram, we'd need to allocate a "long" (preferably unsigned long) for each cell. In practice this is overkill; we can get by with 16 bits per cell. Few of the cell counts will overflow, and clamping those that do overflow to the maximum value will give close- enough results. This reduces the recommended histogram size from 256Kb to 128Kb, which is a useful savings on PC-class machines. (In the second pass the histogram space is re-used for pixel mapping data; in that capacity, each cell must be able to store zero to the number of desired colors. 16 bits/cell is plenty for that too.) Since the JPEG code is intended to run in small memory model on 80x86 machines, we can't just allocate the histogram in one chunk. Instead of a true 3-D array, we use a row of pointers to 2-D arrays. Each pointer corresponds to a C0 value (typically 2^5 = 32 pointers) and each 2-D array has 2^6*2^5 = 2048 or 2^6*2^6 = 4096 entries. Note that on 80x86 machines, the pointer row is in near memory but the actual arrays are in far memory (same arrangement as we use for image arrays). Declarations for Floyd-Steinberg dithering. Errors are accumulated into the array fserrors[], at a resolution of 1/16th of a pixel count. The error at a given pixel is propagated to its not-yet-processed neighbors using the standard F-S fractions, ... (here) 7/16 3/16 5/16 1/16 We work left-to-right on even rows, right-to-left on odd rows. We can get away with a single array (holding one row's worth of errors) by using it to store the current row's errors at pixel columns not yet processed, but the next row's errors at columns already processed. We need only a few extra variables to hold the errors immediately around the current column. (If we are lucky, those variables are in registers, but even if not, they're probably cheaper to access than array elements are.) The fserrors[] array has (#columns + 2) entries; the extra entry at each end saves us from special-casing the first and last pixels. Each entry is three values long, one value for each color component.