From cfd27ef2ad8b005fd47ab41ef29b71d9e3d48201 Mon Sep 17 00:00:00 2001 From: =?UTF-8?q?J=C3=B6rg=20Frings-F=C3=BCrst?= Date: Thu, 8 Oct 2015 12:32:49 +0200 Subject: Imported Upstream version 1.0.25 --- include/sane/config.h.in | 12 +- include/sane/sanei_ir.h | 393 +++++++++++++++++++++++++++++++++++++++++++++++ 2 files changed, 399 insertions(+), 6 deletions(-) create mode 100644 include/sane/sanei_ir.h (limited to 'include/sane') diff --git a/include/sane/config.h.in b/include/sane/config.h.in index c62938b..ace060c 100644 --- a/include/sane/config.h.in +++ b/include/sane/config.h.in @@ -61,9 +61,6 @@ /* Define to 1 if you have the `cfmakeraw' function. */ #undef HAVE_CFMAKERAW -/* Is /usr/include/cups/cups.h available? */ -#undef HAVE_CUPS - /* Define to 1 if you have the header file. */ #undef HAVE_DDK_NTDDSCSI_H @@ -174,6 +171,9 @@ /* Define to 1 if you have the libjpeg library. */ #undef HAVE_LIBJPEG +/* Define to 1 if you have the libpng library. */ +#undef HAVE_LIBPNG + /* Define to 1 if you have the net-snmp library. */ #undef HAVE_LIBSNMP @@ -454,9 +454,6 @@ */ #undef LT_OBJDIR -/* Define to 1 if your C compiler doesn't accept -c and -o together. */ -#undef NO_MINUS_C_MINUS_O - /* Define to the name of the distribution. */ #undef PACKAGE @@ -490,6 +487,9 @@ /* SANE DLL minor number */ #undef SANE_DLL_V_MINOR +/* Define to 1 if you have the providing inb,outb. */ +#undef SANE_HAVE_SYS_IO_H_WITH_INB_OUTB + /* SCSI command buffer size */ #undef SCSIBUFFERSIZE diff --git a/include/sane/sanei_ir.h b/include/sane/sanei_ir.h new file mode 100644 index 0000000..aaca524 --- /dev/null +++ b/include/sane/sanei_ir.h @@ -0,0 +1,393 @@ +/** @file sanei_ir.h + * + * This file provides an interface to the + * sanei_ir functions for utilizing the infrared plane + * + * Copyright (C) 2012 Michael Rickmann + * + * This file is part of the SANE package. + * + * Essentially three things have to be done: + * - 1) reduce red spectral overlap from the infrared (ired) plane + * - 2) find the dirt + * - 3) replace the dirt + * + * - 1) is mainly adressed by sanei_ir_spectral_clean + * - 2) by sanei_ir_filter_madmean + * - 3) by sanei_ir_dilate_mean + */ + + +#ifndef SANEI_IR_H +#define SANEI_IR_H + +#include + +#define SAMPLE_SIZE 40000 /**< maximal for random sampling */ + +#define HISTOGRAM_SHIFT 8 /**< standard histogram size */ +#define HISTOGRAM_SIZE (1 << HISTOGRAM_SHIFT) + +#define SAFE_LOG(x) ( ((x) > 0.0) ? log ((x)) : (0.0) ) /**< define log (0) = 0 */ + +#define MAD_WIN2_SIZE(x) ( (((x) * 4) / 3) | 1 ) /**< MAD filter: 2nd window size */ + +typedef uint16_t SANE_Uint; + +/** + * @brief Pointer to access values of different bit depths + */ +typedef union +{ + uint8_t *b8; /**< <= 8 bits */ + uint16_t *b16; /**< > 8, <= 16 bits */ +} +SANEI_IR_bufptr; + + +/** Initialize sanei_ir. + * + * Call this before any other sanei_ir function. + */ +extern void sanei_ir_init (void); + +/** + * @brief Create the normalized histogram of a grayscale image + * + * @param[in] params describes image + * @param[in] img_data image pointer { grayscale } + * @param[out] histogram an array of double with histogram + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * @note + * histogram has to be freed by calling routine + */ +extern SANE_Status +sanei_ir_create_norm_histogram (const SANE_Parameters * params, + const SANE_Uint *img_data, + double ** histogram); + +/** + * @brief Implements Yen's thresholding method + * + * @param[in] params describes image + * @param[in] norm_histo points to a normalized histogram + * @param[out] thresh found threshold + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * -# Yen J.C., Chang F.J., and Chang S. (1995) "A New Criterion + * for Automatic Multilevel Thresholding" IEEE Trans. on Image + * Processing, 4(3): 370-378 + * -# Sezgin M. and Sankur B. (2004) "Survey over Image Thresholding + * Techniques and Quantitative Performance Evaluation" Journal of + * Electronic Imaging, 13(1): 146-165 + * -# M. Emre Celebi, 06.15.2007, fourier_0.8, + * http://sourceforge.net/projects/fourier-ipal/ + * -# ImageJ Multithresholder plugin, + * http://rsbweb.nih.gov/ij/plugins/download/AutoThresholder.java + */ +extern SANE_Status +sanei_ir_threshold_yen (const SANE_Parameters * params, + double * norm_histo, int *thresh); + +/** + * @brief Implements Otsu's thresholding method + * + * @param[in] params describes image + * @param[in] norm_histo points to a normalized histogram + * @param[out] thresh found threshold + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * -# Otsu N. (1979) "A Threshold Selection Method from Gray Level Histograms" + * IEEE Trans. on Systems, Man and Cybernetics, 9(1): 62-66 + * -# M. Emre Celebi, 06.15.2007, fourier_0.8 + * http://sourceforge.net/projects/fourier-ipal/ + */ +extern SANE_Status +sanei_ir_threshold_otsu (const SANE_Parameters * params, + double * norm_histo, int *thresh); + +/** + * @brief Implements a Maximum Entropy thresholding method + * + * @param[in] params describes image + * @param[in] norm_histo points to a normalized histogram + * @param[out] thresh found threshold + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * -# Kapur J.N., Sahoo P.K., and Wong A.K.C. (1985) "A New Method for + * Gray-Level Picture Thresholding Using the Entropy of the Histogram" + * Graphical Models and Image Processing, 29(3): 273-285 + * -# M. Emre Celebi, 06.15.2007, fourier_0.8 + * http://sourceforge.net/projects/fourier-ipal/ + * -# ImageJ Multithresholder plugin, + * http://rsbweb.nih.gov/ij/plugins/download/AutoThresholder.java + */ +extern SANE_Status +sanei_ir_threshold_maxentropy (const SANE_Parameters * params, + double * norm_histo, int *thresh); + +/** + * @brief Generate gray scale luminance image from separate R, G, B images + * + * @param params points to image description + * @param[in] in_img pointer to at least 3 planes of image data + * @param[out] out_img newly allocated image + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * - SANE_STATUS_UNSUPPORTED - wrong input bit depth + * + * @note out_img has to be freed by the calling routine. + * @note on input params describe a single color plane, + * on output params are updated if image depth is scaled + */ +SANE_Status +sanei_ir_RGB_luminance (SANE_Parameters * params, const SANE_Uint **in_img, + SANE_Uint **out_img); + +/** + * @brief Convert image from >8 bit depth to an 8 bit image. + * + * @param[in] params pimage description + * @param[in] in_img points to input image data + * @param[out] out_params if != NULL + * receives description of new image + * @param[out] out_img newly allocated 8-bit image + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * - SANE_STATUS_UNSUPPORTED - wrong input bit depth + * + * @note + * out_img has to be freed by the calling routine, + */ + +extern SANE_Status +sanei_ir_to_8bit (SANE_Parameters * params, const SANE_Uint *in_img, + SANE_Parameters * out_params, SANE_Uint **out_img); + +/** + * @brief Allocate and initialize logarithmic lookup table + * + * @param[in] length of table, usually 1 << depth + * @param[out] lut_ln adress of pointer to allocated table + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * @note natural logarithms are provided + */ +SANE_Status sanei_ir_ln_table (int len, double **lut_ln); + +/** + * @brief Reduces red spectral overlap from an infrared image plane + * + * @param[in] params pointer to image description + * @param[in] lut_ln pointer lookup table + * if NULL it is dynamically handled + * @param[in] red_data pointer to red image plane + * @param ired_data pointer to ired image plane + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * This routine is based on the observation that the relation beween the infrared value + * ired and the red value red of an image point can be described by ired = b + a * ln (red). + * First points are randomly sampled to calculate the linear regression coefficent a. + * Then ired' = ired - a * ln (red) is calculated for each pixel. Finally, the ir' image + * is scaled between 0 and maximal value. For the logarithms a lookup table is used. + * Negative films show very little spectral overlap but positive film usually has to be + * cleaned. As we do a statistical measure of the film here dark margins and lumps of + * dirt have to be excluded. + * + * @note original ired data are replaced by the cleaned ones +*/ +extern SANE_Status +sanei_ir_spectral_clean (const SANE_Parameters * params, double *lut_ln, + const SANE_Uint *red_data, + SANE_Uint *ir_data); + +/** + * @brief Optimized mean filter + * + * @param[in] params pointer to image description + * @param[in] in_img Pointer to grey scale image data + * @param[out] out_img Pointer to grey scale image data + * @param[in] win_rows Height of filtering window, odd + * @param[in] win_cols Width of filtering window, odd + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * - SANE_STATUS_INVAL - wrong window size + * + * @note At the image margins the size of the filtering window + * is adapted. So there is no need to pad the image. + * @note Memory for the output image has to be allocated before + */ +extern SANE_Status +sanei_ir_filter_mean (const SANE_Parameters * params, + const SANE_Uint *in_img, SANE_Uint *out_img, + int win_rows, int win_cols); + + +/** + * @brief Find noise by adaptive thresholding + * + * @param[in] params pointer to image description + * @param[in] in_img pointer to grey scale image + * @param[out] out_img address of pointer to newly allocated binary image + * @param[in] win_size Size of filtering window + * @param[in] a_val Parameter, below is definetly clean + * @param[in] b_val Parameter, above is definetly noisy + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * This routine follows the concept of Crnojevic's MAD (median of the absolute deviations + * from the median) filter. The first median filter step is replaced with a mean filter. + * The dirty pixels which we wish to remove are always darker than the real signal. But + * at high resolutions the scanner may generate some noise and the ired cleaning step can + * reverse things. So a maximum filter will not do. + * The second median is replaced by a mean filter to reduce computation time. Inspite of + * these changes Crnojevic's recommendations for the choice of the parameters "a" and "b" + * are still valid when scaled to the color depth. + * + * @reco Crnojevic recommends 10 < a_val < 30 and 50 < b_val < 100 for 8 bit color depth + * + * @note a_val, b_val are scaled by the routine according to bit depth + * @note "0" in the mask output is regarded "dirty", 255 "clean" + * + * -# Crnojevic V. (2005) "Impulse Noise Filter with Adaptive Mad-Based Threshold" + * Proc. of the IEEE Int. Conf. on Image Processing, 3: 337-340 + */ +extern SANE_Status +sanei_ir_filter_madmean (const SANE_Parameters * params, + const SANE_Uint *in_img, + SANE_Uint ** out_img, int win_size, + int a_val, int b_val); + + +/** + * @brief Add dark pixels to mask from static threshold + * + * @param[in] params pointer to image description + * @param[in] in_img pointer to grey scale image + * @param mask_img pointer to binary image (0, 255) + * @param[in] threshold below which the pixel is set 0 + */ +void +sanei_ir_add_threshold (const SANE_Parameters * params, + const SANE_Uint *in_img, + SANE_Uint * mask_img, int threshold); + + +/** + * @brief Calculates minimal Manhattan distances for an image mask + * + * @param[in] params pointer to image description + * @param[in] mask_img pointer to binary image (0, 255) + * @param[out] dist_map integer pointer to map of closest distances + * @param[out] idx_map integer pointer to indices of closest pixels + * @param[in] erode == 0: closest pixel has value 0, != 0: is 255 + * + * manhattan_dist takes a mask image consisting of 0 or 255 values. Given that + * a 0 represents a dirty pixel and erode != 0, manhattan_dist will calculate the + * shortest distance to a clean (255) pixel and record which pixel that was so + * that the clean parts of the image can be dilated into the dirty ones. Thresholding + * can be done on the distance. Conversely, if erode == 0 the distance of a clean + * pixel to the closest dirty one is calculated which can be used to dilate the mask. + * + * @ref extended and C version of + * http://ostermiller.org/dilate_and_erode.html + */ +void +sanei_ir_manhattan_dist (const SANE_Parameters * params, + const SANE_Uint * mask_img, unsigned int *dist_map, + unsigned int *idx_map, unsigned int erode); + + +/** + * @brief Dilate or erode a mask image + * + * @param[in] params pointer to image description + * @param mask_img pointer to binary image (0, 255) + * @param dist_map integer pointer to map of closest distances + * @param idx_map integer pointer to indices of closest pixels + * @param[in] by number of pixels, > 0 dilate, < 0 erode + * + * @note by > 0 will enlarge the 0 valued area + */ +void +sanei_ir_dilate (const SANE_Parameters * params, SANE_Uint * mask_img, + unsigned int *dist_map, unsigned int *idx_map, int by); + +/** + * @brief Suggest cropping for dark margins of positive film + * + * @param[in] params pointer to image description + * @param[in] dist_map integer pointer to map of closest distances + * @param[in] inner crop within (!=0) or outside (==0) the image's edges + * @param[out] edges pointer to array holding top, bottom, left + * and right edges + * + * The distance map as calculated by sanei_ir_manhattan_dist contains + * distances to the next clean pixel. Dark margins are detected as dirt. + * So the first/last rows/columns tell us how to crop. This is rather + * fast if the distance map has been calculated anyhow. + */ +void +sanei_ir_find_crop (const SANE_Parameters * params, + unsigned int * dist_map, int inner, int * edges); + +/** + * @brief Dilate clean image parts into dirty ones and smooth int inner, + * + * @param[in] params pointer to image description + * @param in_img array of pointers to color planes of image + * @param[in] mask_img pointer to dirt mask image + * @param[in] dist_max threshold up to which dilation is done + * @param[in] expand the dirt mask before replacing the pixels + * @param[in] win_size size of adaptive mean filtering window + * @param[in] smooth triangular filter whole image for grain removal + * @param[in] inner find crop within or outside the image's edges + * @param[out] crop array of 4 integers, if non-NULL, top, bottom, + * left and right values for cropping are returned. + * + * @return + * - SANE_STATUS_GOOD - success + * - SANE_STATUS_NO_MEM - if out of memory + * + * The main purpose of this routine is to replace dirty pixels. + * As spin-off it obtains half of what is needed for film grain + * smoothening and most of how to crop positive film. + * To speed things up these functions are also implemented. + */ +SANE_Status +sanei_ir_dilate_mean (const SANE_Parameters * params, + SANE_Uint **in_img, + SANE_Uint *mask_img, + int dist_max, int expand, int win_size, + SANE_Bool smooth, int inner, + int *crop); + + +#endif /* not SANEI_IR_H */ -- cgit v1.2.3