Additional photo processing algorithms#
Detailed Description#
Classes#
Name |
Description |
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Gray-world white balance algorithm. View details |
More sophisticated learning-based automatic white balance algorithm. View details |
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A simple white balance algorithm that works by independently stretching each of the input image channels to the specified range. For increased robustness it ignores the top and bottom \(p\%\) of pixel values. View details |
This algorithm decomposes image into two layers: base layer and detail layer using bilateral filter and compresses contrast of the base layer thus preserving all the details. View details |
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The base class for auto white balance algorithms. View details |
Enumerations#
enum cv::xphoto::Bm3dSteps {
cv::xphoto::BM3D_STEPALL = 0,
cv::xphoto::BM3D_STEP1 = 1,
cv::xphoto::BM3D_STEP2 = 2
}BM3D algorithm steps. View details
Various inpainting algorithms. View details
enum cv::xphoto::TransformTypes {
cv::xphoto::HAAR = 0
}BM3D transform types. View details
Functions#
Return |
Name |
Description |
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Implements an efficient fixed-point approximation for applying channel gains, which is the last step of multiple white balance algorithms. |
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Performs image denoising using the Block-Matching and 3D-filtering algorithm http://www.cs.tut.fi/~foi/GCF-BM3D/BM3D_TIP_2007.pdf with several computational optimizations. Noise expected to be a gaussian white noise. |
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Performs image denoising using the Block-Matching and 3D-filtering algorithm http://www.cs.tut.fi/~foi/GCF-BM3D/BM3D_TIP_2007.pdf with several computational optimizations. Noise expected to be a gaussian white noise. |
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Creates an instance of GrayworldWB. |
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Creates an instance of LearningBasedWB. |
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Creates an instance of SimpleWB. |
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Creates TonemapDurand object. |
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The function implements simple dct-based denoising. |
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The function implements different single-image inpainting algorithms. |
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oilPainting See the book [142] for details. |
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oilPainting See the book [142] for details. |
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Enumeration Type Documentation#
Bm3dSteps#
#include <opencv2/xphoto/bm3d_image_denoising.hpp>
BM3D algorithm steps.
Enumerator:
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Execute all steps of the algorithm |
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Execute only first step of the algorithm |
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Execute only second step of the algorithm |
InpaintTypes#
#include <opencv2/xphoto/inpainting.hpp>
Various inpainting algorithms.
See also
Enumerator:
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This algorithm searches for dominant correspondences (transformations) of image patches and tries to seamlessly fill-in the area to be inpainted using this transformations |
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Performs Frequency Selective Reconstruction (FSR). One of the two quality profiles BEST and FAST can be chosen, depending on the time available for reconstruction. See [116] and [263] for details. The algorithm may be utilized for the following areas of application:
1-channel grayscale or 3-channel BGR image are accepted. Conventional accepted ranges:
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See INPAINT_FSR_BEST. |
TransformTypes#
enum cv::xphoto::TransformTypes
#include <opencv2/xphoto/bm3d_image_denoising.hpp>
BM3D transform types.
Enumerator:
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Un-normalized Haar transform |
Function Documentation#
applyChannelGains()#
void cv::xphoto::applyChannelGains(
InputArray src,
OutputArray dst,
float gainB,
float gainG,
float gainR )
#include <opencv2/xphoto/white_balance.hpp>
Python:
cv.xphoto.applyChannelGains(src, gainB, gainG, gainR[, dst]) -> dst
Implements an efficient fixed-point approximation for applying channel gains, which is the last step of multiple white balance algorithms.
Parameters
src— Input three-channel image in the BGR color space (either CV_8UC3 or CV_16UC3)dst— Output image of the same size and type as src.gainB— gain for the B channelgainG— gain for the G channelgainR— gain for the R channel
bm3dDenoising()#
void cv::xphoto::bm3dDenoising(
InputArray src,
InputOutputArray dstStep1,
OutputArray dstStep2,
float h = 1,
int templateWindowSize = 4,
int searchWindowSize = 16,
int blockMatchingStep1 = 2500,
int blockMatchingStep2 = 400,
int groupSize = 8,
int slidingStep = 1,
float beta = 2.0f,
int normType = cv::NORM_L2,
int step = cv::xphoto::BM3D_STEPALL,
int transformType = cv::xphoto::HAAR )
#include <opencv2/xphoto/bm3d_image_denoising.hpp>
Python:
cv.xphoto.bm3dDenoising(src, dstStep1[, dstStep2[, h[, templateWindowSize[, searchWindowSize[, blockMatchingStep1[, blockMatchingStep2[, groupSize[, slidingStep[, beta[, normType[, step[, transformType]]]]]]]]]]]]) -> dstStep1, dstStep2
cv.xphoto.bm3dDenoising(src[, dst[, h[, templateWindowSize[, searchWindowSize[, blockMatchingStep1[, blockMatchingStep2[, groupSize[, slidingStep[, beta[, normType[, step[, transformType]]]]]]]]]]]]) -> dst
Performs image denoising using the Block-Matching and 3D-filtering algorithm http://www.cs.tut.fi/~foi/GCF-BM3D/BM3D_TIP_2007.pdf with several computational optimizations. Noise expected to be a gaussian white noise.
This function expected to be applied to grayscale images. Advanced usage of this function can be manual denoising of colored image in different colorspaces.
See also
Parameters
src— Input 8-bit or 16-bit 1-channel image.dstStep1— Output image of the first step of BM3D with the same size and type as src.dstStep2— Output image of the second step of BM3D with the same size and type as src.h— Parameter regulating filter strength. Big h value perfectly removes noise but also removes image details, smaller h value preserves details but also preserves some noise.templateWindowSize— Size in pixels of the template patch that is used for block-matching. Should be power of 2.searchWindowSize— Size in pixels of the window that is used to perform block-matching. Affect performance linearly: greater searchWindowsSize - greater denoising time. Must be larger than templateWindowSize.blockMatchingStep1— Block matching threshold for the first step of BM3D (hard thresholding), i.e. maximum distance for which two blocks are considered similar. Value expressed in euclidean distance.blockMatchingStep2— Block matching threshold for the second step of BM3D (Wiener filtering), i.e. maximum distance for which two blocks are considered similar. Value expressed in euclidean distance.groupSize— Maximum size of the 3D group for collaborative filtering.slidingStep— Sliding step to process every next reference block.beta— Kaiser window parameter that affects the sidelobe attenuation of the transform of the window. Kaiser window is used in order to reduce border effects. To prevent usage of the window, set beta to zero.normType— Norm used to calculate distance between blocks. L2 is slower than L1 but yields more accurate results.step— Step of BM3D to be executed. Possible variants are: step 1, step 2, both steps.transformType— Type of the orthogonal transform used in collaborative filtering step. Currently only Haar transform is supported.
bm3dDenoising()#
void cv::xphoto::bm3dDenoising(
InputArray src,
OutputArray dst,
float h = 1,
int templateWindowSize = 4,
int searchWindowSize = 16,
int blockMatchingStep1 = 2500,
int blockMatchingStep2 = 400,
int groupSize = 8,
int slidingStep = 1,
float beta = 2.0f,
int normType = cv::NORM_L2,
int step = cv::xphoto::BM3D_STEPALL,
int transformType = cv::xphoto::HAAR )
#include <opencv2/xphoto/bm3d_image_denoising.hpp>
Python:
cv.xphoto.bm3dDenoising(src, dstStep1[, dstStep2[, h[, templateWindowSize[, searchWindowSize[, blockMatchingStep1[, blockMatchingStep2[, groupSize[, slidingStep[, beta[, normType[, step[, transformType]]]]]]]]]]]]) -> dstStep1, dstStep2
cv.xphoto.bm3dDenoising(src[, dst[, h[, templateWindowSize[, searchWindowSize[, blockMatchingStep1[, blockMatchingStep2[, groupSize[, slidingStep[, beta[, normType[, step[, transformType]]]]]]]]]]]]) -> dst
Performs image denoising using the Block-Matching and 3D-filtering algorithm http://www.cs.tut.fi/~foi/GCF-BM3D/BM3D_TIP_2007.pdf with several computational optimizations. Noise expected to be a gaussian white noise.
This function expected to be applied to grayscale images. Advanced usage of this function can be manual denoising of colored image in different colorspaces.
See also
Parameters
src— Input 8-bit or 16-bit 1-channel image.dst— Output image with the same size and type as src.h— Parameter regulating filter strength. Big h value perfectly removes noise but also removes image details, smaller h value preserves details but also preserves some noise.templateWindowSize— Size in pixels of the template patch that is used for block-matching. Should be power of 2.searchWindowSize— Size in pixels of the window that is used to perform block-matching. Affect performance linearly: greater searchWindowsSize - greater denoising time. Must be larger than templateWindowSize.blockMatchingStep1— Block matching threshold for the first step of BM3D (hard thresholding), i.e. maximum distance for which two blocks are considered similar. Value expressed in euclidean distance.blockMatchingStep2— Block matching threshold for the second step of BM3D (Wiener filtering), i.e. maximum distance for which two blocks are considered similar. Value expressed in euclidean distance.groupSize— Maximum size of the 3D group for collaborative filtering.slidingStep— Sliding step to process every next reference block.beta— Kaiser window parameter that affects the sidelobe attenuation of the transform of the window. Kaiser window is used in order to reduce border effects. To prevent usage of the window, set beta to zero.normType— Norm used to calculate distance between blocks. L2 is slower than L1 but yields more accurate results.step— Step of BM3D to be executed. Allowed are only BM3D_STEP1 and BM3D_STEPALL. BM3D_STEP2 is not allowed as it requires basic estimate to be present.transformType— Type of the orthogonal transform used in collaborative filtering step. Currently only Haar transform is supported.
createGrayworldWB()#
Ptr< GrayworldWB > cv::xphoto::createGrayworldWB()
#include <opencv2/xphoto/white_balance.hpp>
Python:
cv.xphoto.createGrayworldWB() -> retval
Creates an instance of GrayworldWB.
createLearningBasedWB()#
Ptr< LearningBasedWB > cv::xphoto::createLearningBasedWB(const String & path_to_model = String())
#include <opencv2/xphoto/white_balance.hpp>
Python:
cv.xphoto.createLearningBasedWB([, path_to_model]) -> retval
Creates an instance of LearningBasedWB.
Parameters
path_to_model— Path to a .yml file with the model. If not specified, the default model is used
createSimpleWB()#
Ptr< SimpleWB > cv::xphoto::createSimpleWB()
#include <opencv2/xphoto/white_balance.hpp>
Python:
cv.xphoto.createSimpleWB() -> retval
Creates an instance of SimpleWB.
createTonemapDurand()#
Ptr< TonemapDurand > cv::xphoto::createTonemapDurand(
float gamma = 1.0f,
float contrast = 4.0f,
float saturation = 1.0f,
float sigma_color = 2.0f,
float sigma_space = 2.0f )
#include <opencv2/xphoto/tonemap.hpp>
Python:
cv.xphoto.createTonemapDurand([, gamma[, contrast[, saturation[, sigma_color[, sigma_space]]]]]) -> retval
Creates TonemapDurand object.
You need to set the OPENCV_ENABLE_NONFREE option in cmake to use those. Use them at your own risk.
Parameters
gamma— gamma value for gamma correction. See createTonemapcontrast— resulting contrast on logarithmic scale, i. e. log(max / min), where max and min are maximum and minimum luminance values of the resulting image.saturation— saturation enhancement value. See createTonemapDragosigma_color— bilateral filter sigma in color spacesigma_space— bilateral filter sigma in coordinate space
dctDenoising()#
void cv::xphoto::dctDenoising(
const Mat & src,
Mat & dst,
const double sigma,
const int psize = 16 )
#include <opencv2/xphoto/dct_image_denoising.hpp>
Python:
cv.xphoto.dctDenoising(src, dst, sigma[, psize])
The function implements simple dct-based denoising.
http://www.ipol.im/pub/art/2011/ys-dct/.
See also
Parameters
src— source imagedst— destination imagesigma— expected noise standard deviationpsize— size of block side where dct is computed
inpaint()#
void cv::xphoto::inpaint(
const Mat & src,
const Mat & mask,
Mat & dst,
const int algorithmType )
#include <opencv2/xphoto/inpainting.hpp>
Python:
cv.xphoto.inpaint(src, mask, dst, algorithmType)
The function implements different single-image inpainting algorithms.
See the original papers [135] (Shiftmap) or [116] and [263] (FSR) for details.
Parameters
src— source imageINPAINT_SHIFTMAP: it could be of any type and any number of channels from 1 to 4. In case of 3- and 4-channels images the function expect them in CIELab colorspace or similar one, where first color component shows intensity, while second and third shows colors. Nonetheless you can try any colorspaces.
INPAINT_FSR_BEST or INPAINT_FSR_FAST: 1-channel grayscale or 3-channel BGR image.
mask— mask (CV_8UC1), where non-zero pixels indicate valid image area, while zero pixels indicate area to be inpainteddst— destination imagealgorithmType— see xphoto::InpaintTypes
oilPainting()#
void cv::xphoto::oilPainting(
InputArray src,
OutputArray dst,
int size,
int dynRatio )
#include <opencv2/xphoto/oilpainting.hpp>
Python:
cv.xphoto.oilPainting(src, size, dynRatio, code[, dst]) -> dst
cv.xphoto.oilPainting(src, size, dynRatio[, dst]) -> dst
oilPainting See the book [142] for details.
Parameters
src— Input three-channel or one channel image (either CV_8UC3 or CV_8UC1)dst— Output image of the same size and type as src.size— neighbouring size is 2-size+1dynRatio— image is divided by dynRatio before histogram processing
oilPainting()#
void cv::xphoto::oilPainting(
InputArray src,
OutputArray dst,
int size,
int dynRatio,
int code )
#include <opencv2/xphoto/oilpainting.hpp>
Python:
cv.xphoto.oilPainting(src, size, dynRatio, code[, dst]) -> dst
cv.xphoto.oilPainting(src, size, dynRatio[, dst]) -> dst
oilPainting See the book [142] for details.
Parameters
src— Input three-channel or one channel image (either CV_8UC3 or CV_8UC1)dst— Output image of the same size and type as src.size— neighbouring size is 2-size+1dynRatio— image is divided by dynRatio before histogram processingcode— color space conversion code(see ColorConversionCodes). Histogram will used only first plane