2016-04-28 21:40:36 +02:00
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/*M///////////////////////////////////////////////////////////////////////////////////////
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//
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// IMPORTANT: READ BEFORE DOWNLOADING, COPYING, INSTALLING OR USING.
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// By downloading, copying, installing or using the software you agree to this license.
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// copy or use the software.
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//
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// License Agreement
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// For Open Source Computer Vision Library
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// Copyright (C) 2000-2008, Intel Corporation, all rights reserved.
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// Copyright (C) 2009, Willow Garage Inc., all rights reserved.
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// Copyright (C) 2013, OpenCV Foundation, all rights reserved.
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//M*/
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2018-02-01 21:10:10 +01:00
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#ifndef OPENCV_TRACKING_HPP
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#define OPENCV_TRACKING_HPP
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2016-04-28 21:40:36 +02:00
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#include "opencv2/core.hpp"
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#include "opencv2/imgproc.hpp"
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namespace cv
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{
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//! @addtogroup video_track
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//! @{
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enum { OPTFLOW_USE_INITIAL_FLOW = 4,
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OPTFLOW_LK_GET_MIN_EIGENVALS = 8,
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OPTFLOW_FARNEBACK_GAUSSIAN = 256
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};
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/** @brief Finds an object center, size, and orientation.
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@param probImage Back projection of the object histogram. See calcBackProject.
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@param window Initial search window.
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@param criteria Stop criteria for the underlying meanShift.
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returns
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(in old interfaces) Number of iterations CAMSHIFT took to converge
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The function implements the CAMSHIFT object tracking algorithm @cite Bradski98 . First, it finds an
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object center using meanShift and then adjusts the window size and finds the optimal rotation. The
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function returns the rotated rectangle structure that includes the object position, size, and
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orientation. The next position of the search window can be obtained with RotatedRect::boundingRect()
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See the OpenCV sample camshiftdemo.c that tracks colored objects.
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@note
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- (Python) A sample explaining the camshift tracking algorithm can be found at
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opencv_source_code/samples/python/camshift.py
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*/
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CV_EXPORTS_W RotatedRect CamShift( InputArray probImage, CV_IN_OUT Rect& window,
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TermCriteria criteria );
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/** @example camshiftdemo.cpp
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An example using the mean-shift tracking algorithm
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*/
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2016-04-28 21:40:36 +02:00
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/** @brief Finds an object on a back projection image.
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@param probImage Back projection of the object histogram. See calcBackProject for details.
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@param window Initial search window.
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@param criteria Stop criteria for the iterative search algorithm.
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returns
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: Number of iterations CAMSHIFT took to converge.
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The function implements the iterative object search algorithm. It takes the input back projection of
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an object and the initial position. The mass center in window of the back projection image is
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computed and the search window center shifts to the mass center. The procedure is repeated until the
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specified number of iterations criteria.maxCount is done or until the window center shifts by less
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than criteria.epsilon. The algorithm is used inside CamShift and, unlike CamShift , the search
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window size or orientation do not change during the search. You can simply pass the output of
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calcBackProject to this function. But better results can be obtained if you pre-filter the back
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projection and remove the noise. For example, you can do this by retrieving connected components
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with findContours , throwing away contours with small area ( contourArea ), and rendering the
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remaining contours with drawContours.
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*/
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CV_EXPORTS_W int meanShift( InputArray probImage, CV_IN_OUT Rect& window, TermCriteria criteria );
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/** @brief Constructs the image pyramid which can be passed to calcOpticalFlowPyrLK.
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@param img 8-bit input image.
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@param pyramid output pyramid.
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@param winSize window size of optical flow algorithm. Must be not less than winSize argument of
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calcOpticalFlowPyrLK. It is needed to calculate required padding for pyramid levels.
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@param maxLevel 0-based maximal pyramid level number.
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@param withDerivatives set to precompute gradients for the every pyramid level. If pyramid is
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constructed without the gradients then calcOpticalFlowPyrLK will calculate them internally.
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@param pyrBorder the border mode for pyramid layers.
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@param derivBorder the border mode for gradients.
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@param tryReuseInputImage put ROI of input image into the pyramid if possible. You can pass false
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to force data copying.
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@return number of levels in constructed pyramid. Can be less than maxLevel.
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*/
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CV_EXPORTS_W int buildOpticalFlowPyramid( InputArray img, OutputArrayOfArrays pyramid,
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Size winSize, int maxLevel, bool withDerivatives = true,
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int pyrBorder = BORDER_REFLECT_101,
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int derivBorder = BORDER_CONSTANT,
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bool tryReuseInputImage = true );
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2018-02-01 21:10:10 +01:00
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/** @example lkdemo.cpp
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An example using the Lucas-Kanade optical flow algorithm
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*/
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/** @brief Calculates an optical flow for a sparse feature set using the iterative Lucas-Kanade method with
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pyramids.
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@param prevImg first 8-bit input image or pyramid constructed by buildOpticalFlowPyramid.
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@param nextImg second input image or pyramid of the same size and the same type as prevImg.
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@param prevPts vector of 2D points for which the flow needs to be found; point coordinates must be
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single-precision floating-point numbers.
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@param nextPts output vector of 2D points (with single-precision floating-point coordinates)
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containing the calculated new positions of input features in the second image; when
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OPTFLOW_USE_INITIAL_FLOW flag is passed, the vector must have the same size as in the input.
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@param status output status vector (of unsigned chars); each element of the vector is set to 1 if
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the flow for the corresponding features has been found, otherwise, it is set to 0.
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@param err output vector of errors; each element of the vector is set to an error for the
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corresponding feature, type of the error measure can be set in flags parameter; if the flow wasn't
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found then the error is not defined (use the status parameter to find such cases).
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@param winSize size of the search window at each pyramid level.
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@param maxLevel 0-based maximal pyramid level number; if set to 0, pyramids are not used (single
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level), if set to 1, two levels are used, and so on; if pyramids are passed to input then
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algorithm will use as many levels as pyramids have but no more than maxLevel.
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@param criteria parameter, specifying the termination criteria of the iterative search algorithm
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(after the specified maximum number of iterations criteria.maxCount or when the search window
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moves by less than criteria.epsilon.
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@param flags operation flags:
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- **OPTFLOW_USE_INITIAL_FLOW** uses initial estimations, stored in nextPts; if the flag is
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not set, then prevPts is copied to nextPts and is considered the initial estimate.
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- **OPTFLOW_LK_GET_MIN_EIGENVALS** use minimum eigen values as an error measure (see
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minEigThreshold description); if the flag is not set, then L1 distance between patches
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around the original and a moved point, divided by number of pixels in a window, is used as a
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error measure.
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@param minEigThreshold the algorithm calculates the minimum eigen value of a 2x2 normal matrix of
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optical flow equations (this matrix is called a spatial gradient matrix in @cite Bouguet00), divided
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by number of pixels in a window; if this value is less than minEigThreshold, then a corresponding
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feature is filtered out and its flow is not processed, so it allows to remove bad points and get a
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performance boost.
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The function implements a sparse iterative version of the Lucas-Kanade optical flow in pyramids. See
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@cite Bouguet00 . The function is parallelized with the TBB library.
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@note
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- An example using the Lucas-Kanade optical flow algorithm can be found at
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opencv_source_code/samples/cpp/lkdemo.cpp
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- (Python) An example using the Lucas-Kanade optical flow algorithm can be found at
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opencv_source_code/samples/python/lk_track.py
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- (Python) An example using the Lucas-Kanade tracker for homography matching can be found at
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opencv_source_code/samples/python/lk_homography.py
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*/
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CV_EXPORTS_W void calcOpticalFlowPyrLK( InputArray prevImg, InputArray nextImg,
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InputArray prevPts, InputOutputArray nextPts,
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OutputArray status, OutputArray err,
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Size winSize = Size(21,21), int maxLevel = 3,
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TermCriteria criteria = TermCriteria(TermCriteria::COUNT+TermCriteria::EPS, 30, 0.01),
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int flags = 0, double minEigThreshold = 1e-4 );
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/** @brief Computes a dense optical flow using the Gunnar Farneback's algorithm.
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@param prev first 8-bit single-channel input image.
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@param next second input image of the same size and the same type as prev.
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@param flow computed flow image that has the same size as prev and type CV_32FC2.
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@param pyr_scale parameter, specifying the image scale (\<1) to build pyramids for each image;
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pyr_scale=0.5 means a classical pyramid, where each next layer is twice smaller than the previous
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one.
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@param levels number of pyramid layers including the initial image; levels=1 means that no extra
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layers are created and only the original images are used.
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@param winsize averaging window size; larger values increase the algorithm robustness to image
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noise and give more chances for fast motion detection, but yield more blurred motion field.
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@param iterations number of iterations the algorithm does at each pyramid level.
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@param poly_n size of the pixel neighborhood used to find polynomial expansion in each pixel;
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larger values mean that the image will be approximated with smoother surfaces, yielding more
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robust algorithm and more blurred motion field, typically poly_n =5 or 7.
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@param poly_sigma standard deviation of the Gaussian that is used to smooth derivatives used as a
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basis for the polynomial expansion; for poly_n=5, you can set poly_sigma=1.1, for poly_n=7, a
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good value would be poly_sigma=1.5.
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@param flags operation flags that can be a combination of the following:
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- **OPTFLOW_USE_INITIAL_FLOW** uses the input flow as an initial flow approximation.
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- **OPTFLOW_FARNEBACK_GAUSSIAN** uses the Gaussian \f$\texttt{winsize}\times\texttt{winsize}\f$
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filter instead of a box filter of the same size for optical flow estimation; usually, this
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option gives z more accurate flow than with a box filter, at the cost of lower speed;
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normally, winsize for a Gaussian window should be set to a larger value to achieve the same
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level of robustness.
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The function finds an optical flow for each prev pixel using the @cite Farneback2003 algorithm so that
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\f[\texttt{prev} (y,x) \sim \texttt{next} ( y + \texttt{flow} (y,x)[1], x + \texttt{flow} (y,x)[0])\f]
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@note
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- An example using the optical flow algorithm described by Gunnar Farneback can be found at
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opencv_source_code/samples/cpp/fback.cpp
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- (Python) An example using the optical flow algorithm described by Gunnar Farneback can be
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found at opencv_source_code/samples/python/opt_flow.py
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*/
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CV_EXPORTS_W void calcOpticalFlowFarneback( InputArray prev, InputArray next, InputOutputArray flow,
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double pyr_scale, int levels, int winsize,
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int iterations, int poly_n, double poly_sigma,
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int flags );
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/** @brief Computes an optimal affine transformation between two 2D point sets.
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@param src First input 2D point set stored in std::vector or Mat, or an image stored in Mat.
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@param dst Second input 2D point set of the same size and the same type as A, or another image.
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@param fullAffine If true, the function finds an optimal affine transformation with no additional
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restrictions (6 degrees of freedom). Otherwise, the class of transformations to choose from is
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limited to combinations of translation, rotation, and uniform scaling (4 degrees of freedom).
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The function finds an optimal affine transform *[A|b]* (a 2 x 3 floating-point matrix) that
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approximates best the affine transformation between:
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* Two point sets
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* Two raster images. In this case, the function first finds some features in the src image and
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finds the corresponding features in dst image. After that, the problem is reduced to the first
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case.
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In case of point sets, the problem is formulated as follows: you need to find a 2x2 matrix *A* and
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2x1 vector *b* so that:
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\f[[A^*|b^*] = arg \min _{[A|b]} \sum _i \| \texttt{dst}[i] - A { \texttt{src}[i]}^T - b \| ^2\f]
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where src[i] and dst[i] are the i-th points in src and dst, respectively
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\f$[A|b]\f$ can be either arbitrary (when fullAffine=true ) or have a form of
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\f[\begin{bmatrix} a_{11} & a_{12} & b_1 \\ -a_{12} & a_{11} & b_2 \end{bmatrix}\f]
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when fullAffine=false.
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@sa
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estimateAffine2D, estimateAffinePartial2D, getAffineTransform, getPerspectiveTransform, findHomography
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*/
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CV_EXPORTS_W Mat estimateRigidTransform( InputArray src, InputArray dst, bool fullAffine );
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enum
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{
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MOTION_TRANSLATION = 0,
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MOTION_EUCLIDEAN = 1,
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MOTION_AFFINE = 2,
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MOTION_HOMOGRAPHY = 3
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};
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2018-02-01 21:10:10 +01:00
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/** @example image_alignment.cpp
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An example using the image alignment ECC algorithm
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*/
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2016-04-28 21:40:36 +02:00
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/** @brief Finds the geometric transform (warp) between two images in terms of the ECC criterion @cite EP08 .
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@param templateImage single-channel template image; CV_8U or CV_32F array.
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@param inputImage single-channel input image which should be warped with the final warpMatrix in
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order to provide an image similar to templateImage, same type as temlateImage.
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@param warpMatrix floating-point \f$2\times 3\f$ or \f$3\times 3\f$ mapping matrix (warp).
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@param motionType parameter, specifying the type of motion:
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- **MOTION_TRANSLATION** sets a translational motion model; warpMatrix is \f$2\times 3\f$ with
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the first \f$2\times 2\f$ part being the unity matrix and the rest two parameters being
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estimated.
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- **MOTION_EUCLIDEAN** sets a Euclidean (rigid) transformation as motion model; three
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parameters are estimated; warpMatrix is \f$2\times 3\f$.
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- **MOTION_AFFINE** sets an affine motion model (DEFAULT); six parameters are estimated;
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warpMatrix is \f$2\times 3\f$.
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- **MOTION_HOMOGRAPHY** sets a homography as a motion model; eight parameters are
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estimated;\`warpMatrix\` is \f$3\times 3\f$.
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@param criteria parameter, specifying the termination criteria of the ECC algorithm;
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criteria.epsilon defines the threshold of the increment in the correlation coefficient between two
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iterations (a negative criteria.epsilon makes criteria.maxcount the only termination criterion).
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Default values are shown in the declaration above.
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@param inputMask An optional mask to indicate valid values of inputImage.
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The function estimates the optimum transformation (warpMatrix) with respect to ECC criterion
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(@cite EP08), that is
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\f[\texttt{warpMatrix} = \texttt{warpMatrix} = \arg\max_{W} \texttt{ECC}(\texttt{templateImage}(x,y),\texttt{inputImage}(x',y'))\f]
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where
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\f[\begin{bmatrix} x' \\ y' \end{bmatrix} = W \cdot \begin{bmatrix} x \\ y \\ 1 \end{bmatrix}\f]
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(the equation holds with homogeneous coordinates for homography). It returns the final enhanced
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correlation coefficient, that is the correlation coefficient between the template image and the
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final warped input image. When a \f$3\times 3\f$ matrix is given with motionType =0, 1 or 2, the third
|
|
|
|
row is ignored.
|
|
|
|
|
|
|
|
Unlike findHomography and estimateRigidTransform, the function findTransformECC implements an
|
|
|
|
area-based alignment that builds on intensity similarities. In essence, the function updates the
|
|
|
|
initial transformation that roughly aligns the images. If this information is missing, the identity
|
2018-02-01 21:10:10 +01:00
|
|
|
warp (unity matrix) is used as an initialization. Note that if images undergo strong
|
2016-04-28 21:40:36 +02:00
|
|
|
displacements/rotations, an initial transformation that roughly aligns the images is necessary
|
|
|
|
(e.g., a simple euclidean/similarity transform that allows for the images showing the same image
|
|
|
|
content approximately). Use inverse warping in the second image to take an image close to the first
|
|
|
|
one, i.e. use the flag WARP_INVERSE_MAP with warpAffine or warpPerspective. See also the OpenCV
|
|
|
|
sample image_alignment.cpp that demonstrates the use of the function. Note that the function throws
|
|
|
|
an exception if algorithm does not converges.
|
|
|
|
|
|
|
|
@sa
|
2018-02-01 21:10:10 +01:00
|
|
|
estimateAffine2D, estimateAffinePartial2D, findHomography
|
2016-04-28 21:40:36 +02:00
|
|
|
*/
|
|
|
|
CV_EXPORTS_W double findTransformECC( InputArray templateImage, InputArray inputImage,
|
|
|
|
InputOutputArray warpMatrix, int motionType = MOTION_AFFINE,
|
|
|
|
TermCriteria criteria = TermCriteria(TermCriteria::COUNT+TermCriteria::EPS, 50, 0.001),
|
|
|
|
InputArray inputMask = noArray());
|
|
|
|
|
2018-02-01 21:10:10 +01:00
|
|
|
/** @example kalman.cpp
|
|
|
|
An example using the standard Kalman filter
|
|
|
|
*/
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @brief Kalman filter class.
|
|
|
|
|
|
|
|
The class implements a standard Kalman filter <http://en.wikipedia.org/wiki/Kalman_filter>,
|
|
|
|
@cite Welch95 . However, you can modify transitionMatrix, controlMatrix, and measurementMatrix to get
|
2018-02-01 21:10:10 +01:00
|
|
|
an extended Kalman filter functionality.
|
|
|
|
@note In C API when CvKalman\* kalmanFilter structure is not needed anymore, it should be released
|
|
|
|
with cvReleaseKalman(&kalmanFilter)
|
2016-04-28 21:40:36 +02:00
|
|
|
*/
|
|
|
|
class CV_EXPORTS_W KalmanFilter
|
|
|
|
{
|
|
|
|
public:
|
|
|
|
CV_WRAP KalmanFilter();
|
|
|
|
/** @overload
|
|
|
|
@param dynamParams Dimensionality of the state.
|
|
|
|
@param measureParams Dimensionality of the measurement.
|
|
|
|
@param controlParams Dimensionality of the control vector.
|
|
|
|
@param type Type of the created matrices that should be CV_32F or CV_64F.
|
|
|
|
*/
|
|
|
|
CV_WRAP KalmanFilter( int dynamParams, int measureParams, int controlParams = 0, int type = CV_32F );
|
|
|
|
|
|
|
|
/** @brief Re-initializes Kalman filter. The previous content is destroyed.
|
|
|
|
|
|
|
|
@param dynamParams Dimensionality of the state.
|
|
|
|
@param measureParams Dimensionality of the measurement.
|
|
|
|
@param controlParams Dimensionality of the control vector.
|
|
|
|
@param type Type of the created matrices that should be CV_32F or CV_64F.
|
|
|
|
*/
|
|
|
|
void init( int dynamParams, int measureParams, int controlParams = 0, int type = CV_32F );
|
|
|
|
|
|
|
|
/** @brief Computes a predicted state.
|
|
|
|
|
|
|
|
@param control The optional input control
|
|
|
|
*/
|
|
|
|
CV_WRAP const Mat& predict( const Mat& control = Mat() );
|
|
|
|
|
|
|
|
/** @brief Updates the predicted state from the measurement.
|
|
|
|
|
|
|
|
@param measurement The measured system parameters
|
|
|
|
*/
|
|
|
|
CV_WRAP const Mat& correct( const Mat& measurement );
|
|
|
|
|
|
|
|
CV_PROP_RW Mat statePre; //!< predicted state (x'(k)): x(k)=A*x(k-1)+B*u(k)
|
|
|
|
CV_PROP_RW Mat statePost; //!< corrected state (x(k)): x(k)=x'(k)+K(k)*(z(k)-H*x'(k))
|
|
|
|
CV_PROP_RW Mat transitionMatrix; //!< state transition matrix (A)
|
|
|
|
CV_PROP_RW Mat controlMatrix; //!< control matrix (B) (not used if there is no control)
|
|
|
|
CV_PROP_RW Mat measurementMatrix; //!< measurement matrix (H)
|
|
|
|
CV_PROP_RW Mat processNoiseCov; //!< process noise covariance matrix (Q)
|
|
|
|
CV_PROP_RW Mat measurementNoiseCov;//!< measurement noise covariance matrix (R)
|
|
|
|
CV_PROP_RW Mat errorCovPre; //!< priori error estimate covariance matrix (P'(k)): P'(k)=A*P(k-1)*At + Q)*/
|
|
|
|
CV_PROP_RW Mat gain; //!< Kalman gain matrix (K(k)): K(k)=P'(k)*Ht*inv(H*P'(k)*Ht+R)
|
|
|
|
CV_PROP_RW Mat errorCovPost; //!< posteriori error estimate covariance matrix (P(k)): P(k)=(I-K(k)*H)*P'(k)
|
|
|
|
|
|
|
|
// temporary matrices
|
|
|
|
Mat temp1;
|
|
|
|
Mat temp2;
|
|
|
|
Mat temp3;
|
|
|
|
Mat temp4;
|
|
|
|
Mat temp5;
|
|
|
|
};
|
|
|
|
|
|
|
|
|
|
|
|
class CV_EXPORTS_W DenseOpticalFlow : public Algorithm
|
|
|
|
{
|
|
|
|
public:
|
|
|
|
/** @brief Calculates an optical flow.
|
|
|
|
|
|
|
|
@param I0 first 8-bit single-channel input image.
|
|
|
|
@param I1 second input image of the same size and the same type as prev.
|
|
|
|
@param flow computed flow image that has the same size as prev and type CV_32FC2.
|
|
|
|
*/
|
|
|
|
CV_WRAP virtual void calc( InputArray I0, InputArray I1, InputOutputArray flow ) = 0;
|
|
|
|
/** @brief Releases all inner buffers.
|
|
|
|
*/
|
|
|
|
CV_WRAP virtual void collectGarbage() = 0;
|
|
|
|
};
|
|
|
|
|
2018-02-01 21:10:10 +01:00
|
|
|
/** @brief Base interface for sparse optical flow algorithms.
|
|
|
|
*/
|
|
|
|
class CV_EXPORTS_W SparseOpticalFlow : public Algorithm
|
|
|
|
{
|
|
|
|
public:
|
|
|
|
/** @brief Calculates a sparse optical flow.
|
|
|
|
|
|
|
|
@param prevImg First input image.
|
|
|
|
@param nextImg Second input image of the same size and the same type as prevImg.
|
|
|
|
@param prevPts Vector of 2D points for which the flow needs to be found.
|
|
|
|
@param nextPts Output vector of 2D points containing the calculated new positions of input features in the second image.
|
|
|
|
@param status Output status vector. Each element of the vector is set to 1 if the
|
|
|
|
flow for the corresponding features has been found. Otherwise, it is set to 0.
|
|
|
|
@param err Optional output vector that contains error response for each point (inverse confidence).
|
|
|
|
*/
|
|
|
|
CV_WRAP virtual void calc(InputArray prevImg, InputArray nextImg,
|
|
|
|
InputArray prevPts, InputOutputArray nextPts,
|
|
|
|
OutputArray status,
|
|
|
|
OutputArray err = cv::noArray()) = 0;
|
|
|
|
};
|
|
|
|
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @brief "Dual TV L1" Optical Flow Algorithm.
|
|
|
|
|
|
|
|
The class implements the "Dual TV L1" optical flow algorithm described in @cite Zach2007 and
|
|
|
|
@cite Javier2012 .
|
|
|
|
Here are important members of the class that control the algorithm, which you can set after
|
|
|
|
constructing the class instance:
|
|
|
|
|
|
|
|
- member double tau
|
|
|
|
Time step of the numerical scheme.
|
|
|
|
|
|
|
|
- member double lambda
|
|
|
|
Weight parameter for the data term, attachment parameter. This is the most relevant
|
|
|
|
parameter, which determines the smoothness of the output. The smaller this parameter is,
|
|
|
|
the smoother the solutions we obtain. It depends on the range of motions of the images, so
|
|
|
|
its value should be adapted to each image sequence.
|
|
|
|
|
|
|
|
- member double theta
|
|
|
|
Weight parameter for (u - v)\^2, tightness parameter. It serves as a link between the
|
|
|
|
attachment and the regularization terms. In theory, it should have a small value in order
|
|
|
|
to maintain both parts in correspondence. The method is stable for a large range of values
|
|
|
|
of this parameter.
|
|
|
|
|
|
|
|
- member int nscales
|
|
|
|
Number of scales used to create the pyramid of images.
|
|
|
|
|
|
|
|
- member int warps
|
|
|
|
Number of warpings per scale. Represents the number of times that I1(x+u0) and grad(
|
|
|
|
I1(x+u0) ) are computed per scale. This is a parameter that assures the stability of the
|
|
|
|
method. It also affects the running time, so it is a compromise between speed and
|
|
|
|
accuracy.
|
|
|
|
|
|
|
|
- member double epsilon
|
|
|
|
Stopping criterion threshold used in the numerical scheme, which is a trade-off between
|
|
|
|
precision and running time. A small value will yield more accurate solutions at the
|
|
|
|
expense of a slower convergence.
|
|
|
|
|
|
|
|
- member int iterations
|
|
|
|
Stopping criterion iterations number used in the numerical scheme.
|
|
|
|
|
|
|
|
C. Zach, T. Pock and H. Bischof, "A Duality Based Approach for Realtime TV-L1 Optical Flow".
|
|
|
|
Javier Sanchez, Enric Meinhardt-Llopis and Gabriele Facciolo. "TV-L1 Optical Flow Estimation".
|
|
|
|
*/
|
|
|
|
class CV_EXPORTS_W DualTVL1OpticalFlow : public DenseOpticalFlow
|
|
|
|
{
|
|
|
|
public:
|
|
|
|
//! @brief Time step of the numerical scheme
|
|
|
|
/** @see setTau */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual double getTau() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getTau @see getTau */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setTau(double val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Weight parameter for the data term, attachment parameter
|
|
|
|
/** @see setLambda */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual double getLambda() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getLambda @see getLambda */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setLambda(double val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Weight parameter for (u - v)^2, tightness parameter
|
|
|
|
/** @see setTheta */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual double getTheta() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getTheta @see getTheta */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setTheta(double val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief coefficient for additional illumination variation term
|
|
|
|
/** @see setGamma */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual double getGamma() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getGamma @see getGamma */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setGamma(double val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Number of scales used to create the pyramid of images
|
|
|
|
/** @see setScalesNumber */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual int getScalesNumber() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getScalesNumber @see getScalesNumber */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setScalesNumber(int val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Number of warpings per scale
|
|
|
|
/** @see setWarpingsNumber */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual int getWarpingsNumber() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getWarpingsNumber @see getWarpingsNumber */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setWarpingsNumber(int val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Stopping criterion threshold used in the numerical scheme, which is a trade-off between precision and running time
|
|
|
|
/** @see setEpsilon */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual double getEpsilon() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getEpsilon @see getEpsilon */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setEpsilon(double val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Inner iterations (between outlier filtering) used in the numerical scheme
|
|
|
|
/** @see setInnerIterations */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual int getInnerIterations() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getInnerIterations @see getInnerIterations */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setInnerIterations(int val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Outer iterations (number of inner loops) used in the numerical scheme
|
|
|
|
/** @see setOuterIterations */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual int getOuterIterations() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getOuterIterations @see getOuterIterations */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setOuterIterations(int val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Use initial flow
|
|
|
|
/** @see setUseInitialFlow */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual bool getUseInitialFlow() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getUseInitialFlow @see getUseInitialFlow */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setUseInitialFlow(bool val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Step between scales (<1)
|
|
|
|
/** @see setScaleStep */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual double getScaleStep() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getScaleStep @see getScaleStep */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setScaleStep(double val) = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
//! @brief Median filter kernel size (1 = no filter) (3 or 5)
|
|
|
|
/** @see setMedianFiltering */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual int getMedianFiltering() const = 0;
|
2016-04-28 21:40:36 +02:00
|
|
|
/** @copybrief getMedianFiltering @see getMedianFiltering */
|
2018-02-01 21:10:10 +01:00
|
|
|
CV_WRAP virtual void setMedianFiltering(int val) = 0;
|
|
|
|
|
|
|
|
/** @brief Creates instance of cv::DualTVL1OpticalFlow*/
|
|
|
|
CV_WRAP static Ptr<DualTVL1OpticalFlow> create(
|
|
|
|
double tau = 0.25,
|
|
|
|
double lambda = 0.15,
|
|
|
|
double theta = 0.3,
|
|
|
|
int nscales = 5,
|
|
|
|
int warps = 5,
|
|
|
|
double epsilon = 0.01,
|
|
|
|
int innnerIterations = 30,
|
|
|
|
int outerIterations = 10,
|
|
|
|
double scaleStep = 0.8,
|
|
|
|
double gamma = 0.0,
|
|
|
|
int medianFiltering = 5,
|
|
|
|
bool useInitialFlow = false);
|
2016-04-28 21:40:36 +02:00
|
|
|
};
|
|
|
|
|
|
|
|
/** @brief Creates instance of cv::DenseOpticalFlow
|
|
|
|
*/
|
|
|
|
CV_EXPORTS_W Ptr<DualTVL1OpticalFlow> createOptFlow_DualTVL1();
|
|
|
|
|
2018-02-01 21:10:10 +01:00
|
|
|
/** @brief Class computing a dense optical flow using the Gunnar Farneback's algorithm.
|
|
|
|
*/
|
|
|
|
class CV_EXPORTS_W FarnebackOpticalFlow : public DenseOpticalFlow
|
|
|
|
{
|
|
|
|
public:
|
|
|
|
CV_WRAP virtual int getNumLevels() const = 0;
|
|
|
|
CV_WRAP virtual void setNumLevels(int numLevels) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual double getPyrScale() const = 0;
|
|
|
|
CV_WRAP virtual void setPyrScale(double pyrScale) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual bool getFastPyramids() const = 0;
|
|
|
|
CV_WRAP virtual void setFastPyramids(bool fastPyramids) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual int getWinSize() const = 0;
|
|
|
|
CV_WRAP virtual void setWinSize(int winSize) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual int getNumIters() const = 0;
|
|
|
|
CV_WRAP virtual void setNumIters(int numIters) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual int getPolyN() const = 0;
|
|
|
|
CV_WRAP virtual void setPolyN(int polyN) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual double getPolySigma() const = 0;
|
|
|
|
CV_WRAP virtual void setPolySigma(double polySigma) = 0;
|
|
|
|
|
|
|
|
CV_WRAP virtual int getFlags() const = 0;
|
|
|
|
CV_WRAP virtual void setFlags(int flags) = 0;
|
|
|
|
|
|
|
|
CV_WRAP static Ptr<FarnebackOpticalFlow> create(
|
|
|
|
int numLevels = 5,
|
|
|
|
double pyrScale = 0.5,
|
|
|
|
bool fastPyramids = false,
|
|
|
|
int winSize = 13,
|
|
|
|
int numIters = 10,
|
|
|
|
int polyN = 5,
|
|
|
|
double polySigma = 1.1,
|
|
|
|
int flags = 0);
|
|
|
|
};
|
|
|
|
|
|
|
|
|
|
|
|
/** @brief Class used for calculating a sparse optical flow.
|
|
|
|
|
|
|
|
The class can calculate an optical flow for a sparse feature set using the
|
|
|
|
iterative Lucas-Kanade method with pyramids.
|
|
|
|
|
|
|
|
@sa calcOpticalFlowPyrLK
|
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|
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*/
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class CV_EXPORTS_W SparsePyrLKOpticalFlow : public SparseOpticalFlow
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{
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public:
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CV_WRAP virtual Size getWinSize() const = 0;
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CV_WRAP virtual void setWinSize(Size winSize) = 0;
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CV_WRAP virtual int getMaxLevel() const = 0;
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CV_WRAP virtual void setMaxLevel(int maxLevel) = 0;
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CV_WRAP virtual TermCriteria getTermCriteria() const = 0;
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CV_WRAP virtual void setTermCriteria(TermCriteria& crit) = 0;
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CV_WRAP virtual int getFlags() const = 0;
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CV_WRAP virtual void setFlags(int flags) = 0;
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CV_WRAP virtual double getMinEigThreshold() const = 0;
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CV_WRAP virtual void setMinEigThreshold(double minEigThreshold) = 0;
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CV_WRAP static Ptr<SparsePyrLKOpticalFlow> create(
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Size winSize = Size(21, 21),
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int maxLevel = 3, TermCriteria crit =
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TermCriteria(TermCriteria::COUNT+TermCriteria::EPS, 30, 0.01),
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int flags = 0,
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double minEigThreshold = 1e-4);
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};
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2016-04-28 21:40:36 +02:00
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//! @} video_track
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} // cv
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#endif
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