Fix(wechat_code): Modify isnan for compatibility with -ffast_math. #3490fix#3150
Merge with https://github.com/opencv/opencv/pull/23881
Reference: https://stackoverflow.com/questions/7263404/mingw32-stdisnan-with-ffast-math
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first proposal of cv::remap with relative displacement field
Relates to [#24621](https://github.com/opencv/opencv/pull/24621), [#24603](https://github.com/opencv/opencv/issues/24603)
CUDA implementation of the feature
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Add interleaved versions of phase/cartToPolar/polarToCart #3607
This PR is for performance only (at the cost of more template code and increased GPU code size) The additional variants can help the caller skip the creation of temporary GPU mats (where memory is more likely to be a critical resource), and can even allow in-place processing. magnitude/angles/x/y are often already interleaved when dealing with DFTs.
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supports empty kernels in cuda::SeparableLinearFilters #3731
[#25408](https://github.com/opencv/opencv/issues/25408)
When only 1D convolution is needed (row or column filter only), `cuda::LinearFilter` might be slower than `cuda::SeparableLinearFilter`
Using `cuda::SeparableLinearFilter` for 1D convolution can be done by using a `(1)` kernel for the ignored dimension.
By supporting empty kernels in `cuda::SeparableLinearFilter`, there is no need for that `(1)` kernel any more.
Additionaly, the inner `_buf ` used to store the intermediate convolution result can be saved when a single convolution is needed.
In "legacy" usage (row+col kernels), there is no regression in `cuda::SeparableLinearFilter` performance.
As soon as an empty kernel is used, the performance is largely increased.
Devil in the details : the "in-place" processing is supported and might need intermediate buf, but still no regression.
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Add conditional include for <cuda/std/tuple> to support CUDA 12.4+ #3751
Fixes https://github.com/opencv/opencv_contrib/issues/3752
Adds a preprocessor check to conditionally include <cuda/std/tuple> only for CUDA versions 12.4 and above. This ensures backward compatibility with older legacy CUDA versions.
Related to pull request #3744
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Added CUDA 12.4+ support #3744
Tries to fix https://github.com/opencv/opencv_contrib/issues/3690 for CUDA 12.4+
Related patch to main repo: https://github.com/opencv/opencv/pull/25658
Changes:
- Added branches to support new variadic implementation of thrust::tuple
- Added branch with std::array instead of std::tuple in split-merge and grid operations. The new branch got rid of namespace clash: cv::cuda in OpenCV and ::cuda in CUDA standard library (injected by Thrust). Old tuple branches presumed for compatibility with old code and CUDA versions before 12.4.
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Misc thinning fixes. #3743
- edges could be modified
- 2 sets of iterations were always done even if the first set did not return any change
- countNonZero is slow compared to hasNonZero
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Implemented fast median filter for CUDA using Wavelet Matrix, a constant-time, HDR-compatible method #3627
I replaced the existing CUDA implementation of the histogram-based median filter with an implementation of a new wavelet matrix-based median filter algorithm, which I presented at SIGGRAPH Asia 2022.
This paper won the Best Paper Award in the journal track of technical papers (ACM Transactions on Graphics).
This new algorithm, like the histogram method, has the property that the window radius does not affect the computation time, and is several times faster than the histogram method. Furthermore, while the histogram method does not support HDR and only supports 8U images, this new algorithm supports HDR and also supports 16U and 32F images.
I (the author) have published the implementation on my personal GitHub and made some modifications for OpenCV to make it accessible from OpenCV. I used the CUB library, which is part of the standard toolkit since CUDA 11.0. Therefore, depending on the CUDA_VERSION, the code is written to use the new algorithm for versions 11.0 and above, and the existing histogram method for versions 10 and below.
Regarding the old histogram-based code, the CPU version of the median filter supports 16U and 32F for window sizes up to 5, but it seems that the histogram CUDA version of the median filter does not. Also, the number of channels supported is different: the CPU version supports 1, 3, and 4 channels, while the CUDA version supports only 1 channel. In addition, for the CUDA version of the histogram method, pixels at the edges of the image, i.e. where the window is insufficient, were set to zero. For example, if the window size is 7, the width of the 3 pixels at the top, bottom, left, and right were not calculated correctly. When checking the tests, it was found that they compared with the CPU version by cropping the edges with rect, and also the cropping area was too wide, with 8 pixels cropped from the top, bottom, left, and right when the window size was 7.
In this PR, I first corrected the rect range for the tests so that both the old histogram method and the new wavelet matrix method can pass. Also, the CUDA version now supports 16U, 32F, and multi-channel formats such as 3 and 4 channels. In addition, while the CPU version only supports window sizes up to 5 for HDR, the new CUDA Wavelet Matrix method supports sizes of 7 and above. Additionally, I have added new tests for 16U, 32F, and multi-channel formats, specifically 3 and 4 channels.
Paper’s project page: [Constant Time Median Filter using 2D Wavelet Matrix | Interactive Graphics & Engineering Lab](https://cgenglab.github.io/en/publication/sigga22_wmatrix_median/)
My implementation (as author): [GitHub - TumoiYorozu/WMatrixMedian](https://github.com/TumoiYorozu/WMatrixMedian)
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Fixed Wredundant-move produced by GCC 13.2 (Ubuntu 24.04). #3734
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ovis: force camera extent update to get correct bbox #3735
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---
fixes#3732
Camera spatial velocity computation through interaction matrix #3641
### Feature
The code computed camera spatial velocity given two images, pixels depth, camera matrix and the timestamp between the images. This is enabled by, so called, interaction matrix (usually utilized in visual servoing applications) relating pixel plane velocities to the camera spatial velocity in 3D i.e., twist - velocity and angular rate of the camera. The inverse problem can be solved by sampling pixel & their velocities to solve least-squares for twist. The relationship can be seen below in the picture.
The code does not include a proper example and is not tested but if there is interest I could contribute more appealing example and use case for camera velocity computation. However, I attach below a dummy example with random data simply to make sure that it's running as is. I have used this before in aiding UAV localization and thought someone else might benefit from it being integrated into `opencv`.
```c++
#include "opencv2/rgbd/twist.hpp"
#include "opencv2/core.hpp"
#include "opencv2/imgproc.hpp"
int main()
{
using namespace cv::rgbd;
Twist t;
// create two random image
cv::Mat im0(480, 640, CV_8UC1);
cv::Mat im1(480, 640, CV_8UC1);
cv::Mat depths0(480, 640, CV_32F);
cv::Mat K = cv::Mat::eye(3, 3, CV_32F);
cv::theRNG().state = time(0);
cv::randn(im0, 0, 255);
cv::randn(im1, 0, 255);
cv::randn(depths0, 0, 100);
cv::Vec6d twist = t.compute(im0, im1, depths0, K, 0.1);
return 0;
}
```
References
1. Chaumette, François, and Seth Hutchinson. "Visual servo control. I. Basic approaches." IEEE Robotics & Automation Magazine 13.4 (2006): 82-90.
2. https://robotacademy.net.au/lesson/image-based-visual-servoing/
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cudawarped
Alexander Smorkalov
Alexander Smorkalov
masterAllen
Nano
Kumataro
Yannis Guyon
Pierre Chatelier
Gregor Burger
Peter Rekdal Khan-Sunde
Vincent Rabaud
Wang Qiang
TumoiYorozu
Pavel Rojtberg
sdy623
catree
ernie
Maksim Shabunin
AleksandrPanov
roger8