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a99b4071a2
GSoC module to save and load point cloud * Add functionality to read point cloud data from files * address issues found on review, add tests for mesh, refactor * enable fail-safe execution and empty arrays as output * Some improvements for point cloud io module Co-authored-by: Julie Bareeva <julia.bareeva@xperience.ai>
2669 lines
136 KiB
C++
2669 lines
136 KiB
C++
// This file is part of OpenCV project.
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// It is subject to the license terms in the LICENSE file found in the top-level directory
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// of this distribution and at http://opencv.org/license.html
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#ifndef OPENCV_3D_HPP
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#define OPENCV_3D_HPP
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#include "opencv2/core.hpp"
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#include "opencv2/core/types_c.h"
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#include "opencv2/3d/depth.hpp"
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#include "opencv2/3d/odometry.hpp"
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#include "opencv2/3d/odometry_frame.hpp"
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#include "opencv2/3d/odometry_settings.hpp"
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#include "opencv2/3d/volume.hpp"
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#include "opencv2/3d/ptcloud.hpp"
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/**
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@defgroup _3d 3D vision functionality
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Most of the functions in this section use a so-called pinhole camera model. The view of a scene
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is obtained by projecting a scene's 3D point \f$P_w\f$ into the image plane using a perspective
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transformation which forms the corresponding pixel \f$p\f$. Both \f$P_w\f$ and \f$p\f$ are
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represented in homogeneous coordinates, i.e. as 3D and 2D homogeneous vector respectively. You will
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find a brief introduction to projective geometry, homogeneous vectors and homogeneous
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transformations at the end of this section's introduction. For more succinct notation, we often drop
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the 'homogeneous' and say vector instead of homogeneous vector.
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The distortion-free projective transformation given by a pinhole camera model is shown below.
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\f[s \; p = A \begin{bmatrix} R|t \end{bmatrix} P_w,\f]
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where \f$P_w\f$ is a 3D point expressed with respect to the world coordinate system,
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\f$p\f$ is a 2D pixel in the image plane, \f$A\f$ is the camera intrinsic matrix,
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\f$R\f$ and \f$t\f$ are the rotation and translation that describe the change of coordinates from
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world to camera coordinate systems (or camera frame) and \f$s\f$ is the projective transformation's
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arbitrary scaling and not part of the camera model.
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The camera intrinsic matrix \f$A\f$ (notation used as in @cite Zhang2000 and also generally notated
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as \f$K\f$) projects 3D points given in the camera coordinate system to 2D pixel coordinates, i.e.
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\f[p = A P_c.\f]
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The camera intrinsic matrix \f$A\f$ is composed of the focal lengths \f$f_x\f$ and \f$f_y\f$, which are
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expressed in pixel units, and the principal point \f$(c_x, c_y)\f$, that is usually close to the
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image center:
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\f[A = \vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1},\f]
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and thus
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\f[s \vecthree{u}{v}{1} = \vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1} \vecthree{X_c}{Y_c}{Z_c}.\f]
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The matrix of intrinsic parameters does not depend on the scene viewed. So, once estimated, it can
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be re-used as long as the focal length is fixed (in case of a zoom lens). Thus, if an image from the
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camera is scaled by a factor, all of these parameters need to be scaled (multiplied/divided,
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respectively) by the same factor.
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The joint rotation-translation matrix \f$[R|t]\f$ is the matrix product of a projective
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transformation and a homogeneous transformation. The 3-by-4 projective transformation maps 3D points
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represented in camera coordinates to 2D points in the image plane and represented in normalized
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camera coordinates \f$x' = X_c / Z_c\f$ and \f$y' = Y_c / Z_c\f$:
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\f[Z_c \begin{bmatrix}
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x' \\
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y' \\
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1
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\end{bmatrix} = \begin{bmatrix}
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1 & 0 & 0 & 0 \\
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0 & 1 & 0 & 0 \\
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0 & 0 & 1 & 0
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\end{bmatrix}
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\begin{bmatrix}
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X_c \\
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Y_c \\
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Z_c \\
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1
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\end{bmatrix}.\f]
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The homogeneous transformation is encoded by the extrinsic parameters \f$R\f$ and \f$t\f$ and
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represents the change of basis from world coordinate system \f$w\f$ to the camera coordinate sytem
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\f$c\f$. Thus, given the representation of the point \f$P\f$ in world coordinates, \f$P_w\f$, we
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obtain \f$P\f$'s representation in the camera coordinate system, \f$P_c\f$, by
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\f[P_c = \begin{bmatrix}
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R & t \\
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0 & 1
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\end{bmatrix} P_w,\f]
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This homogeneous transformation is composed out of \f$R\f$, a 3-by-3 rotation matrix, and \f$t\f$, a
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3-by-1 translation vector:
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\f[\begin{bmatrix}
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R & t \\
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0 & 1
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\end{bmatrix} = \begin{bmatrix}
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r_{11} & r_{12} & r_{13} & t_x \\
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r_{21} & r_{22} & r_{23} & t_y \\
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r_{31} & r_{32} & r_{33} & t_z \\
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0 & 0 & 0 & 1
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\end{bmatrix},
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\f]
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and therefore
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\f[\begin{bmatrix}
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X_c \\
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Y_c \\
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Z_c \\
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1
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\end{bmatrix} = \begin{bmatrix}
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r_{11} & r_{12} & r_{13} & t_x \\
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r_{21} & r_{22} & r_{23} & t_y \\
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r_{31} & r_{32} & r_{33} & t_z \\
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0 & 0 & 0 & 1
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\end{bmatrix}
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\begin{bmatrix}
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X_w \\
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Y_w \\
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Z_w \\
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1
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\end{bmatrix}.\f]
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Combining the projective transformation and the homogeneous transformation, we obtain the projective
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transformation that maps 3D points in world coordinates into 2D points in the image plane and in
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normalized camera coordinates:
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\f[Z_c \begin{bmatrix}
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x' \\
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y' \\
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1
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\end{bmatrix} = \begin{bmatrix} R|t \end{bmatrix} \begin{bmatrix}
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X_w \\
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Y_w \\
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Z_w \\
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1
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\end{bmatrix} = \begin{bmatrix}
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r_{11} & r_{12} & r_{13} & t_x \\
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r_{21} & r_{22} & r_{23} & t_y \\
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r_{31} & r_{32} & r_{33} & t_z
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\end{bmatrix}
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\begin{bmatrix}
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X_w \\
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Y_w \\
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Z_w \\
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1
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\end{bmatrix},\f]
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with \f$x' = X_c / Z_c\f$ and \f$y' = Y_c / Z_c\f$. Putting the equations for instrincs and extrinsics together, we can write out
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\f$s \; p = A \begin{bmatrix} R|t \end{bmatrix} P_w\f$ as
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\f[s \vecthree{u}{v}{1} = \vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}
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\begin{bmatrix}
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r_{11} & r_{12} & r_{13} & t_x \\
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r_{21} & r_{22} & r_{23} & t_y \\
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r_{31} & r_{32} & r_{33} & t_z
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\end{bmatrix}
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\begin{bmatrix}
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X_w \\
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Y_w \\
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Z_w \\
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1
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\end{bmatrix}.\f]
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If \f$Z_c \ne 0\f$, the transformation above is equivalent to the following,
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\f[\begin{bmatrix}
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u \\
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v
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\end{bmatrix} = \begin{bmatrix}
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f_x X_c/Z_c + c_x \\
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f_y Y_c/Z_c + c_y
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\end{bmatrix}\f]
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with
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\f[\vecthree{X_c}{Y_c}{Z_c} = \begin{bmatrix}
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R|t
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\end{bmatrix} \begin{bmatrix}
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X_w \\
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Y_w \\
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Z_w \\
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1
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\end{bmatrix}.\f]
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The following figure illustrates the pinhole camera model.
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![Pinhole camera model](pics/pinhole_camera_model.png)
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Real lenses usually have some distortion, mostly radial distortion, and slight tangential distortion.
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So, the above model is extended as:
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\f[\begin{bmatrix}
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u \\
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v
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\end{bmatrix} = \begin{bmatrix}
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f_x x'' + c_x \\
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f_y y'' + c_y
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\end{bmatrix}\f]
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where
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\f[\begin{bmatrix}
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x'' \\
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y''
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\end{bmatrix} = \begin{bmatrix}
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x' \frac{1 + k_1 r^2 + k_2 r^4 + k_3 r^6}{1 + k_4 r^2 + k_5 r^4 + k_6 r^6} + 2 p_1 x' y' + p_2(r^2 + 2 x'^2) + s_1 r^2 + s_2 r^4 \\
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y' \frac{1 + k_1 r^2 + k_2 r^4 + k_3 r^6}{1 + k_4 r^2 + k_5 r^4 + k_6 r^6} + p_1 (r^2 + 2 y'^2) + 2 p_2 x' y' + s_3 r^2 + s_4 r^4 \\
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\end{bmatrix}\f]
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with
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\f[r^2 = x'^2 + y'^2\f]
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and
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\f[\begin{bmatrix}
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x'\\
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y'
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\end{bmatrix} = \begin{bmatrix}
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X_c/Z_c \\
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Y_c/Z_c
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\end{bmatrix},\f]
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if \f$Z_c \ne 0\f$.
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The distortion parameters are the radial coefficients \f$k_1\f$, \f$k_2\f$, \f$k_3\f$, \f$k_4\f$, \f$k_5\f$, and \f$k_6\f$
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,\f$p_1\f$ and \f$p_2\f$ are the tangential distortion coefficients, and \f$s_1\f$, \f$s_2\f$, \f$s_3\f$, and \f$s_4\f$,
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are the thin prism distortion coefficients. Higher-order coefficients are not considered in OpenCV.
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The next figures show two common types of radial distortion: barrel distortion
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(\f$ 1 + k_1 r^2 + k_2 r^4 + k_3 r^6 \f$ monotonically decreasing)
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and pincushion distortion (\f$ 1 + k_1 r^2 + k_2 r^4 + k_3 r^6 \f$ monotonically increasing).
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Radial distortion is always monotonic for real lenses,
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and if the estimator produces a non-monotonic result,
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this should be considered a calibration failure.
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More generally, radial distortion must be monotonic and the distortion function must be bijective.
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A failed estimation result may look deceptively good near the image center
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but will work poorly in e.g. AR/SFM applications.
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The optimization method used in OpenCV camera calibration does not include these constraints as
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the framework does not support the required integer programming and polynomial inequalities.
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See [issue #15992](https://github.com/opencv/opencv/issues/15992) for additional information.
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![](pics/distortion_examples.png)
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![](pics/distortion_examples2.png)
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In some cases, the image sensor may be tilted in order to focus an oblique plane in front of the
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camera (Scheimpflug principle). This can be useful for particle image velocimetry (PIV) or
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triangulation with a laser fan. The tilt causes a perspective distortion of \f$x''\f$ and
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\f$y''\f$. This distortion can be modeled in the following way, see e.g. @cite Louhichi07.
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\f[\begin{bmatrix}
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u \\
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v
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\end{bmatrix} = \begin{bmatrix}
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f_x x''' + c_x \\
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f_y y''' + c_y
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\end{bmatrix},\f]
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where
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\f[s\vecthree{x'''}{y'''}{1} =
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\vecthreethree{R_{33}(\tau_x, \tau_y)}{0}{-R_{13}(\tau_x, \tau_y)}
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{0}{R_{33}(\tau_x, \tau_y)}{-R_{23}(\tau_x, \tau_y)}
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{0}{0}{1} R(\tau_x, \tau_y) \vecthree{x''}{y''}{1}\f]
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and the matrix \f$R(\tau_x, \tau_y)\f$ is defined by two rotations with angular parameter
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\f$\tau_x\f$ and \f$\tau_y\f$, respectively,
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\f[
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R(\tau_x, \tau_y) =
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\vecthreethree{\cos(\tau_y)}{0}{-\sin(\tau_y)}{0}{1}{0}{\sin(\tau_y)}{0}{\cos(\tau_y)}
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\vecthreethree{1}{0}{0}{0}{\cos(\tau_x)}{\sin(\tau_x)}{0}{-\sin(\tau_x)}{\cos(\tau_x)} =
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\vecthreethree{\cos(\tau_y)}{\sin(\tau_y)\sin(\tau_x)}{-\sin(\tau_y)\cos(\tau_x)}
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{0}{\cos(\tau_x)}{\sin(\tau_x)}
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{\sin(\tau_y)}{-\cos(\tau_y)\sin(\tau_x)}{\cos(\tau_y)\cos(\tau_x)}.
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\f]
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In the functions below the coefficients are passed or returned as
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\f[(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6 [, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f]
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vector. That is, if the vector contains four elements, it means that \f$k_3=0\f$ . The distortion
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coefficients do not depend on the scene viewed. Thus, they also belong to the intrinsic camera
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parameters. And they remain the same regardless of the captured image resolution. If, for example, a
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camera has been calibrated on images of 320 x 240 resolution, absolutely the same distortion
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coefficients can be used for 640 x 480 images from the same camera while \f$f_x\f$, \f$f_y\f$,
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\f$c_x\f$, and \f$c_y\f$ need to be scaled appropriately.
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The functions below use the above model to do the following:
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- Project 3D points to the image plane given intrinsic and extrinsic parameters.
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- Compute extrinsic parameters given intrinsic parameters, a few 3D points, and their
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projections.
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- Estimate intrinsic and extrinsic camera parameters from several views of a known calibration
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pattern (every view is described by several 3D-2D point correspondences).
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- Estimate the relative position and orientation of the stereo camera "heads" and compute the
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*rectification* transformation that makes the camera optical axes parallel.
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<B> Homogeneous Coordinates </B><br>
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Homogeneous Coordinates are a system of coordinates that are used in projective geometry. Their use
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allows to represent points at infinity by finite coordinates and simplifies formulas when compared
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to the cartesian counterparts, e.g. they have the advantage that affine transformations can be
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expressed as linear homogeneous transformation.
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One obtains the homogeneous vector \f$P_h\f$ by appending a 1 along an n-dimensional cartesian
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vector \f$P\f$ e.g. for a 3D cartesian vector the mapping \f$P \rightarrow P_h\f$ is:
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\f[\begin{bmatrix}
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X \\
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Y \\
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Z
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\end{bmatrix} \rightarrow \begin{bmatrix}
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X \\
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Y \\
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Z \\
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1
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\end{bmatrix}.\f]
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For the inverse mapping \f$P_h \rightarrow P\f$, one divides all elements of the homogeneous vector
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by its last element, e.g. for a 3D homogeneous vector one gets its 2D cartesian counterpart by:
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\f[\begin{bmatrix}
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X \\
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Y \\
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W
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\end{bmatrix} \rightarrow \begin{bmatrix}
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X / W \\
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Y / W
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\end{bmatrix},\f]
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if \f$W \ne 0\f$.
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Due to this mapping, all multiples \f$k P_h\f$, for \f$k \ne 0\f$, of a homogeneous point represent
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the same point \f$P_h\f$. An intuitive understanding of this property is that under a projective
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transformation, all multiples of \f$P_h\f$ are mapped to the same point. This is the physical
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observation one does for pinhole cameras, as all points along a ray through the camera's pinhole are
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projected to the same image point, e.g. all points along the red ray in the image of the pinhole
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camera model above would be mapped to the same image coordinate. This property is also the source
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for the scale ambiguity s in the equation of the pinhole camera model.
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As mentioned, by using homogeneous coordinates we can express any change of basis parameterized by
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\f$R\f$ and \f$t\f$ as a linear transformation, e.g. for the change of basis from coordinate system
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0 to coordinate system 1 becomes:
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\f[P_1 = R P_0 + t \rightarrow P_{h_1} = \begin{bmatrix}
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R & t \\
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0 & 1
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\end{bmatrix} P_{h_0}.\f]
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@note
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- Many functions in this module take a camera intrinsic matrix as an input parameter. Although all
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functions assume the same structure of this parameter, they may name it differently. The
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parameter's description, however, will be clear in that a camera intrinsic matrix with the structure
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shown above is required.
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- A calibration sample for 3 cameras in a horizontal position can be found at
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opencv_source_code/samples/cpp/3calibration.cpp
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- A calibration sample based on a sequence of images can be found at
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opencv_source_code/samples/cpp/calibration.cpp
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- A calibration sample in order to do 3D reconstruction can be found at
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opencv_source_code/samples/cpp/build3dmodel.cpp
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- A calibration example on stereo calibration can be found at
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opencv_source_code/samples/cpp/stereo_calib.cpp
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- A calibration example on stereo matching can be found at
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opencv_source_code/samples/cpp/stereo_match.cpp
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- (Python) A camera calibration sample can be found at
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opencv_source_code/samples/python/calibrate.py
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*/
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namespace cv {
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//! @addtogroup _3d
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//! @{
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//! type of the robust estimation algorithm
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enum { LMEDS = 4, //!< least-median of squares algorithm
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RANSAC = 8, //!< RANSAC algorithm
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RHO = 16, //!< RHO algorithm
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USAC_DEFAULT = 32, //!< USAC algorithm, default settings
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USAC_PARALLEL = 33, //!< USAC, parallel version
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USAC_FM_8PTS = 34, //!< USAC, fundamental matrix 8 points
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USAC_FAST = 35, //!< USAC, fast settings
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USAC_ACCURATE = 36, //!< USAC, accurate settings
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USAC_PROSAC = 37, //!< USAC, sorted points, runs PROSAC
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USAC_MAGSAC = 38 //!< USAC, runs MAGSAC++
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};
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enum SolvePnPMethod {
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SOLVEPNP_ITERATIVE = 0, //!< Pose refinement using non-linear Levenberg-Marquardt minimization scheme @cite Madsen04 @cite Eade13 \n
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//!< Initial solution for non-planar "objectPoints" needs at least 6 points and uses the DLT algorithm. \n
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//!< Initial solution for planar "objectPoints" needs at least 4 points and uses pose from homography decomposition.
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SOLVEPNP_EPNP = 1, //!< EPnP: Efficient Perspective-n-Point Camera Pose Estimation @cite lepetit2009epnp
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SOLVEPNP_P3P = 2, //!< Complete Solution Classification for the Perspective-Three-Point Problem @cite gao2003complete
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SOLVEPNP_DLS = 3, //!< **Broken implementation. Using this flag will fallback to EPnP.** \n
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//!< A Direct Least-Squares (DLS) Method for PnP @cite hesch2011direct
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SOLVEPNP_UPNP = 4, //!< **Broken implementation. Using this flag will fallback to EPnP.** \n
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//!< Exhaustive Linearization for Robust Camera Pose and Focal Length Estimation @cite penate2013exhaustive
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SOLVEPNP_AP3P = 5, //!< An Efficient Algebraic Solution to the Perspective-Three-Point Problem @cite Ke17
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SOLVEPNP_IPPE = 6, //!< Infinitesimal Plane-Based Pose Estimation @cite Collins14 \n
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//!< Object points must be coplanar.
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SOLVEPNP_IPPE_SQUARE = 7, //!< Infinitesimal Plane-Based Pose Estimation @cite Collins14 \n
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//!< This is a special case suitable for marker pose estimation.\n
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//!< 4 coplanar object points must be defined in the following order:
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|
//!< - point 0: [-squareLength / 2, squareLength / 2, 0]
|
|
//!< - point 1: [ squareLength / 2, squareLength / 2, 0]
|
|
//!< - point 2: [ squareLength / 2, -squareLength / 2, 0]
|
|
//!< - point 3: [-squareLength / 2, -squareLength / 2, 0]
|
|
SOLVEPNP_SQPNP = 8, //!< SQPnP: A Consistently Fast and Globally OptimalSolution to the Perspective-n-Point Problem @cite Terzakis2020SQPnP
|
|
#ifndef CV_DOXYGEN
|
|
SOLVEPNP_MAX_COUNT //!< Used for count
|
|
#endif
|
|
};
|
|
|
|
//! the algorithm for finding fundamental matrix
|
|
enum { FM_7POINT = 1, //!< 7-point algorithm
|
|
FM_8POINT = 2, //!< 8-point algorithm
|
|
FM_LMEDS = 4, //!< least-median algorithm. 7-point algorithm is used.
|
|
FM_RANSAC = 8 //!< RANSAC algorithm. It needs at least 15 points. 7-point algorithm is used.
|
|
};
|
|
|
|
enum SamplingMethod { SAMPLING_UNIFORM, SAMPLING_PROGRESSIVE_NAPSAC, SAMPLING_NAPSAC,
|
|
SAMPLING_PROSAC };
|
|
enum LocalOptimMethod {LOCAL_OPTIM_NULL, LOCAL_OPTIM_INNER_LO, LOCAL_OPTIM_INNER_AND_ITER_LO,
|
|
LOCAL_OPTIM_GC, LOCAL_OPTIM_SIGMA};
|
|
enum ScoreMethod {SCORE_METHOD_RANSAC, SCORE_METHOD_MSAC, SCORE_METHOD_MAGSAC, SCORE_METHOD_LMEDS};
|
|
enum NeighborSearchMethod { NEIGH_FLANN_KNN, NEIGH_GRID, NEIGH_FLANN_RADIUS };
|
|
|
|
struct CV_EXPORTS_W_SIMPLE UsacParams
|
|
{ // in alphabetical order
|
|
CV_WRAP UsacParams();
|
|
CV_PROP_RW double confidence;
|
|
CV_PROP_RW bool isParallel;
|
|
CV_PROP_RW int loIterations;
|
|
CV_PROP_RW LocalOptimMethod loMethod;
|
|
CV_PROP_RW int loSampleSize;
|
|
CV_PROP_RW int maxIterations;
|
|
CV_PROP_RW NeighborSearchMethod neighborsSearch;
|
|
CV_PROP_RW int randomGeneratorState;
|
|
CV_PROP_RW SamplingMethod sampler;
|
|
CV_PROP_RW ScoreMethod score;
|
|
CV_PROP_RW double threshold;
|
|
};
|
|
|
|
/** @brief Converts a rotation matrix to a rotation vector or vice versa.
|
|
|
|
@param src Input rotation vector (3x1 or 1x3) or rotation matrix (3x3).
|
|
@param dst Output rotation matrix (3x3) or rotation vector (3x1 or 1x3), respectively.
|
|
@param jacobian Optional output Jacobian matrix, 3x9 or 9x3, which is a matrix of partial
|
|
derivatives of the output array components with respect to the input array components.
|
|
|
|
\f[\begin{array}{l} \theta \leftarrow norm(r) \\ r \leftarrow r/ \theta \\ R = \cos(\theta) I + (1- \cos{\theta} ) r r^T + \sin(\theta) \vecthreethree{0}{-r_z}{r_y}{r_z}{0}{-r_x}{-r_y}{r_x}{0} \end{array}\f]
|
|
|
|
Inverse transformation can be also done easily, since
|
|
|
|
\f[\sin ( \theta ) \vecthreethree{0}{-r_z}{r_y}{r_z}{0}{-r_x}{-r_y}{r_x}{0} = \frac{R - R^T}{2}\f]
|
|
|
|
A rotation vector is a convenient and most compact representation of a rotation matrix (since any
|
|
rotation matrix has just 3 degrees of freedom). The representation is used in the global 3D geometry
|
|
optimization procedures like @ref calibrateCamera, @ref stereoCalibrate, or @ref solvePnP .
|
|
|
|
@note More information about the computation of the derivative of a 3D rotation matrix with respect to its exponential coordinate
|
|
can be found in:
|
|
- A Compact Formula for the Derivative of a 3-D Rotation in Exponential Coordinates, Guillermo Gallego, Anthony J. Yezzi @cite Gallego2014ACF
|
|
|
|
@note Useful information on SE(3) and Lie Groups can be found in:
|
|
- A tutorial on SE(3) transformation parameterizations and on-manifold optimization, Jose-Luis Blanco @cite blanco2010tutorial
|
|
- Lie Groups for 2D and 3D Transformation, Ethan Eade @cite Eade17
|
|
- A micro Lie theory for state estimation in robotics, Joan Solà, Jérémie Deray, Dinesh Atchuthan @cite Sol2018AML
|
|
*/
|
|
CV_EXPORTS_W void Rodrigues( InputArray src, OutputArray dst, OutputArray jacobian = noArray() );
|
|
|
|
|
|
/** @brief Type of matrix used in LevMarq solver
|
|
|
|
Matrix type can be dense, sparse or chosen automatically based on a matrix size, performance considerations or backend availability.
|
|
|
|
Note: only dense matrix is now supported
|
|
*/
|
|
enum class MatrixType
|
|
{
|
|
AUTO = 0,
|
|
DENSE = 1,
|
|
SPARSE = 2
|
|
};
|
|
|
|
/** @brief Type of variables used in LevMarq solver
|
|
|
|
Variables can be linear, rotation (SO(3) group) or rigid transformation (SE(3) group) with corresponding jacobians and exponential updates.
|
|
|
|
Note: only linear variables are now supported
|
|
*/
|
|
enum class VariableType
|
|
{
|
|
LINEAR = 0,
|
|
SO3 = 1,
|
|
SE3 = 2
|
|
};
|
|
|
|
/** @brief Levenberg-Marquadt solver
|
|
|
|
A Levenberg-Marquadt algorithm locally minimizes an objective function value (aka energy, cost or error) starting from
|
|
current param vector.
|
|
To do that, at each iteration it repeatedly calculates the energy at probe points until it's reduced.
|
|
To calculate a probe point, a linear equation is solved: (J^T*J + lambda*D)*dx = -J^T*b where J is a function jacobian,
|
|
b is a vector of residuals (aka errors or energy terms), D is a diagonal matrix generated from J^T*J diagonal
|
|
and lambda changes for each probe point. Then the resulting dx is "added" to current variable and it forms
|
|
a probe value. "Added" is quoted because in some groups (e.g. SO(3) group) such an increment can be a non-trivial operation.
|
|
|
|
For more details, please refer to Wikipedia page (https://en.wikipedia.org/wiki/Levenberg%E2%80%93Marquardt_algorithm).
|
|
|
|
This solver supports fixed variables and two forms of callback function:
|
|
1. Generating ordinary jacobian J and residual vector err ("long")
|
|
2. Generating normal equation matrix J^T*J and gradient vector J^T*err
|
|
|
|
Currently the solver supports dense jacobian matrix and linear parameter increment.
|
|
*/
|
|
class CV_EXPORTS LevMarq
|
|
{
|
|
public:
|
|
/** @brief Optimization report
|
|
|
|
The structure is returned when optimization is over.
|
|
*/
|
|
struct CV_EXPORTS Report
|
|
{
|
|
Report(bool isFound, int nIters, double finalEnergy) :
|
|
found(isFound), iters(nIters), energy(finalEnergy)
|
|
{ }
|
|
// true if the cost function converged to a local minimum which is checked by check* fields, thresholds and other options
|
|
// false if the cost function failed to converge because of error, amount of iterations exhausted or lambda explosion
|
|
bool found;
|
|
// amount of iterations elapsed until the optimization stopped
|
|
int iters;
|
|
// energy value reached by the optimization
|
|
double energy;
|
|
};
|
|
|
|
/** @brief Structure to keep LevMarq settings
|
|
|
|
The structure allows a user to pass algorithm parameters along with their names like this:
|
|
@code
|
|
MySolver solver(nVars, callback, MySolver::Settings().geodesicS(true).geoScale(1.0));
|
|
@endcode
|
|
*/
|
|
struct CV_EXPORTS Settings
|
|
{
|
|
Settings();
|
|
|
|
inline Settings& setJacobiScaling (bool v) { jacobiScaling = v; return *this; }
|
|
inline Settings& setUpDouble (bool v) { upDouble = v; return *this; }
|
|
inline Settings& setUseStepQuality (bool v) { useStepQuality = v; return *this; }
|
|
inline Settings& setClampDiagonal (bool v) { clampDiagonal = v; return *this; }
|
|
inline Settings& setStepNormInf (bool v) { stepNormInf = v; return *this; }
|
|
inline Settings& setCheckRelEnergyChange (bool v) { checkRelEnergyChange = v; return *this; }
|
|
inline Settings& setCheckMinGradient (bool v) { checkMinGradient = v; return *this; }
|
|
inline Settings& setCheckStepNorm (bool v) { checkStepNorm = v; return *this; }
|
|
inline Settings& setGeodesic (bool v) { geodesic = v; return *this; }
|
|
inline Settings& setHGeo (double v) { hGeo = v; return *this; }
|
|
inline Settings& setGeoScale (double v) { geoScale = v; return *this; }
|
|
inline Settings& setStepNormTolerance (double v) { stepNormTolerance = v; return *this; }
|
|
inline Settings& setRelEnergyDeltaTolerance(double v) { relEnergyDeltaTolerance = v; return *this; }
|
|
inline Settings& setMinGradientTolerance (double v) { minGradientTolerance = v; return *this; }
|
|
inline Settings& setSmallEnergyTolerance (double v) { smallEnergyTolerance = v; return *this; }
|
|
inline Settings& setMaxIterations (int v) { maxIterations = (unsigned int)v; return *this; }
|
|
inline Settings& setInitialLambda (double v) { initialLambda = v; return *this; }
|
|
inline Settings& setInitialLmUpFactor (double v) { initialLmUpFactor = v; return *this; }
|
|
inline Settings& setInitialLmDownFactor (double v) { initialLmDownFactor = v; return *this; }
|
|
|
|
// normalize jacobian columns for better conditioning
|
|
// slows down sparse solver, but maybe this'd be useful for some other solver
|
|
bool jacobiScaling;
|
|
// double upFactor until the probe is successful
|
|
bool upDouble;
|
|
// use stepQuality metrics for steps down
|
|
bool useStepQuality;
|
|
// clamp diagonal values added to J^T*J to pre-defined range of values
|
|
bool clampDiagonal;
|
|
// to use squared L2 norm or Inf norm for step size estimation
|
|
bool stepNormInf;
|
|
// to use relEnergyDeltaTolerance or not
|
|
bool checkRelEnergyChange;
|
|
// to use minGradientTolerance or not
|
|
bool checkMinGradient;
|
|
// to use stepNormTolerance or not
|
|
bool checkStepNorm;
|
|
// to use geodesic acceleration or not
|
|
bool geodesic;
|
|
// second directional derivative approximation step for geodesic acceleration
|
|
double hGeo;
|
|
// how much of geodesic acceleration is used
|
|
double geoScale;
|
|
// optimization stops when norm2(dx) drops below this value
|
|
double stepNormTolerance;
|
|
// optimization stops when relative energy change drops below this value
|
|
double relEnergyDeltaTolerance;
|
|
// optimization stops when max gradient value (J^T*b vector) drops below this value
|
|
double minGradientTolerance;
|
|
// optimization stops when energy drops below this value
|
|
double smallEnergyTolerance;
|
|
// optimization stops after a number of iterations performed
|
|
unsigned int maxIterations;
|
|
|
|
// LevMarq up and down params
|
|
double initialLambda;
|
|
double initialLmUpFactor;
|
|
double initialLmDownFactor;
|
|
};
|
|
|
|
/** "Long" callback: f(param, &err, &J) -> bool
|
|
Computes error and Jacobian for the specified vector of parameters,
|
|
returns true on success.
|
|
|
|
param: the current vector of parameters
|
|
err: output vector of errors: err_i = actual_f_i - ideal_f_i
|
|
J: output Jacobian: J_ij = d(err_i)/d(param_j)
|
|
|
|
Param vector values may be changed by the callback only if they are fixed.
|
|
Changing non-fixed variables may lead to incorrect results.
|
|
When J=noArray(), it means that it does not need to be computed.
|
|
Dimensionality of error vector and param vector can be different.
|
|
The callback should explicitly allocate (with "create" method) each output array
|
|
(unless it's noArray()).
|
|
*/
|
|
typedef std::function<bool(InputOutputArray, OutputArray, OutputArray)> LongCallback;
|
|
|
|
/** Normal callback: f(param, &JtErr, &JtJ, &errnorm) -> bool
|
|
|
|
Computes squared L2 error norm, normal equation matrix J^T*J and J^T*err vector
|
|
where J is MxN Jacobian: J_ij = d(err_i)/d(param_j)
|
|
err is Mx1 vector of errors: err_i = actual_f_i - ideal_f_i
|
|
M is a number of error terms, N is a number of variables to optimize.
|
|
Make sense to use this class instead of usual Callback if the number
|
|
of error terms greatly exceeds the number of variables.
|
|
|
|
param: the current Nx1 vector of parameters
|
|
JtErr: output Nx1 vector J^T*err
|
|
JtJ: output NxN matrix J^T*J
|
|
errnorm: output total error: dot(err, err)
|
|
|
|
Param vector values may be changed by the callback only if they are fixed.
|
|
Changing non-fixed variables may lead to incorrect results.
|
|
If JtErr or JtJ are empty, they don't have to be computed.
|
|
The callback should explicitly allocate (with "create" method) each output array
|
|
(unless it's noArray()).
|
|
*/
|
|
typedef std::function<bool(InputOutputArray, OutputArray, OutputArray, double&)> NormalCallback;
|
|
|
|
/**
|
|
Creates a solver
|
|
|
|
@param nvars Number of variables in a param vector
|
|
@param callback "Long" callback, produces jacobian and residuals for each energy term, returns true on success
|
|
@param settings LevMarq settings structure, see LevMarqBase class for details
|
|
@param mask Indicates what variables are fixed during optimization (zeros) and what vars to optimize (non-zeros)
|
|
@param matrixType Type of matrix used in the solver; only DENSE and AUTO are supported now
|
|
@param paramType Type of optimized parameters; only LINEAR is supported now
|
|
@param nerrs Energy terms amount. If zero, callback-generated jacobian size is used instead
|
|
@param solveMethod What method to use for linear system solving
|
|
*/
|
|
LevMarq(int nvars, LongCallback callback, const Settings& settings = Settings(), InputArray mask = noArray(),
|
|
MatrixType matrixType = MatrixType::AUTO, VariableType paramType = VariableType::LINEAR, int nerrs = 0, int solveMethod = DECOMP_SVD);
|
|
/**
|
|
Creates a solver
|
|
|
|
@param nvars Number of variables in a param vector
|
|
@param callback Normal callback, produces J^T*J and J^T*b directly instead of J and b, returns true on success
|
|
@param settings LevMarq settings structure, see LevMarqBase class for details
|
|
@param mask Indicates what variables are fixed during optimization (zeros) and what vars to optimize (non-zeros)
|
|
@param matrixType Type of matrix used in the solver; only DENSE and AUTO are supported now
|
|
@param paramType Type of optimized parameters; only LINEAR is supported now
|
|
@param LtoR Indicates what part of symmetric matrix to copy to another part: lower or upper. Used only with alt. callback
|
|
@param solveMethod What method to use for linear system solving
|
|
*/
|
|
LevMarq(int nvars, NormalCallback callback, const Settings& settings = Settings(), InputArray mask = noArray(),
|
|
MatrixType matrixType = MatrixType::AUTO, VariableType paramType = VariableType::LINEAR, bool LtoR = false, int solveMethod = DECOMP_SVD);
|
|
|
|
/**
|
|
Creates a solver
|
|
|
|
@param param Input/output vector containing starting param vector and resulting optimized params
|
|
@param callback "Long" callback, produces jacobian and residuals for each energy term, returns true on success
|
|
@param settings LevMarq settings structure, see LevMarqBase class for details
|
|
@param mask Indicates what variables are fixed during optimization (zeros) and what vars to optimize (non-zeros)
|
|
@param matrixType Type of matrix used in the solver; only DENSE and AUTO are supported now
|
|
@param paramType Type of optimized parameters; only LINEAR is supported now
|
|
@param nerrs Energy terms amount. If zero, callback-generated jacobian size is used instead
|
|
@param solveMethod What method to use for linear system solving
|
|
*/
|
|
LevMarq(InputOutputArray param, LongCallback callback, const Settings& settings = Settings(), InputArray mask = noArray(),
|
|
MatrixType matrixType = MatrixType::AUTO, VariableType paramType = VariableType::LINEAR, int nerrs = 0, int solveMethod = DECOMP_SVD);
|
|
/**
|
|
Creates a solver
|
|
|
|
@param param Input/output vector containing starting param vector and resulting optimized params
|
|
@param callback Normal callback, produces J^T*J and J^T*b directly instead of J and b, returns true on success
|
|
@param settings LevMarq settings structure, see LevMarqBase class for details
|
|
@param mask Indicates what variables are fixed during optimization (zeros) and what vars to optimize (non-zeros)
|
|
@param matrixType Type of matrix used in the solver; only DENSE and AUTO are supported now
|
|
@param paramType Type of optimized parameters; only LINEAR is supported now
|
|
@param LtoR Indicates what part of symmetric matrix to copy to another part: lower or upper. Used only with alt. callback
|
|
@param solveMethod What method to use for linear system solving
|
|
*/
|
|
LevMarq(InputOutputArray param, NormalCallback callback, const Settings& settings = Settings(), InputArray mask = noArray(),
|
|
MatrixType matrixType = MatrixType::AUTO, VariableType paramType = VariableType::LINEAR, bool LtoR = false, int solveMethod = DECOMP_SVD);
|
|
|
|
/**
|
|
Runs Levenberg-Marquadt algorithm using current settings and given parameters vector.
|
|
The method returns the optimization report.
|
|
*/
|
|
Report optimize();
|
|
|
|
/** @brief Runs optimization using the passed vector of parameters as the start point.
|
|
|
|
The final vector of parameters (whether the algorithm converged or not) is stored at the same
|
|
vector.
|
|
This method can be used instead of the optimize() method if rerun with different start points is required.
|
|
The method returns the optimization report.
|
|
|
|
@param param initial/final vector of parameters.
|
|
|
|
Note that the dimensionality of parameter space is defined by the size of param vector,
|
|
and the dimensionality of optimized criteria is defined by the size of err vector
|
|
computed by the callback.
|
|
*/
|
|
Report run(InputOutputArray param);
|
|
|
|
private:
|
|
class Impl;
|
|
Ptr<Impl> pImpl;
|
|
};
|
|
|
|
|
|
/** @example samples/cpp/tutorial_code/features2D/Homography/pose_from_homography.cpp
|
|
An example program about pose estimation from coplanar points
|
|
|
|
Check @ref tutorial_homography "the corresponding tutorial" for more details
|
|
*/
|
|
|
|
/** @brief Finds a perspective transformation between two planes.
|
|
|
|
@param srcPoints Coordinates of the points in the original plane, a matrix of the type CV_32FC2
|
|
or vector\<Point2f\> .
|
|
@param dstPoints Coordinates of the points in the target plane, a matrix of the type CV_32FC2 or
|
|
a vector\<Point2f\> .
|
|
@param method Method used to compute a homography matrix. The following methods are possible:
|
|
- **0** - a regular method using all the points, i.e., the least squares method
|
|
- @ref RANSAC - RANSAC-based robust method
|
|
- @ref LMEDS - Least-Median robust method
|
|
- @ref RHO - PROSAC-based robust method
|
|
@param ransacReprojThreshold Maximum allowed reprojection error to treat a point pair as an inlier
|
|
(used in the RANSAC and RHO methods only). That is, if
|
|
\f[\| \texttt{dstPoints} _i - \texttt{convertPointsHomogeneous} ( \texttt{H} * \texttt{srcPoints} _i) \|_2 > \texttt{ransacReprojThreshold}\f]
|
|
then the point \f$i\f$ is considered as an outlier. If srcPoints and dstPoints are measured in pixels,
|
|
it usually makes sense to set this parameter somewhere in the range of 1 to 10.
|
|
@param mask Optional output mask set by a robust method ( RANSAC or LMeDS ). Note that the input
|
|
mask values are ignored.
|
|
@param maxIters The maximum number of RANSAC iterations.
|
|
@param confidence Confidence level, between 0 and 1.
|
|
|
|
The function finds and returns the perspective transformation \f$H\f$ between the source and the
|
|
destination planes:
|
|
|
|
\f[s_i \vecthree{x'_i}{y'_i}{1} \sim H \vecthree{x_i}{y_i}{1}\f]
|
|
|
|
so that the back-projection error
|
|
|
|
\f[\sum _i \left ( x'_i- \frac{h_{11} x_i + h_{12} y_i + h_{13}}{h_{31} x_i + h_{32} y_i + h_{33}} \right )^2+ \left ( y'_i- \frac{h_{21} x_i + h_{22} y_i + h_{23}}{h_{31} x_i + h_{32} y_i + h_{33}} \right )^2\f]
|
|
|
|
is minimized. If the parameter method is set to the default value 0, the function uses all the point
|
|
pairs to compute an initial homography estimate with a simple least-squares scheme.
|
|
|
|
However, if not all of the point pairs ( \f$srcPoints_i\f$, \f$dstPoints_i\f$ ) fit the rigid perspective
|
|
transformation (that is, there are some outliers), this initial estimate will be poor. In this case,
|
|
you can use one of the three robust methods. The methods RANSAC, LMeDS and RHO try many different
|
|
random subsets of the corresponding point pairs (of four pairs each, collinear pairs are discarded), estimate the homography matrix
|
|
using this subset and a simple least-squares algorithm, and then compute the quality/goodness of the
|
|
computed homography (which is the number of inliers for RANSAC or the least median re-projection error for
|
|
LMeDS). The best subset is then used to produce the initial estimate of the homography matrix and
|
|
the mask of inliers/outliers.
|
|
|
|
Regardless of the method, robust or not, the computed homography matrix is refined further (using
|
|
inliers only in case of a robust method) with the Levenberg-Marquardt method to reduce the
|
|
re-projection error even more.
|
|
|
|
The methods RANSAC and RHO can handle practically any ratio of outliers but need a threshold to
|
|
distinguish inliers from outliers. The method LMeDS does not need any threshold but it works
|
|
correctly only when there are more than 50% of inliers. Finally, if there are no outliers and the
|
|
noise is rather small, use the default method (method=0).
|
|
|
|
The function is used to find initial intrinsic and extrinsic matrices. Homography matrix is
|
|
determined up to a scale. Thus, it is normalized so that \f$h_{33}=1\f$. Note that whenever an \f$H\f$ matrix
|
|
cannot be estimated, an empty one will be returned.
|
|
|
|
@sa
|
|
getAffineTransform, estimateAffine2D, estimateAffinePartial2D, getPerspectiveTransform, warpPerspective,
|
|
perspectiveTransform
|
|
*/
|
|
CV_EXPORTS_W Mat findHomography( InputArray srcPoints, InputArray dstPoints,
|
|
int method = 0, double ransacReprojThreshold = 3,
|
|
OutputArray mask=noArray(), const int maxIters = 2000,
|
|
const double confidence = 0.995);
|
|
|
|
/** @overload */
|
|
CV_EXPORTS Mat findHomography( InputArray srcPoints, InputArray dstPoints,
|
|
OutputArray mask, int method = 0, double ransacReprojThreshold = 3 );
|
|
|
|
|
|
CV_EXPORTS_W Mat findHomography(InputArray srcPoints, InputArray dstPoints, OutputArray mask,
|
|
const UsacParams ¶ms);
|
|
|
|
/** @brief Computes an RQ decomposition of 3x3 matrices.
|
|
|
|
@param src 3x3 input matrix.
|
|
@param mtxR Output 3x3 upper-triangular matrix.
|
|
@param mtxQ Output 3x3 orthogonal matrix.
|
|
@param Qx Optional output 3x3 rotation matrix around x-axis.
|
|
@param Qy Optional output 3x3 rotation matrix around y-axis.
|
|
@param Qz Optional output 3x3 rotation matrix around z-axis.
|
|
|
|
The function computes a RQ decomposition using the given rotations. This function is used in
|
|
#decomposeProjectionMatrix to decompose the left 3x3 submatrix of a projection matrix into a camera
|
|
and a rotation matrix.
|
|
|
|
It optionally returns three rotation matrices, one for each axis, and the three Euler angles in
|
|
degrees (as the return value) that could be used in OpenGL. Note, there is always more than one
|
|
sequence of rotations about the three principal axes that results in the same orientation of an
|
|
object, e.g. see @cite Slabaugh . Returned tree rotation matrices and corresponding three Euler angles
|
|
are only one of the possible solutions.
|
|
*/
|
|
CV_EXPORTS_W Vec3d RQDecomp3x3( InputArray src, OutputArray mtxR, OutputArray mtxQ,
|
|
OutputArray Qx = noArray(),
|
|
OutputArray Qy = noArray(),
|
|
OutputArray Qz = noArray());
|
|
|
|
/** @brief Decomposes a projection matrix into a rotation matrix and a camera intrinsic matrix.
|
|
|
|
@param projMatrix 3x4 input projection matrix P.
|
|
@param cameraMatrix Output 3x3 camera intrinsic matrix \f$\cameramatrix{A}\f$.
|
|
@param rotMatrix Output 3x3 external rotation matrix R.
|
|
@param transVect Output 4x1 translation vector T.
|
|
@param rotMatrixX Optional 3x3 rotation matrix around x-axis.
|
|
@param rotMatrixY Optional 3x3 rotation matrix around y-axis.
|
|
@param rotMatrixZ Optional 3x3 rotation matrix around z-axis.
|
|
@param eulerAngles Optional three-element vector containing three Euler angles of rotation in
|
|
degrees.
|
|
|
|
The function computes a decomposition of a projection matrix into a calibration and a rotation
|
|
matrix and the position of a camera.
|
|
|
|
It optionally returns three rotation matrices, one for each axis, and three Euler angles that could
|
|
be used in OpenGL. Note, there is always more than one sequence of rotations about the three
|
|
principal axes that results in the same orientation of an object, e.g. see @cite Slabaugh . Returned
|
|
tree rotation matrices and corresponding three Euler angles are only one of the possible solutions.
|
|
|
|
The function is based on RQDecomp3x3 .
|
|
*/
|
|
CV_EXPORTS_W void decomposeProjectionMatrix( InputArray projMatrix, OutputArray cameraMatrix,
|
|
OutputArray rotMatrix, OutputArray transVect,
|
|
OutputArray rotMatrixX = noArray(),
|
|
OutputArray rotMatrixY = noArray(),
|
|
OutputArray rotMatrixZ = noArray(),
|
|
OutputArray eulerAngles =noArray() );
|
|
|
|
/** @brief Computes partial derivatives of the matrix product for each multiplied matrix.
|
|
|
|
@param A First multiplied matrix.
|
|
@param B Second multiplied matrix.
|
|
@param dABdA First output derivative matrix d(A\*B)/dA of size
|
|
\f$\texttt{A.rows*B.cols} \times {A.rows*A.cols}\f$ .
|
|
@param dABdB Second output derivative matrix d(A\*B)/dB of size
|
|
\f$\texttt{A.rows*B.cols} \times {B.rows*B.cols}\f$ .
|
|
|
|
The function computes partial derivatives of the elements of the matrix product \f$A*B\f$ with regard to
|
|
the elements of each of the two input matrices. The function is used to compute the Jacobian
|
|
matrices in #stereoCalibrate but can also be used in any other similar optimization function.
|
|
*/
|
|
CV_EXPORTS_W void matMulDeriv( InputArray A, InputArray B, OutputArray dABdA, OutputArray dABdB );
|
|
|
|
/** @brief Combines two rotation-and-shift transformations.
|
|
|
|
@param rvec1 First rotation vector.
|
|
@param tvec1 First translation vector.
|
|
@param rvec2 Second rotation vector.
|
|
@param tvec2 Second translation vector.
|
|
@param rvec3 Output rotation vector of the superposition.
|
|
@param tvec3 Output translation vector of the superposition.
|
|
@param dr3dr1 Optional output derivative of rvec3 with regard to rvec1
|
|
@param dr3dt1 Optional output derivative of rvec3 with regard to tvec1
|
|
@param dr3dr2 Optional output derivative of rvec3 with regard to rvec2
|
|
@param dr3dt2 Optional output derivative of rvec3 with regard to tvec2
|
|
@param dt3dr1 Optional output derivative of tvec3 with regard to rvec1
|
|
@param dt3dt1 Optional output derivative of tvec3 with regard to tvec1
|
|
@param dt3dr2 Optional output derivative of tvec3 with regard to rvec2
|
|
@param dt3dt2 Optional output derivative of tvec3 with regard to tvec2
|
|
|
|
The functions compute:
|
|
|
|
\f[\begin{array}{l} \texttt{rvec3} = \mathrm{rodrigues} ^{-1} \left ( \mathrm{rodrigues} ( \texttt{rvec2} ) \cdot \mathrm{rodrigues} ( \texttt{rvec1} ) \right ) \\ \texttt{tvec3} = \mathrm{rodrigues} ( \texttt{rvec2} ) \cdot \texttt{tvec1} + \texttt{tvec2} \end{array} ,\f]
|
|
|
|
where \f$\mathrm{rodrigues}\f$ denotes a rotation vector to a rotation matrix transformation, and
|
|
\f$\mathrm{rodrigues}^{-1}\f$ denotes the inverse transformation. See Rodrigues for details.
|
|
|
|
Also, the functions can compute the derivatives of the output vectors with regards to the input
|
|
vectors (see matMulDeriv ). The functions are used inside #stereoCalibrate but can also be used in
|
|
your own code where Levenberg-Marquardt or another gradient-based solver is used to optimize a
|
|
function that contains a matrix multiplication.
|
|
*/
|
|
CV_EXPORTS_W void composeRT( InputArray rvec1, InputArray tvec1,
|
|
InputArray rvec2, InputArray tvec2,
|
|
OutputArray rvec3, OutputArray tvec3,
|
|
OutputArray dr3dr1 = noArray(), OutputArray dr3dt1 = noArray(),
|
|
OutputArray dr3dr2 = noArray(), OutputArray dr3dt2 = noArray(),
|
|
OutputArray dt3dr1 = noArray(), OutputArray dt3dt1 = noArray(),
|
|
OutputArray dt3dr2 = noArray(), OutputArray dt3dt2 = noArray() );
|
|
|
|
/** @brief Projects 3D points to an image plane.
|
|
|
|
@param objectPoints Array of object points expressed wrt. the world coordinate frame. A 3xN/Nx3
|
|
1-channel or 1xN/Nx1 3-channel (or vector\<Point3f\> ), where N is the number of points in the view.
|
|
@param rvec The rotation vector (@ref Rodrigues) that, together with tvec, performs a change of
|
|
basis from world to camera coordinate system, see @ref calibrateCamera for details.
|
|
@param tvec The translation vector, see parameter description above.
|
|
@param cameraMatrix Camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$ . If the vector is empty, the zero distortion coefficients are assumed.
|
|
@param imagePoints Output array of image points, 1xN/Nx1 2-channel, or
|
|
vector\<Point2f\> .
|
|
@param jacobian Optional output 2Nx(10+\<numDistCoeffs\>) jacobian matrix of derivatives of image
|
|
points with respect to components of the rotation vector, translation vector, focal lengths,
|
|
coordinates of the principal point and the distortion coefficients. In the old interface different
|
|
components of the jacobian are returned via different output parameters.
|
|
@param aspectRatio Optional "fixed aspect ratio" parameter. If the parameter is not 0, the
|
|
function assumes that the aspect ratio (\f$f_x / f_y\f$) is fixed and correspondingly adjusts the
|
|
jacobian matrix.
|
|
|
|
The function computes the 2D projections of 3D points to the image plane, given intrinsic and
|
|
extrinsic camera parameters. Optionally, the function computes Jacobians -matrices of partial
|
|
derivatives of image points coordinates (as functions of all the input parameters) with respect to
|
|
the particular parameters, intrinsic and/or extrinsic. The Jacobians are used during the global
|
|
optimization in @ref calibrateCamera, @ref solvePnP, and @ref stereoCalibrate. The function itself
|
|
can also be used to compute a re-projection error, given the current intrinsic and extrinsic
|
|
parameters.
|
|
|
|
@note By setting rvec = tvec = \f$[0, 0, 0]\f$, or by setting cameraMatrix to a 3x3 identity matrix,
|
|
or by passing zero distortion coefficients, one can get various useful partial cases of the
|
|
function. This means, one can compute the distorted coordinates for a sparse set of points or apply
|
|
a perspective transformation (and also compute the derivatives) in the ideal zero-distortion setup.
|
|
*/
|
|
CV_EXPORTS_W void projectPoints( InputArray objectPoints,
|
|
InputArray rvec, InputArray tvec,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArray imagePoints,
|
|
OutputArray jacobian = noArray(),
|
|
double aspectRatio = 0);
|
|
|
|
/** @overload */
|
|
CV_EXPORTS_AS(projectPointsSepJ) void projectPoints(
|
|
InputArray objectPoints,
|
|
InputArray rvec, InputArray tvec,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArray imagePoints, OutputArray dpdr,
|
|
OutputArray dpdt, OutputArray dpdf=noArray(),
|
|
OutputArray dpdc=noArray(), OutputArray dpdk=noArray(),
|
|
OutputArray dpdo=noArray(), double aspectRatio=0.);
|
|
|
|
/** @example samples/cpp/tutorial_code/features2D/Homography/homography_from_camera_displacement.cpp
|
|
An example program about homography from the camera displacement
|
|
|
|
Check @ref tutorial_homography "the corresponding tutorial" for more details
|
|
*/
|
|
|
|
/** @brief Finds an object pose from 3D-2D point correspondences.
|
|
|
|
@see @ref calib3d_solvePnP
|
|
|
|
This function returns the rotation and the translation vectors that transform a 3D point expressed in the object
|
|
coordinate frame to the camera coordinate frame, using different methods:
|
|
- P3P methods (@ref SOLVEPNP_P3P, @ref SOLVEPNP_AP3P): need 4 input points to return a unique solution.
|
|
- @ref SOLVEPNP_IPPE Input points must be >= 4 and object points must be coplanar.
|
|
- @ref SOLVEPNP_IPPE_SQUARE Special case suitable for marker pose estimation.
|
|
Number of input points must be 4. Object points must be defined in the following order:
|
|
- point 0: [-squareLength / 2, squareLength / 2, 0]
|
|
- point 1: [ squareLength / 2, squareLength / 2, 0]
|
|
- point 2: [ squareLength / 2, -squareLength / 2, 0]
|
|
- point 3: [-squareLength / 2, -squareLength / 2, 0]
|
|
- for all the other flags, number of input points must be >= 4 and object points can be in any configuration.
|
|
|
|
@param objectPoints Array of object points in the object coordinate space, Nx3 1-channel or
|
|
1xN/Nx1 3-channel, where N is the number of points. vector\<Point3d\> can be also passed here.
|
|
@param imagePoints Array of corresponding image points, Nx2 1-channel or 1xN/Nx1 2-channel,
|
|
where N is the number of points. vector\<Point2d\> can be also passed here.
|
|
@param cameraMatrix Input camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param rvec Output rotation vector (see @ref Rodrigues ) that, together with tvec, brings points from
|
|
the model coordinate system to the camera coordinate system.
|
|
@param tvec Output translation vector.
|
|
@param useExtrinsicGuess Parameter used for #SOLVEPNP_ITERATIVE. If true (1), the function uses
|
|
the provided rvec and tvec values as initial approximations of the rotation and translation
|
|
vectors, respectively, and further optimizes them.
|
|
@param flags Method for solving a PnP problem: see @ref calib3d_solvePnP_flags
|
|
|
|
More information about Perspective-n-Points is described in @ref calib3d_solvePnP
|
|
|
|
@note
|
|
- An example of how to use solvePnP for planar augmented reality can be found at
|
|
opencv_source_code/samples/python/plane_ar.py
|
|
- If you are using Python:
|
|
- Numpy array slices won't work as input because solvePnP requires contiguous
|
|
arrays (enforced by the assertion using cv::Mat::checkVector() around line 55 of
|
|
modules/3d/src/solvepnp.cpp version 2.4.9)
|
|
- The P3P algorithm requires image points to be in an array of shape (N,1,2) due
|
|
to its calling of #undistortPoints (around line 75 of modules/3d/src/solvepnp.cpp version 2.4.9)
|
|
which requires 2-channel information.
|
|
- Thus, given some data D = np.array(...) where D.shape = (N,M), in order to use a subset of
|
|
it as, e.g., imagePoints, one must effectively copy it into a new array: imagePoints =
|
|
np.ascontiguousarray(D[:,:2]).reshape((N,1,2))
|
|
- The methods @ref SOLVEPNP_DLS and @ref SOLVEPNP_UPNP cannot be used as the current implementations are
|
|
unstable and sometimes give completely wrong results. If you pass one of these two
|
|
flags, @ref SOLVEPNP_EPNP method will be used instead.
|
|
- The minimum number of points is 4 in the general case. In the case of @ref SOLVEPNP_P3P and @ref SOLVEPNP_AP3P
|
|
methods, it is required to use exactly 4 points (the first 3 points are used to estimate all the solutions
|
|
of the P3P problem, the last one is used to retain the best solution that minimizes the reprojection error).
|
|
- With @ref SOLVEPNP_ITERATIVE method and `useExtrinsicGuess=true`, the minimum number of points is 3 (3 points
|
|
are sufficient to compute a pose but there are up to 4 solutions). The initial solution should be close to the
|
|
global solution to converge.
|
|
- With @ref SOLVEPNP_IPPE input points must be >= 4 and object points must be coplanar.
|
|
- With @ref SOLVEPNP_IPPE_SQUARE this is a special case suitable for marker pose estimation.
|
|
Number of input points must be 4. Object points must be defined in the following order:
|
|
- point 0: [-squareLength / 2, squareLength / 2, 0]
|
|
- point 1: [ squareLength / 2, squareLength / 2, 0]
|
|
- point 2: [ squareLength / 2, -squareLength / 2, 0]
|
|
- point 3: [-squareLength / 2, -squareLength / 2, 0]
|
|
- With @ref SOLVEPNP_SQPNP input points must be >= 3
|
|
*/
|
|
CV_EXPORTS_W bool solvePnP( InputArray objectPoints, InputArray imagePoints,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArray rvec, OutputArray tvec,
|
|
bool useExtrinsicGuess = false, int flags = SOLVEPNP_ITERATIVE );
|
|
|
|
/** @brief Finds an object pose from 3D-2D point correspondences using the RANSAC scheme.
|
|
|
|
@see @ref calib3d_solvePnP
|
|
|
|
@param objectPoints Array of object points in the object coordinate space, Nx3 1-channel or
|
|
1xN/Nx1 3-channel, where N is the number of points. vector\<Point3d\> can be also passed here.
|
|
@param imagePoints Array of corresponding image points, Nx2 1-channel or 1xN/Nx1 2-channel,
|
|
where N is the number of points. vector\<Point2d\> can be also passed here.
|
|
@param cameraMatrix Input camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param rvec Output rotation vector (see @ref Rodrigues ) that, together with tvec, brings points from
|
|
the model coordinate system to the camera coordinate system.
|
|
@param tvec Output translation vector.
|
|
@param useExtrinsicGuess Parameter used for @ref SOLVEPNP_ITERATIVE. If true (1), the function uses
|
|
the provided rvec and tvec values as initial approximations of the rotation and translation
|
|
vectors, respectively, and further optimizes them.
|
|
@param iterationsCount Number of iterations.
|
|
@param reprojectionError Inlier threshold value used by the RANSAC procedure. The parameter value
|
|
is the maximum allowed distance between the observed and computed point projections to consider it
|
|
an inlier.
|
|
@param confidence The probability that the algorithm produces a useful result.
|
|
@param inliers Output vector that contains indices of inliers in objectPoints and imagePoints .
|
|
@param flags Method for solving a PnP problem (see @ref solvePnP ).
|
|
|
|
The function estimates an object pose given a set of object points, their corresponding image
|
|
projections, as well as the camera intrinsic matrix and the distortion coefficients. This function finds such
|
|
a pose that minimizes reprojection error, that is, the sum of squared distances between the observed
|
|
projections imagePoints and the projected (using @ref projectPoints ) objectPoints. The use of RANSAC
|
|
makes the function resistant to outliers.
|
|
|
|
@note
|
|
- An example of how to use solvePNPRansac for object detection can be found at
|
|
opencv_source_code/samples/cpp/tutorial_code/3d/real_time_pose_estimation/
|
|
- The default method used to estimate the camera pose for the Minimal Sample Sets step
|
|
is #SOLVEPNP_EPNP. Exceptions are:
|
|
- if you choose #SOLVEPNP_P3P or #SOLVEPNP_AP3P, these methods will be used.
|
|
- if the number of input points is equal to 4, #SOLVEPNP_P3P is used.
|
|
- The method used to estimate the camera pose using all the inliers is defined by the
|
|
flags parameters unless it is equal to #SOLVEPNP_P3P or #SOLVEPNP_AP3P. In this case,
|
|
the method #SOLVEPNP_EPNP will be used instead.
|
|
*/
|
|
CV_EXPORTS_W bool solvePnPRansac( InputArray objectPoints, InputArray imagePoints,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArray rvec, OutputArray tvec,
|
|
bool useExtrinsicGuess = false, int iterationsCount = 100,
|
|
float reprojectionError = 8.0, double confidence = 0.99,
|
|
OutputArray inliers = noArray(), int flags = SOLVEPNP_ITERATIVE );
|
|
|
|
/*
|
|
Finds rotation and translation vector.
|
|
If cameraMatrix is given then run P3P. Otherwise run linear P6P and output cameraMatrix too.
|
|
*/
|
|
CV_EXPORTS_W bool solvePnPRansac( InputArray objectPoints, InputArray imagePoints,
|
|
InputOutputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArray rvec, OutputArray tvec, OutputArray inliers,
|
|
const UsacParams ¶ms=UsacParams());
|
|
|
|
/** @brief Finds an object pose from 3 3D-2D point correspondences.
|
|
|
|
@see @ref calib3d_solvePnP
|
|
|
|
@param objectPoints Array of object points in the object coordinate space, 3x3 1-channel or
|
|
1x3/3x1 3-channel. vector\<Point3f\> can be also passed here.
|
|
@param imagePoints Array of corresponding image points, 3x2 1-channel or 1x3/3x1 2-channel.
|
|
vector\<Point2f\> can be also passed here.
|
|
@param cameraMatrix Input camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param rvecs Output rotation vectors (see @ref Rodrigues ) that, together with tvecs, brings points from
|
|
the model coordinate system to the camera coordinate system. A P3P problem has up to 4 solutions.
|
|
@param tvecs Output translation vectors.
|
|
@param flags Method for solving a P3P problem:
|
|
- @ref SOLVEPNP_P3P Method is based on the paper of X.S. Gao, X.-R. Hou, J. Tang, H.-F. Chang
|
|
"Complete Solution Classification for the Perspective-Three-Point Problem" (@cite gao2003complete).
|
|
- @ref SOLVEPNP_AP3P Method is based on the paper of T. Ke and S. Roumeliotis.
|
|
"An Efficient Algebraic Solution to the Perspective-Three-Point Problem" (@cite Ke17).
|
|
|
|
The function estimates the object pose given 3 object points, their corresponding image
|
|
projections, as well as the camera intrinsic matrix and the distortion coefficients.
|
|
|
|
@note
|
|
The solutions are sorted by reprojection errors (lowest to highest).
|
|
*/
|
|
CV_EXPORTS_W int solveP3P( InputArray objectPoints, InputArray imagePoints,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArrayOfArrays rvecs, OutputArrayOfArrays tvecs,
|
|
int flags );
|
|
|
|
/** @brief Refine a pose (the translation and the rotation that transform a 3D point expressed in the object coordinate frame
|
|
to the camera coordinate frame) from a 3D-2D point correspondences and starting from an initial solution.
|
|
|
|
@see @ref calib3d_solvePnP
|
|
|
|
@param objectPoints Array of object points in the object coordinate space, Nx3 1-channel or 1xN/Nx1 3-channel,
|
|
where N is the number of points. vector\<Point3d\> can also be passed here.
|
|
@param imagePoints Array of corresponding image points, Nx2 1-channel or 1xN/Nx1 2-channel,
|
|
where N is the number of points. vector\<Point2d\> can also be passed here.
|
|
@param cameraMatrix Input camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param rvec Input/Output rotation vector (see @ref Rodrigues ) that, together with tvec, brings points from
|
|
the model coordinate system to the camera coordinate system. Input values are used as an initial solution.
|
|
@param tvec Input/Output translation vector. Input values are used as an initial solution.
|
|
@param criteria Criteria when to stop the Levenberg-Marquard iterative algorithm.
|
|
|
|
The function refines the object pose given at least 3 object points, their corresponding image
|
|
projections, an initial solution for the rotation and translation vector,
|
|
as well as the camera intrinsic matrix and the distortion coefficients.
|
|
The function minimizes the projection error with respect to the rotation and the translation vectors, according
|
|
to a Levenberg-Marquardt iterative minimization @cite Madsen04 @cite Eade13 process.
|
|
*/
|
|
CV_EXPORTS_W void solvePnPRefineLM( InputArray objectPoints, InputArray imagePoints,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputOutputArray rvec, InputOutputArray tvec,
|
|
TermCriteria criteria = TermCriteria(TermCriteria::EPS +
|
|
TermCriteria::COUNT, 20, FLT_EPSILON));
|
|
|
|
/** @brief Refine a pose (the translation and the rotation that transform a 3D point expressed in the object coordinate frame
|
|
to the camera coordinate frame) from a 3D-2D point correspondences and starting from an initial solution.
|
|
|
|
@see @ref calib3d_solvePnP
|
|
|
|
@param objectPoints Array of object points in the object coordinate space, Nx3 1-channel or 1xN/Nx1 3-channel,
|
|
where N is the number of points. vector\<Point3d\> can also be passed here.
|
|
@param imagePoints Array of corresponding image points, Nx2 1-channel or 1xN/Nx1 2-channel,
|
|
where N is the number of points. vector\<Point2d\> can also be passed here.
|
|
@param cameraMatrix Input camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param rvec Input/Output rotation vector (see @ref Rodrigues ) that, together with tvec, brings points from
|
|
the model coordinate system to the camera coordinate system. Input values are used as an initial solution.
|
|
@param tvec Input/Output translation vector. Input values are used as an initial solution.
|
|
@param criteria Criteria when to stop the Levenberg-Marquard iterative algorithm.
|
|
@param VVSlambda Gain for the virtual visual servoing control law, equivalent to the \f$\alpha\f$
|
|
gain in the Damped Gauss-Newton formulation.
|
|
|
|
The function refines the object pose given at least 3 object points, their corresponding image
|
|
projections, an initial solution for the rotation and translation vector,
|
|
as well as the camera intrinsic matrix and the distortion coefficients.
|
|
The function minimizes the projection error with respect to the rotation and the translation vectors, using a
|
|
virtual visual servoing (VVS) @cite Chaumette06 @cite Marchand16 scheme.
|
|
*/
|
|
CV_EXPORTS_W void solvePnPRefineVVS( InputArray objectPoints, InputArray imagePoints,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputOutputArray rvec, InputOutputArray tvec,
|
|
TermCriteria criteria = TermCriteria(TermCriteria::EPS +
|
|
TermCriteria::COUNT, 20, FLT_EPSILON),
|
|
double VVSlambda = 1);
|
|
|
|
/** @brief Finds an object pose from 3D-2D point correspondences.
|
|
|
|
@see @ref calib3d_solvePnP
|
|
|
|
This function returns a list of all the possible solutions (a solution is a <rotation vector, translation vector>
|
|
couple), depending on the number of input points and the chosen method:
|
|
- P3P methods (@ref SOLVEPNP_P3P, @ref SOLVEPNP_AP3P): 3 or 4 input points. Number of returned solutions can be between 0 and 4 with 3 input points.
|
|
- @ref SOLVEPNP_IPPE Input points must be >= 4 and object points must be coplanar. Returns 2 solutions.
|
|
- @ref SOLVEPNP_IPPE_SQUARE Special case suitable for marker pose estimation.
|
|
Number of input points must be 4 and 2 solutions are returned. Object points must be defined in the following order:
|
|
- point 0: [-squareLength / 2, squareLength / 2, 0]
|
|
- point 1: [ squareLength / 2, squareLength / 2, 0]
|
|
- point 2: [ squareLength / 2, -squareLength / 2, 0]
|
|
- point 3: [-squareLength / 2, -squareLength / 2, 0]
|
|
- for all the other flags, number of input points must be >= 4 and object points can be in any configuration.
|
|
Only 1 solution is returned.
|
|
|
|
@param objectPoints Array of object points in the object coordinate space, Nx3 1-channel or
|
|
1xN/Nx1 3-channel, where N is the number of points. vector\<Point3d\> can be also passed here.
|
|
@param imagePoints Array of corresponding image points, Nx2 1-channel or 1xN/Nx1 2-channel,
|
|
where N is the number of points. vector\<Point2d\> can be also passed here.
|
|
@param cameraMatrix Input camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param rvecs Vector of output rotation vectors (see @ref Rodrigues ) that, together with tvecs, brings points from
|
|
the model coordinate system to the camera coordinate system.
|
|
@param tvecs Vector of output translation vectors.
|
|
@param useExtrinsicGuess Parameter used for #SOLVEPNP_ITERATIVE. If true (1), the function uses
|
|
the provided rvec and tvec values as initial approximations of the rotation and translation
|
|
vectors, respectively, and further optimizes them.
|
|
@param flags Method for solving a PnP problem: see @ref calib3d_solvePnP_flags
|
|
@param rvec Rotation vector used to initialize an iterative PnP refinement algorithm, when flag is @ref SOLVEPNP_ITERATIVE
|
|
and useExtrinsicGuess is set to true.
|
|
@param tvec Translation vector used to initialize an iterative PnP refinement algorithm, when flag is @ref SOLVEPNP_ITERATIVE
|
|
and useExtrinsicGuess is set to true.
|
|
@param reprojectionError Optional vector of reprojection error, that is the RMS error
|
|
(\f$ \text{RMSE} = \sqrt{\frac{\sum_{i}^{N} \left ( \hat{y_i} - y_i \right )^2}{N}} \f$) between the input image points
|
|
and the 3D object points projected with the estimated pose.
|
|
|
|
More information is described in @ref calib3d_solvePnP
|
|
|
|
@note
|
|
- An example of how to use solvePnP for planar augmented reality can be found at
|
|
opencv_source_code/samples/python/plane_ar.py
|
|
- If you are using Python:
|
|
- Numpy array slices won't work as input because solvePnP requires contiguous
|
|
arrays (enforced by the assertion using cv::Mat::checkVector() around line 55 of
|
|
modules/3d/src/solvepnp.cpp version 2.4.9)
|
|
- The P3P algorithm requires image points to be in an array of shape (N,1,2) due
|
|
to its calling of #undistortPoints (around line 75 of modules/3d/src/solvepnp.cpp version 2.4.9)
|
|
which requires 2-channel information.
|
|
- Thus, given some data D = np.array(...) where D.shape = (N,M), in order to use a subset of
|
|
it as, e.g., imagePoints, one must effectively copy it into a new array: imagePoints =
|
|
np.ascontiguousarray(D[:,:2]).reshape((N,1,2))
|
|
- The methods @ref SOLVEPNP_DLS and @ref SOLVEPNP_UPNP cannot be used as the current implementations are
|
|
unstable and sometimes give completely wrong results. If you pass one of these two
|
|
flags, @ref SOLVEPNP_EPNP method will be used instead.
|
|
- The minimum number of points is 4 in the general case. In the case of @ref SOLVEPNP_P3P and @ref SOLVEPNP_AP3P
|
|
methods, it is required to use exactly 4 points (the first 3 points are used to estimate all the solutions
|
|
of the P3P problem, the last one is used to retain the best solution that minimizes the reprojection error).
|
|
- With @ref SOLVEPNP_ITERATIVE method and `useExtrinsicGuess=true`, the minimum number of points is 3 (3 points
|
|
are sufficient to compute a pose but there are up to 4 solutions). The initial solution should be close to the
|
|
global solution to converge.
|
|
- With @ref SOLVEPNP_IPPE input points must be >= 4 and object points must be coplanar.
|
|
- With @ref SOLVEPNP_IPPE_SQUARE this is a special case suitable for marker pose estimation.
|
|
Number of input points must be 4. Object points must be defined in the following order:
|
|
- point 0: [-squareLength / 2, squareLength / 2, 0]
|
|
- point 1: [ squareLength / 2, squareLength / 2, 0]
|
|
- point 2: [ squareLength / 2, -squareLength / 2, 0]
|
|
- point 3: [-squareLength / 2, -squareLength / 2, 0]
|
|
*/
|
|
CV_EXPORTS_W int solvePnPGeneric( InputArray objectPoints, InputArray imagePoints,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
OutputArrayOfArrays rvecs, OutputArrayOfArrays tvecs,
|
|
bool useExtrinsicGuess = false,
|
|
int flags = SOLVEPNP_ITERATIVE,
|
|
InputArray rvec = noArray(), InputArray tvec = noArray(),
|
|
OutputArray reprojectionError = noArray() );
|
|
|
|
/** @brief Draw axes of the world/object coordinate system from pose estimation. @sa solvePnP
|
|
|
|
@param image Input/output image. It must have 1 or 3 channels. The number of channels is not altered.
|
|
@param cameraMatrix Input 3x3 floating-point matrix of camera intrinsic parameters.
|
|
\f$\cameramatrix{A}\f$
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is empty, the zero distortion coefficients are assumed.
|
|
@param rvec Rotation vector (see @ref Rodrigues ) that, together with tvec, brings points from
|
|
the model coordinate system to the camera coordinate system.
|
|
@param tvec Translation vector.
|
|
@param length Length of the painted axes in the same unit than tvec (usually in meters).
|
|
@param thickness Line thickness of the painted axes.
|
|
|
|
This function draws the axes of the world/object coordinate system w.r.t. to the camera frame.
|
|
OX is drawn in red, OY in green and OZ in blue.
|
|
*/
|
|
CV_EXPORTS_W void drawFrameAxes(InputOutputArray image, InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputArray rvec, InputArray tvec, float length, int thickness=3);
|
|
|
|
/** @brief Converts points from Euclidean to homogeneous space.
|
|
|
|
@param src Input vector of N-dimensional points.
|
|
@param dst Output vector of N+1-dimensional points.
|
|
@param dtype The desired output array depth (either CV_32F or CV_64F are currently supported).
|
|
If it's -1, then it's set automatically to CV_32F or CV_64F, depending on the input depth.
|
|
|
|
The function converts points from Euclidean to homogeneous space by appending 1's to the tuple of
|
|
point coordinates. That is, each point (x1, x2, ..., xn) is converted to (x1, x2, ..., xn, 1).
|
|
*/
|
|
CV_EXPORTS_W void convertPointsToHomogeneous( InputArray src, OutputArray dst, int dtype=-1 );
|
|
|
|
/** @brief Converts points from homogeneous to Euclidean space.
|
|
|
|
@param src Input vector of N-dimensional points.
|
|
@param dst Output vector of N-1-dimensional points.
|
|
@param dtype The desired output array depth (either CV_32F or CV_64F are currently supported).
|
|
If it's -1, then it's set automatically to CV_32F or CV_64F, depending on the input depth.
|
|
|
|
The function converts points homogeneous to Euclidean space using perspective projection. That is,
|
|
each point (x1, x2, ... x(n-1), xn) is converted to (x1/xn, x2/xn, ..., x(n-1)/xn). When xn=0, the
|
|
output point coordinates will be (0,0,0,...).
|
|
*/
|
|
CV_EXPORTS_W void convertPointsFromHomogeneous( InputArray src, OutputArray dst, int dtype=-1 );
|
|
|
|
/** @brief Converts points to/from homogeneous coordinates.
|
|
|
|
@param src Input array or vector of 2D, 3D, or 4D points.
|
|
@param dst Output vector of 2D, 3D, or 4D points.
|
|
|
|
The function converts 2D or 3D points from/to homogeneous coordinates by calling either
|
|
#convertPointsToHomogeneous or #convertPointsFromHomogeneous.
|
|
|
|
@note The function is obsolete. Use one of the previous two functions instead.
|
|
*/
|
|
CV_EXPORTS void convertPointsHomogeneous( InputArray src, OutputArray dst );
|
|
|
|
/** @brief Calculates a fundamental matrix from the corresponding points in two images.
|
|
|
|
@param points1 Array of N points from the first image. The point coordinates should be
|
|
floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param method Method for computing a fundamental matrix.
|
|
- @ref FM_7POINT for a 7-point algorithm. \f$N = 7\f$
|
|
- @ref FM_8POINT for an 8-point algorithm. \f$N \ge 8\f$
|
|
- @ref FM_RANSAC for the RANSAC algorithm. \f$N \ge 8\f$
|
|
- @ref FM_LMEDS for the LMedS algorithm. \f$N \ge 8\f$
|
|
@param ransacReprojThreshold Parameter used only for RANSAC. It is the maximum distance from a point to an epipolar
|
|
line in pixels, beyond which the point is considered an outlier and is not used for computing the
|
|
final fundamental matrix. It can be set to something like 1-3, depending on the accuracy of the
|
|
point localization, image resolution, and the image noise.
|
|
@param confidence Parameter used for the RANSAC and LMedS methods only. It specifies a desirable level
|
|
of confidence (probability) that the estimated matrix is correct.
|
|
@param[out] mask optional output mask
|
|
@param maxIters The maximum number of robust method iterations.
|
|
|
|
The epipolar geometry is described by the following equation:
|
|
|
|
\f[[p_2; 1]^T F [p_1; 1] = 0\f]
|
|
|
|
where \f$F\f$ is a fundamental matrix, \f$p_1\f$ and \f$p_2\f$ are corresponding points in the first and the
|
|
second images, respectively.
|
|
|
|
The function calculates the fundamental matrix using one of four methods listed above and returns
|
|
the found fundamental matrix. Normally just one matrix is found. But in case of the 7-point
|
|
algorithm, the function may return up to 3 solutions ( \f$9 \times 3\f$ matrix that stores all 3
|
|
matrices sequentially).
|
|
|
|
The calculated fundamental matrix may be passed further to computeCorrespondEpilines that finds the
|
|
epipolar lines corresponding to the specified points. It can also be passed to
|
|
#stereoRectifyUncalibrated to compute the rectification transformation. :
|
|
@code
|
|
// Example. Estimation of fundamental matrix using the RANSAC algorithm
|
|
int point_count = 100;
|
|
vector<Point2f> points1(point_count);
|
|
vector<Point2f> points2(point_count);
|
|
|
|
// initialize the points here ...
|
|
for( int i = 0; i < point_count; i++ )
|
|
{
|
|
points1[i] = ...;
|
|
points2[i] = ...;
|
|
}
|
|
|
|
Mat fundamental_matrix =
|
|
findFundamentalMat(points1, points2, FM_RANSAC, 3, 0.99);
|
|
@endcode
|
|
*/
|
|
CV_EXPORTS_W Mat findFundamentalMat( InputArray points1, InputArray points2,
|
|
int method, double ransacReprojThreshold, double confidence,
|
|
int maxIters, OutputArray mask = noArray() );
|
|
|
|
/** @overload */
|
|
CV_EXPORTS_W Mat findFundamentalMat( InputArray points1, InputArray points2,
|
|
int method = FM_RANSAC,
|
|
double ransacReprojThreshold = 3., double confidence = 0.99,
|
|
OutputArray mask = noArray() );
|
|
|
|
/** @overload */
|
|
CV_EXPORTS Mat findFundamentalMat( InputArray points1, InputArray points2,
|
|
OutputArray mask, int method = FM_RANSAC,
|
|
double ransacReprojThreshold = 3., double confidence = 0.99 );
|
|
|
|
|
|
CV_EXPORTS_W Mat findFundamentalMat( InputArray points1, InputArray points2,
|
|
OutputArray mask, const UsacParams ¶ms);
|
|
|
|
/** @brief Calculates an essential matrix from the corresponding points in two images.
|
|
|
|
@param points1 Array of N (N \>= 5) 2D points from the first image. The point coordinates should
|
|
be floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param cameraMatrix Camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
Note that this function assumes that points1 and points2 are feature points from cameras with the
|
|
same camera intrinsic matrix. If this assumption does not hold for your use case, use
|
|
#undistortPoints with `P = cv::NoArray()` for both cameras to transform image points
|
|
to normalized image coordinates, which are valid for the identity camera intrinsic matrix. When
|
|
passing these coordinates, pass the identity matrix for this parameter.
|
|
@param method Method for computing an essential matrix.
|
|
- @ref RANSAC for the RANSAC algorithm.
|
|
- @ref LMEDS for the LMedS algorithm.
|
|
@param prob Parameter used for the RANSAC or LMedS methods only. It specifies a desirable level of
|
|
confidence (probability) that the estimated matrix is correct.
|
|
@param threshold Parameter used for RANSAC. It is the maximum distance from a point to an epipolar
|
|
line in pixels, beyond which the point is considered an outlier and is not used for computing the
|
|
final fundamental matrix. It can be set to something like 1-3, depending on the accuracy of the
|
|
point localization, image resolution, and the image noise.
|
|
@param mask Output array of N elements, every element of which is set to 0 for outliers and to 1
|
|
for the other points. The array is computed only in the RANSAC and LMedS methods.
|
|
@param maxIters The maximum number of robust method iterations.
|
|
|
|
This function estimates essential matrix based on the five-point algorithm solver in @cite Nister03 .
|
|
@cite SteweniusCFS is also a related. The epipolar geometry is described by the following equation:
|
|
|
|
\f[[p_2; 1]^T K^{-T} E K^{-1} [p_1; 1] = 0\f]
|
|
|
|
where \f$E\f$ is an essential matrix, \f$p_1\f$ and \f$p_2\f$ are corresponding points in the first and the
|
|
second images, respectively. The result of this function may be passed further to
|
|
#decomposeEssentialMat or #recoverPose to recover the relative pose between cameras.
|
|
*/
|
|
CV_EXPORTS_W
|
|
Mat findEssentialMat(
|
|
InputArray points1, InputArray points2,
|
|
InputArray cameraMatrix, int method = RANSAC,
|
|
double prob = 0.999, double threshold = 1.0,
|
|
int maxIters = 1000, OutputArray mask = noArray()
|
|
);
|
|
|
|
/** @overload
|
|
@param points1 Array of N (N \>= 5) 2D points from the first image. The point coordinates should
|
|
be floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param focal focal length of the camera. Note that this function assumes that points1 and points2
|
|
are feature points from cameras with same focal length and principal point.
|
|
@param pp principal point of the camera.
|
|
@param method Method for computing a fundamental matrix.
|
|
- @ref RANSAC for the RANSAC algorithm.
|
|
- @ref LMEDS for the LMedS algorithm.
|
|
@param threshold Parameter used for RANSAC. It is the maximum distance from a point to an epipolar
|
|
line in pixels, beyond which the point is considered an outlier and is not used for computing the
|
|
final fundamental matrix. It can be set to something like 1-3, depending on the accuracy of the
|
|
point localization, image resolution, and the image noise.
|
|
@param prob Parameter used for the RANSAC or LMedS methods only. It specifies a desirable level of
|
|
confidence (probability) that the estimated matrix is correct.
|
|
@param mask Output array of N elements, every element of which is set to 0 for outliers and to 1
|
|
for the other points. The array is computed only in the RANSAC and LMedS methods.
|
|
@param maxIters The maximum number of robust method iterations.
|
|
|
|
This function differs from the one above that it computes camera intrinsic matrix from focal length and
|
|
principal point:
|
|
|
|
\f[A =
|
|
\begin{bmatrix}
|
|
f & 0 & x_{pp} \\
|
|
0 & f & y_{pp} \\
|
|
0 & 0 & 1
|
|
\end{bmatrix}\f]
|
|
*/
|
|
CV_EXPORTS_W
|
|
Mat findEssentialMat(
|
|
InputArray points1, InputArray points2,
|
|
double focal = 1.0, Point2d pp = Point2d(0, 0),
|
|
int method = RANSAC, double prob = 0.999,
|
|
double threshold = 1.0, int maxIters = 1000,
|
|
OutputArray mask = noArray()
|
|
);
|
|
|
|
/** @brief Calculates an essential matrix from the corresponding points in two images from potentially two different cameras.
|
|
|
|
@param points1 Array of N (N \>= 5) 2D points from the first image. The point coordinates should
|
|
be floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param cameraMatrix1 Camera matrix \f$K = \vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}\f$ .
|
|
Note that this function assumes that points1 and points2 are feature points from cameras with the
|
|
same camera matrix. If this assumption does not hold for your use case, use
|
|
#undistortPoints with `P = cv::NoArray()` for both cameras to transform image points
|
|
to normalized image coordinates, which are valid for the identity camera matrix. When
|
|
passing these coordinates, pass the identity matrix for this parameter.
|
|
@param cameraMatrix2 Camera matrix \f$K = \vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}\f$ .
|
|
Note that this function assumes that points1 and points2 are feature points from cameras with the
|
|
same camera matrix. If this assumption does not hold for your use case, use
|
|
#undistortPoints with `P = cv::NoArray()` for both cameras to transform image points
|
|
to normalized image coordinates, which are valid for the identity camera matrix. When
|
|
passing these coordinates, pass the identity matrix for this parameter.
|
|
@param distCoeffs1 Input vector of distortion coefficients
|
|
\f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
of 4, 5, 8, 12 or 14 elements. If the vector is NULL/empty, the zero distortion coefficients are assumed.
|
|
@param distCoeffs2 Input vector of distortion coefficients
|
|
\f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
of 4, 5, 8, 12 or 14 elements. If the vector is NULL/empty, the zero distortion coefficients are assumed.
|
|
@param method Method for computing an essential matrix.
|
|
- @ref RANSAC for the RANSAC algorithm.
|
|
- @ref LMEDS for the LMedS algorithm.
|
|
@param prob Parameter used for the RANSAC or LMedS methods only. It specifies a desirable level of
|
|
confidence (probability) that the estimated matrix is correct.
|
|
@param threshold Parameter used for RANSAC. It is the maximum distance from a point to an epipolar
|
|
line in pixels, beyond which the point is considered an outlier and is not used for computing the
|
|
final fundamental matrix. It can be set to something like 1-3, depending on the accuracy of the
|
|
point localization, image resolution, and the image noise.
|
|
@param mask Output array of N elements, every element of which is set to 0 for outliers and to 1
|
|
for the other points. The array is computed only in the RANSAC and LMedS methods.
|
|
|
|
This function estimates essential matrix based on the five-point algorithm solver in @cite Nister03 .
|
|
@cite SteweniusCFS is also a related. The epipolar geometry is described by the following equation:
|
|
|
|
\f[[p_2; 1]^T K^{-T} E K^{-1} [p_1; 1] = 0\f]
|
|
|
|
where \f$E\f$ is an essential matrix, \f$p_1\f$ and \f$p_2\f$ are corresponding points in the first and the
|
|
second images, respectively. The result of this function may be passed further to
|
|
#decomposeEssentialMat or #recoverPose to recover the relative pose between cameras.
|
|
*/
|
|
CV_EXPORTS_W Mat findEssentialMat( InputArray points1, InputArray points2,
|
|
InputArray cameraMatrix1, InputArray distCoeffs1,
|
|
InputArray cameraMatrix2, InputArray distCoeffs2,
|
|
int method = RANSAC,
|
|
double prob = 0.999, double threshold = 1.0,
|
|
OutputArray mask = noArray() );
|
|
|
|
|
|
CV_EXPORTS_W Mat findEssentialMat( InputArray points1, InputArray points2,
|
|
InputArray cameraMatrix1, InputArray cameraMatrix2,
|
|
InputArray dist_coeff1, InputArray dist_coeff2, OutputArray mask,
|
|
const UsacParams ¶ms);
|
|
|
|
/** @brief Decompose an essential matrix to possible rotations and translation.
|
|
|
|
@param E The input essential matrix.
|
|
@param R1 One possible rotation matrix.
|
|
@param R2 Another possible rotation matrix.
|
|
@param t One possible translation.
|
|
|
|
This function decomposes the essential matrix E using svd decomposition @cite HartleyZ00. In
|
|
general, four possible poses exist for the decomposition of E. They are \f$[R_1, t]\f$,
|
|
\f$[R_1, -t]\f$, \f$[R_2, t]\f$, \f$[R_2, -t]\f$.
|
|
|
|
If E gives the epipolar constraint \f$[p_2; 1]^T A^{-T} E A^{-1} [p_1; 1] = 0\f$ between the image
|
|
points \f$p_1\f$ in the first image and \f$p_2\f$ in second image, then any of the tuples
|
|
\f$[R_1, t]\f$, \f$[R_1, -t]\f$, \f$[R_2, t]\f$, \f$[R_2, -t]\f$ is a change of basis from the first
|
|
camera's coordinate system to the second camera's coordinate system. However, by decomposing E, one
|
|
can only get the direction of the translation. For this reason, the translation t is returned with
|
|
unit length.
|
|
*/
|
|
CV_EXPORTS_W void decomposeEssentialMat( InputArray E, OutputArray R1, OutputArray R2, OutputArray t );
|
|
|
|
/** @brief Recovers the relative camera rotation and the translation from corresponding points in two images from two different cameras, using cheirality check. Returns the number of
|
|
inliers that pass the check.
|
|
|
|
@param points1 Array of N 2D points from the first image. The point coordinates should be
|
|
floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param cameraMatrix1 Input/output camera matrix for the first camera, the same as in
|
|
@ref calibrateCamera. Furthermore, for the stereo case, additional flags may be used, see below.
|
|
@param distCoeffs1 Input/output vector of distortion coefficients, the same as in
|
|
@ref calibrateCamera.
|
|
@param cameraMatrix2 Input/output camera matrix for the first camera, the same as in
|
|
@ref calibrateCamera. Furthermore, for the stereo case, additional flags may be used, see below.
|
|
@param distCoeffs2 Input/output vector of distortion coefficients, the same as in
|
|
@ref calibrateCamera.
|
|
@param E The output essential matrix.
|
|
@param R Output rotation matrix. Together with the translation vector, this matrix makes up a tuple
|
|
that performs a change of basis from the first camera's coordinate system to the second camera's
|
|
coordinate system. Note that, in general, t can not be used for this tuple, see the parameter
|
|
described below.
|
|
@param t Output translation vector. This vector is obtained by @ref decomposeEssentialMat and
|
|
therefore is only known up to scale, i.e. t is the direction of the translation vector and has unit
|
|
length.
|
|
@param method Method for computing an essential matrix.
|
|
- @ref RANSAC for the RANSAC algorithm.
|
|
- @ref LMEDS for the LMedS algorithm.
|
|
@param prob Parameter used for the RANSAC or LMedS methods only. It specifies a desirable level of
|
|
confidence (probability) that the estimated matrix is correct.
|
|
@param threshold Parameter used for RANSAC. It is the maximum distance from a point to an epipolar
|
|
line in pixels, beyond which the point is considered an outlier and is not used for computing the
|
|
final fundamental matrix. It can be set to something like 1-3, depending on the accuracy of the
|
|
point localization, image resolution, and the image noise.
|
|
@param mask Input/output mask for inliers in points1 and points2. If it is not empty, then it marks
|
|
inliers in points1 and points2 for then given essential matrix E. Only these inliers will be used to
|
|
recover pose. In the output mask only inliers which pass the cheirality check.
|
|
|
|
This function decomposes an essential matrix using @ref decomposeEssentialMat and then verifies
|
|
possible pose hypotheses by doing cheirality check. The cheirality check means that the
|
|
triangulated 3D points should have positive depth. Some details can be found in @cite Nister03.
|
|
|
|
This function can be used to process the output E and mask from @ref findEssentialMat. In this
|
|
scenario, points1 and points2 are the same input for findEssentialMat.:
|
|
@code
|
|
// Example. Estimation of fundamental matrix using the RANSAC algorithm
|
|
int point_count = 100;
|
|
vector<Point2f> points1(point_count);
|
|
vector<Point2f> points2(point_count);
|
|
|
|
// initialize the points here ...
|
|
for( int i = 0; i < point_count; i++ )
|
|
{
|
|
points1[i] = ...;
|
|
points2[i] = ...;
|
|
}
|
|
|
|
// Input: camera calibration of both cameras, for example using intrinsic chessboard calibration.
|
|
Mat cameraMatrix1, distCoeffs1, cameraMatrix2, distCoeffs2;
|
|
|
|
// Output: Essential matrix, relative rotation and relative translation.
|
|
Mat E, R, t, mask;
|
|
|
|
recoverPose(points1, points2, cameraMatrix1, distCoeffs1, cameraMatrix2, distCoeffs2, E, R, t, mask);
|
|
@endcode
|
|
*/
|
|
CV_EXPORTS_W int recoverPose( InputArray points1, InputArray points2,
|
|
InputArray cameraMatrix1, InputArray distCoeffs1,
|
|
InputArray cameraMatrix2, InputArray distCoeffs2,
|
|
OutputArray E, OutputArray R, OutputArray t,
|
|
int method = cv::RANSAC, double prob = 0.999, double threshold = 1.0,
|
|
InputOutputArray mask = noArray());
|
|
|
|
/** @brief Recovers the relative camera rotation and the translation from an estimated essential
|
|
matrix and the corresponding points in two images, using cheirality check. Returns the number of
|
|
inliers that pass the check.
|
|
|
|
@param E The input essential matrix.
|
|
@param points1 Array of N 2D points from the first image. The point coordinates should be
|
|
floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param cameraMatrix Camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
Note that this function assumes that points1 and points2 are feature points from cameras with the
|
|
same camera intrinsic matrix.
|
|
@param R Output rotation matrix. Together with the translation vector, this matrix makes up a tuple
|
|
that performs a change of basis from the first camera's coordinate system to the second camera's
|
|
coordinate system. Note that, in general, t can not be used for this tuple, see the parameter
|
|
described below.
|
|
@param t Output translation vector. This vector is obtained by @ref decomposeEssentialMat and
|
|
therefore is only known up to scale, i.e. t is the direction of the translation vector and has unit
|
|
length.
|
|
@param mask Input/output mask for inliers in points1 and points2. If it is not empty, then it marks
|
|
inliers in points1 and points2 for then given essential matrix E. Only these inliers will be used to
|
|
recover pose. In the output mask only inliers which pass the cheirality check.
|
|
|
|
This function decomposes an essential matrix using @ref decomposeEssentialMat and then verifies
|
|
possible pose hypotheses by doing cheirality check. The cheirality check means that the
|
|
triangulated 3D points should have positive depth. Some details can be found in @cite Nister03.
|
|
|
|
This function can be used to process the output E and mask from @ref findEssentialMat. In this
|
|
scenario, points1 and points2 are the same input for #findEssentialMat :
|
|
@code
|
|
// Example. Estimation of fundamental matrix using the RANSAC algorithm
|
|
int point_count = 100;
|
|
vector<Point2f> points1(point_count);
|
|
vector<Point2f> points2(point_count);
|
|
|
|
// initialize the points here ...
|
|
for( int i = 0; i < point_count; i++ )
|
|
{
|
|
points1[i] = ...;
|
|
points2[i] = ...;
|
|
}
|
|
|
|
// cametra matrix with both focal lengths = 1, and principal point = (0, 0)
|
|
Mat cameraMatrix = Mat::eye(3, 3, CV_64F);
|
|
|
|
Mat E, R, t, mask;
|
|
|
|
E = findEssentialMat(points1, points2, cameraMatrix, RANSAC, 0.999, 1.0, mask);
|
|
recoverPose(E, points1, points2, cameraMatrix, R, t, mask);
|
|
@endcode
|
|
*/
|
|
CV_EXPORTS_W int recoverPose( InputArray E, InputArray points1, InputArray points2,
|
|
InputArray cameraMatrix, OutputArray R, OutputArray t,
|
|
InputOutputArray mask = noArray() );
|
|
|
|
/** @overload
|
|
@param E The input essential matrix.
|
|
@param points1 Array of N 2D points from the first image. The point coordinates should be
|
|
floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1 .
|
|
@param R Output rotation matrix. Together with the translation vector, this matrix makes up a tuple
|
|
that performs a change of basis from the first camera's coordinate system to the second camera's
|
|
coordinate system. Note that, in general, t can not be used for this tuple, see the parameter
|
|
description below.
|
|
@param t Output translation vector. This vector is obtained by @ref decomposeEssentialMat and
|
|
therefore is only known up to scale, i.e. t is the direction of the translation vector and has unit
|
|
length.
|
|
@param focal Focal length of the camera. Note that this function assumes that points1 and points2
|
|
are feature points from cameras with same focal length and principal point.
|
|
@param pp principal point of the camera.
|
|
@param mask Input/output mask for inliers in points1 and points2. If it is not empty, then it marks
|
|
inliers in points1 and points2 for then given essential matrix E. Only these inliers will be used to
|
|
recover pose. In the output mask only inliers which pass the cheirality check.
|
|
|
|
This function differs from the one above that it computes camera intrinsic matrix from focal length and
|
|
principal point:
|
|
|
|
\f[A =
|
|
\begin{bmatrix}
|
|
f & 0 & x_{pp} \\
|
|
0 & f & y_{pp} \\
|
|
0 & 0 & 1
|
|
\end{bmatrix}\f]
|
|
*/
|
|
CV_EXPORTS_W int recoverPose( InputArray E, InputArray points1, InputArray points2,
|
|
OutputArray R, OutputArray t,
|
|
double focal = 1.0, Point2d pp = Point2d(0, 0),
|
|
InputOutputArray mask = noArray() );
|
|
|
|
/** @overload
|
|
@param E The input essential matrix.
|
|
@param points1 Array of N 2D points from the first image. The point coordinates should be
|
|
floating-point (single or double precision).
|
|
@param points2 Array of the second image points of the same size and format as points1.
|
|
@param cameraMatrix Camera intrinsic matrix \f$\cameramatrix{A}\f$ .
|
|
Note that this function assumes that points1 and points2 are feature points from cameras with the
|
|
same camera intrinsic matrix.
|
|
@param R Output rotation matrix. Together with the translation vector, this matrix makes up a tuple
|
|
that performs a change of basis from the first camera's coordinate system to the second camera's
|
|
coordinate system. Note that, in general, t can not be used for this tuple, see the parameter
|
|
description below.
|
|
@param t Output translation vector. This vector is obtained by @ref decomposeEssentialMat and
|
|
therefore is only known up to scale, i.e. t is the direction of the translation vector and has unit
|
|
length.
|
|
@param distanceThresh threshold distance which is used to filter out far away points (i.e. infinite
|
|
points).
|
|
@param mask Input/output mask for inliers in points1 and points2. If it is not empty, then it marks
|
|
inliers in points1 and points2 for then given essential matrix E. Only these inliers will be used to
|
|
recover pose. In the output mask only inliers which pass the cheirality check.
|
|
@param triangulatedPoints 3D points which were reconstructed by triangulation.
|
|
|
|
This function differs from the one above that it outputs the triangulated 3D point that are used for
|
|
the cheirality check.
|
|
*/
|
|
CV_EXPORTS_W int recoverPose( InputArray E, InputArray points1, InputArray points2,
|
|
InputArray cameraMatrix, OutputArray R, OutputArray t,
|
|
double distanceThresh, InputOutputArray mask = noArray(),
|
|
OutputArray triangulatedPoints = noArray());
|
|
|
|
/** @brief For points in an image of a stereo pair, computes the corresponding epilines in the other image.
|
|
|
|
@param points Input points. \f$N \times 1\f$ or \f$1 \times N\f$ matrix of type CV_32FC2 or
|
|
vector\<Point2f\> .
|
|
@param whichImage Index of the image (1 or 2) that contains the points .
|
|
@param F Fundamental matrix that can be estimated using #findFundamentalMat or #stereoRectify .
|
|
@param lines Output vector of the epipolar lines corresponding to the points in the other image.
|
|
Each line \f$ax + by + c=0\f$ is encoded by 3 numbers \f$(a, b, c)\f$ .
|
|
|
|
For every point in one of the two images of a stereo pair, the function finds the equation of the
|
|
corresponding epipolar line in the other image.
|
|
|
|
From the fundamental matrix definition (see #findFundamentalMat ), line \f$l^{(2)}_i\f$ in the second
|
|
image for the point \f$p^{(1)}_i\f$ in the first image (when whichImage=1 ) is computed as:
|
|
|
|
\f[l^{(2)}_i = F p^{(1)}_i\f]
|
|
|
|
And vice versa, when whichImage=2, \f$l^{(1)}_i\f$ is computed from \f$p^{(2)}_i\f$ as:
|
|
|
|
\f[l^{(1)}_i = F^T p^{(2)}_i\f]
|
|
|
|
Line coefficients are defined up to a scale. They are normalized so that \f$a_i^2+b_i^2=1\f$ .
|
|
*/
|
|
CV_EXPORTS_W void computeCorrespondEpilines( InputArray points, int whichImage,
|
|
InputArray F, OutputArray lines );
|
|
|
|
/** @brief This function reconstructs 3-dimensional points (in homogeneous coordinates) by using
|
|
their observations with a stereo camera.
|
|
|
|
@param projMatr1 3x4 projection matrix of the first camera, i.e. this matrix projects 3D points
|
|
given in the world's coordinate system into the first image.
|
|
@param projMatr2 3x4 projection matrix of the second camera, i.e. this matrix projects 3D points
|
|
given in the world's coordinate system into the second image.
|
|
@param projPoints1 2xN array of feature points in the first image. In the case of the c++ version,
|
|
it can be also a vector of feature points or two-channel matrix of size 1xN or Nx1.
|
|
@param projPoints2 2xN array of corresponding points in the second image. In the case of the c++
|
|
version, it can be also a vector of feature points or two-channel matrix of size 1xN or Nx1.
|
|
@param points4D 4xN array of reconstructed points in homogeneous coordinates. These points are
|
|
returned in the world's coordinate system.
|
|
|
|
@note
|
|
Keep in mind that all input data should be of float type in order for this function to work.
|
|
|
|
@note
|
|
If the projection matrices from @ref stereoRectify are used, then the returned points are
|
|
represented in the first camera's rectified coordinate system.
|
|
|
|
@sa
|
|
reprojectImageTo3D
|
|
*/
|
|
CV_EXPORTS_W void triangulatePoints( InputArray projMatr1, InputArray projMatr2,
|
|
InputArray projPoints1, InputArray projPoints2,
|
|
OutputArray points4D );
|
|
|
|
/** @brief Refines coordinates of corresponding points.
|
|
|
|
@param F 3x3 fundamental matrix.
|
|
@param points1 1xN array containing the first set of points.
|
|
@param points2 1xN array containing the second set of points.
|
|
@param newPoints1 The optimized points1.
|
|
@param newPoints2 The optimized points2.
|
|
|
|
The function implements the Optimal Triangulation Method (see Multiple View Geometry for details).
|
|
For each given point correspondence points1[i] \<-\> points2[i], and a fundamental matrix F, it
|
|
computes the corrected correspondences newPoints1[i] \<-\> newPoints2[i] that minimize the geometric
|
|
error \f$d(points1[i], newPoints1[i])^2 + d(points2[i],newPoints2[i])^2\f$ (where \f$d(a,b)\f$ is the
|
|
geometric distance between points \f$a\f$ and \f$b\f$ ) subject to the epipolar constraint
|
|
\f$newPoints2^T * F * newPoints1 = 0\f$ .
|
|
*/
|
|
CV_EXPORTS_W void correctMatches( InputArray F, InputArray points1, InputArray points2,
|
|
OutputArray newPoints1, OutputArray newPoints2 );
|
|
|
|
/** @brief Calculates the Sampson Distance between two points.
|
|
|
|
The function cv::sampsonDistance calculates and returns the first order approximation of the geometric error as:
|
|
\f[
|
|
sd( \texttt{pt1} , \texttt{pt2} )=
|
|
\frac{(\texttt{pt2}^t \cdot \texttt{F} \cdot \texttt{pt1})^2}
|
|
{((\texttt{F} \cdot \texttt{pt1})(0))^2 +
|
|
((\texttt{F} \cdot \texttt{pt1})(1))^2 +
|
|
((\texttt{F}^t \cdot \texttt{pt2})(0))^2 +
|
|
((\texttt{F}^t \cdot \texttt{pt2})(1))^2}
|
|
\f]
|
|
The fundamental matrix may be calculated using the #findFundamentalMat function. See @cite HartleyZ00 11.4.3 for details.
|
|
@param pt1 first homogeneous 2d point
|
|
@param pt2 second homogeneous 2d point
|
|
@param F fundamental matrix
|
|
@return The computed Sampson distance.
|
|
*/
|
|
CV_EXPORTS_W double sampsonDistance(InputArray pt1, InputArray pt2, InputArray F);
|
|
|
|
/** @brief Computes an optimal affine transformation between two 3D point sets.
|
|
|
|
It computes
|
|
\f[
|
|
\begin{bmatrix}
|
|
x\\
|
|
y\\
|
|
z\\
|
|
\end{bmatrix}
|
|
=
|
|
\begin{bmatrix}
|
|
a_{11} & a_{12} & a_{13}\\
|
|
a_{21} & a_{22} & a_{23}\\
|
|
a_{31} & a_{32} & a_{33}\\
|
|
\end{bmatrix}
|
|
\begin{bmatrix}
|
|
X\\
|
|
Y\\
|
|
Z\\
|
|
\end{bmatrix}
|
|
+
|
|
\begin{bmatrix}
|
|
b_1\\
|
|
b_2\\
|
|
b_3\\
|
|
\end{bmatrix}
|
|
\f]
|
|
|
|
@param src First input 3D point set containing \f$(X,Y,Z)\f$.
|
|
@param dst Second input 3D point set containing \f$(x,y,z)\f$.
|
|
@param out Output 3D affine transformation matrix \f$3 \times 4\f$ of the form
|
|
\f[
|
|
\begin{bmatrix}
|
|
a_{11} & a_{12} & a_{13} & b_1\\
|
|
a_{21} & a_{22} & a_{23} & b_2\\
|
|
a_{31} & a_{32} & a_{33} & b_3\\
|
|
\end{bmatrix}
|
|
\f]
|
|
@param inliers Output vector indicating which points are inliers (1-inlier, 0-outlier).
|
|
@param ransacThreshold Maximum reprojection error in the RANSAC algorithm to consider a point as
|
|
an inlier.
|
|
@param confidence Confidence level, between 0 and 1, for the estimated transformation. Anything
|
|
between 0.95 and 0.99 is usually good enough. Values too close to 1 can slow down the estimation
|
|
significantly. Values lower than 0.8-0.9 can result in an incorrectly estimated transformation.
|
|
|
|
The function estimates an optimal 3D affine transformation between two 3D point sets using the
|
|
RANSAC algorithm.
|
|
*/
|
|
CV_EXPORTS_W int estimateAffine3D(InputArray src, InputArray dst,
|
|
OutputArray out, OutputArray inliers,
|
|
double ransacThreshold = 3, double confidence = 0.99);
|
|
|
|
/** @brief Computes an optimal affine transformation between two 3D point sets.
|
|
|
|
It computes \f$R,s,t\f$ minimizing \f$\sum{i} dst_i - c \cdot R \cdot src_i \f$
|
|
where \f$R\f$ is a 3x3 rotation matrix, \f$t\f$ is a 3x1 translation vector and \f$s\f$ is a
|
|
scalar size value. This is an implementation of the algorithm by Umeyama \cite umeyama1991least .
|
|
The estimated affine transform has a homogeneous scale which is a subclass of affine
|
|
transformations with 7 degrees of freedom. The paired point sets need to comprise at least 3
|
|
points each.
|
|
|
|
@param src First input 3D point set.
|
|
@param dst Second input 3D point set.
|
|
@param scale If null is passed, the scale parameter c will be assumed to be 1.0.
|
|
Else the pointed-to variable will be set to the optimal scale.
|
|
@param force_rotation If true, the returned rotation will never be a reflection.
|
|
This might be unwanted, e.g. when optimizing a transform between a right- and a
|
|
left-handed coordinate system.
|
|
@return 3D affine transformation matrix \f$3 \times 4\f$ of the form
|
|
\f[T =
|
|
\begin{bmatrix}
|
|
R & t\\
|
|
\end{bmatrix}
|
|
\f]
|
|
|
|
*/
|
|
CV_EXPORTS_W cv::Mat estimateAffine3D(InputArray src, InputArray dst,
|
|
CV_OUT double* scale = nullptr, bool force_rotation = true);
|
|
|
|
/** @brief Computes an optimal translation between two 3D point sets.
|
|
*
|
|
* It computes
|
|
* \f[
|
|
* \begin{bmatrix}
|
|
* x\\
|
|
* y\\
|
|
* z\\
|
|
* \end{bmatrix}
|
|
* =
|
|
* \begin{bmatrix}
|
|
* X\\
|
|
* Y\\
|
|
* Z\\
|
|
* \end{bmatrix}
|
|
* +
|
|
* \begin{bmatrix}
|
|
* b_1\\
|
|
* b_2\\
|
|
* b_3\\
|
|
* \end{bmatrix}
|
|
* \f]
|
|
*
|
|
* @param src First input 3D point set containing \f$(X,Y,Z)\f$.
|
|
* @param dst Second input 3D point set containing \f$(x,y,z)\f$.
|
|
* @param out Output 3D translation vector \f$3 \times 1\f$ of the form
|
|
* \f[
|
|
* \begin{bmatrix}
|
|
* b_1 \\
|
|
* b_2 \\
|
|
* b_3 \\
|
|
* \end{bmatrix}
|
|
* \f]
|
|
* @param inliers Output vector indicating which points are inliers (1-inlier, 0-outlier).
|
|
* @param ransacThreshold Maximum reprojection error in the RANSAC algorithm to consider a point as
|
|
* an inlier.
|
|
* @param confidence Confidence level, between 0 and 1, for the estimated transformation. Anything
|
|
* between 0.95 and 0.99 is usually good enough. Values too close to 1 can slow down the estimation
|
|
* significantly. Values lower than 0.8-0.9 can result in an incorrectly estimated transformation.
|
|
*
|
|
* The function estimates an optimal 3D translation between two 3D point sets using the
|
|
* RANSAC algorithm.
|
|
* */
|
|
CV_EXPORTS_W int estimateTranslation3D(InputArray src, InputArray dst,
|
|
OutputArray out, OutputArray inliers,
|
|
double ransacThreshold = 3, double confidence = 0.99);
|
|
|
|
/** @brief Computes an optimal affine transformation between two 2D point sets.
|
|
|
|
It computes
|
|
\f[
|
|
\begin{bmatrix}
|
|
x\\
|
|
y\\
|
|
\end{bmatrix}
|
|
=
|
|
\begin{bmatrix}
|
|
a_{11} & a_{12}\\
|
|
a_{21} & a_{22}\\
|
|
\end{bmatrix}
|
|
\begin{bmatrix}
|
|
X\\
|
|
Y\\
|
|
\end{bmatrix}
|
|
+
|
|
\begin{bmatrix}
|
|
b_1\\
|
|
b_2\\
|
|
\end{bmatrix}
|
|
\f]
|
|
|
|
@param from First input 2D point set containing \f$(X,Y)\f$.
|
|
@param to Second input 2D point set containing \f$(x,y)\f$.
|
|
@param inliers Output vector indicating which points are inliers (1-inlier, 0-outlier).
|
|
@param method Robust method used to compute transformation. The following methods are possible:
|
|
- @ref RANSAC - RANSAC-based robust method
|
|
- @ref LMEDS - Least-Median robust method
|
|
RANSAC is the default method.
|
|
@param ransacReprojThreshold Maximum reprojection error in the RANSAC algorithm to consider
|
|
a point as an inlier. Applies only to RANSAC.
|
|
@param maxIters The maximum number of robust method iterations.
|
|
@param confidence Confidence level, between 0 and 1, for the estimated transformation. Anything
|
|
between 0.95 and 0.99 is usually good enough. Values too close to 1 can slow down the estimation
|
|
significantly. Values lower than 0.8-0.9 can result in an incorrectly estimated transformation.
|
|
@param refineIters Maximum number of iterations of refining algorithm (Levenberg-Marquardt).
|
|
Passing 0 will disable refining, so the output matrix will be output of robust method.
|
|
|
|
@return Output 2D affine transformation matrix \f$2 \times 3\f$ or empty matrix if transformation
|
|
could not be estimated. The returned matrix has the following form:
|
|
\f[
|
|
\begin{bmatrix}
|
|
a_{11} & a_{12} & b_1\\
|
|
a_{21} & a_{22} & b_2\\
|
|
\end{bmatrix}
|
|
\f]
|
|
|
|
The function estimates an optimal 2D affine transformation between two 2D point sets using the
|
|
selected robust algorithm.
|
|
|
|
The computed transformation is then refined further (using only inliers) with the
|
|
Levenberg-Marquardt method to reduce the re-projection error even more.
|
|
|
|
@note
|
|
The RANSAC method can handle practically any ratio of outliers but needs a threshold to
|
|
distinguish inliers from outliers. The method LMeDS does not need any threshold but it works
|
|
correctly only when there are more than 50% of inliers.
|
|
|
|
@sa estimateAffinePartial2D, getAffineTransform
|
|
*/
|
|
CV_EXPORTS_W Mat estimateAffine2D(InputArray from, InputArray to, OutputArray inliers = noArray(),
|
|
int method = RANSAC, double ransacReprojThreshold = 3,
|
|
size_t maxIters = 2000, double confidence = 0.99,
|
|
size_t refineIters = 10);
|
|
|
|
|
|
CV_EXPORTS_W Mat estimateAffine2D(InputArray pts1, InputArray pts2, OutputArray inliers,
|
|
const UsacParams ¶ms);
|
|
|
|
/** @brief Computes an optimal limited affine transformation with 4 degrees of freedom between
|
|
two 2D point sets.
|
|
|
|
@param from First input 2D point set.
|
|
@param to Second input 2D point set.
|
|
@param inliers Output vector indicating which points are inliers.
|
|
@param method Robust method used to compute transformation. The following methods are possible:
|
|
- @ref RANSAC - RANSAC-based robust method
|
|
- @ref LMEDS - Least-Median robust method
|
|
RANSAC is the default method.
|
|
@param ransacReprojThreshold Maximum reprojection error in the RANSAC algorithm to consider
|
|
a point as an inlier. Applies only to RANSAC.
|
|
@param maxIters The maximum number of robust method iterations.
|
|
@param confidence Confidence level, between 0 and 1, for the estimated transformation. Anything
|
|
between 0.95 and 0.99 is usually good enough. Values too close to 1 can slow down the estimation
|
|
significantly. Values lower than 0.8-0.9 can result in an incorrectly estimated transformation.
|
|
@param refineIters Maximum number of iterations of refining algorithm (Levenberg-Marquardt).
|
|
Passing 0 will disable refining, so the output matrix will be output of robust method.
|
|
|
|
@return Output 2D affine transformation (4 degrees of freedom) matrix \f$2 \times 3\f$ or
|
|
empty matrix if transformation could not be estimated.
|
|
|
|
The function estimates an optimal 2D affine transformation with 4 degrees of freedom limited to
|
|
combinations of translation, rotation, and uniform scaling. Uses the selected algorithm for robust
|
|
estimation.
|
|
|
|
The computed transformation is then refined further (using only inliers) with the
|
|
Levenberg-Marquardt method to reduce the re-projection error even more.
|
|
|
|
Estimated transformation matrix is:
|
|
\f[ \begin{bmatrix} \cos(\theta) \cdot s & -\sin(\theta) \cdot s & t_x \\
|
|
\sin(\theta) \cdot s & \cos(\theta) \cdot s & t_y
|
|
\end{bmatrix} \f]
|
|
Where \f$ \theta \f$ is the rotation angle, \f$ s \f$ the scaling factor and \f$ t_x, t_y \f$ are
|
|
translations in \f$ x, y \f$ axes respectively.
|
|
|
|
@note
|
|
The RANSAC method can handle practically any ratio of outliers but need a threshold to
|
|
distinguish inliers from outliers. The method LMeDS does not need any threshold but it works
|
|
correctly only when there are more than 50% of inliers.
|
|
|
|
@sa estimateAffine2D, getAffineTransform
|
|
*/
|
|
CV_EXPORTS_W cv::Mat estimateAffinePartial2D(InputArray from, InputArray to, OutputArray inliers = noArray(),
|
|
int method = RANSAC, double ransacReprojThreshold = 3,
|
|
size_t maxIters = 2000, double confidence = 0.99,
|
|
size_t refineIters = 10);
|
|
|
|
/** @example samples/cpp/tutorial_code/features2D/Homography/decompose_homography.cpp
|
|
An example program with homography decomposition.
|
|
|
|
Check @ref tutorial_homography "the corresponding tutorial" for more details.
|
|
*/
|
|
|
|
/** @brief Decompose a homography matrix to rotation(s), translation(s) and plane normal(s).
|
|
|
|
@param H The input homography matrix between two images.
|
|
@param K The input camera intrinsic matrix.
|
|
@param rotations Array of rotation matrices.
|
|
@param translations Array of translation matrices.
|
|
@param normals Array of plane normal matrices.
|
|
|
|
This function extracts relative camera motion between two views of a planar object and returns up to
|
|
four mathematical solution tuples of rotation, translation, and plane normal. The decomposition of
|
|
the homography matrix H is described in detail in @cite Malis.
|
|
|
|
If the homography H, induced by the plane, gives the constraint
|
|
\f[s_i \vecthree{x'_i}{y'_i}{1} \sim H \vecthree{x_i}{y_i}{1}\f] on the source image points
|
|
\f$p_i\f$ and the destination image points \f$p'_i\f$, then the tuple of rotations[k] and
|
|
translations[k] is a change of basis from the source camera's coordinate system to the destination
|
|
camera's coordinate system. However, by decomposing H, one can only get the translation normalized
|
|
by the (typically unknown) depth of the scene, i.e. its direction but with normalized length.
|
|
|
|
If point correspondences are available, at least two solutions may further be invalidated, by
|
|
applying positive depth constraint, i.e. all points must be in front of the camera.
|
|
*/
|
|
CV_EXPORTS_W int decomposeHomographyMat(InputArray H,
|
|
InputArray K,
|
|
OutputArrayOfArrays rotations,
|
|
OutputArrayOfArrays translations,
|
|
OutputArrayOfArrays normals);
|
|
|
|
/** @brief Filters homography decompositions based on additional information.
|
|
|
|
@param rotations Vector of rotation matrices.
|
|
@param normals Vector of plane normal matrices.
|
|
@param beforePoints Vector of (rectified) visible reference points before the homography is applied
|
|
@param afterPoints Vector of (rectified) visible reference points after the homography is applied
|
|
@param possibleSolutions Vector of int indices representing the viable solution set after filtering
|
|
@param pointsMask optional Mat/Vector of 8u type representing the mask for the inliers as given by the #findHomography function
|
|
|
|
This function is intended to filter the output of the #decomposeHomographyMat based on additional
|
|
information as described in @cite Malis . The summary of the method: the #decomposeHomographyMat function
|
|
returns 2 unique solutions and their "opposites" for a total of 4 solutions. If we have access to the
|
|
sets of points visible in the camera frame before and after the homography transformation is applied,
|
|
we can determine which are the true potential solutions and which are the opposites by verifying which
|
|
homographies are consistent with all visible reference points being in front of the camera. The inputs
|
|
are left unchanged; the filtered solution set is returned as indices into the existing one.
|
|
|
|
*/
|
|
CV_EXPORTS_W void filterHomographyDecompByVisibleRefpoints(InputArrayOfArrays rotations,
|
|
InputArrayOfArrays normals,
|
|
InputArray beforePoints,
|
|
InputArray afterPoints,
|
|
OutputArray possibleSolutions,
|
|
InputArray pointsMask = noArray());
|
|
|
|
//! cv::undistort mode
|
|
enum UndistortTypes
|
|
{
|
|
PROJ_SPHERICAL_ORTHO = 0,
|
|
PROJ_SPHERICAL_EQRECT = 1
|
|
};
|
|
|
|
/** @brief Transforms an image to compensate for lens distortion.
|
|
|
|
The function transforms an image to compensate radial and tangential lens distortion.
|
|
|
|
The function is simply a combination of #initUndistortRectifyMap (with unity R ) and #remap
|
|
(with bilinear interpolation). See the former function for details of the transformation being
|
|
performed.
|
|
|
|
Those pixels in the destination image, for which there is no correspondent pixels in the source
|
|
image, are filled with zeros (black color).
|
|
|
|
A particular subset of the source image that will be visible in the corrected image can be regulated
|
|
by newCameraMatrix. You can use #getOptimalNewCameraMatrix to compute the appropriate
|
|
newCameraMatrix depending on your requirements.
|
|
|
|
The camera matrix and the distortion parameters can be determined using #calibrateCamera. If
|
|
the resolution of images is different from the resolution used at the calibration stage, \f$f_x,
|
|
f_y, c_x\f$ and \f$c_y\f$ need to be scaled accordingly, while the distortion coefficients remain
|
|
the same.
|
|
|
|
@param src Input (distorted) image.
|
|
@param dst Output (corrected) image that has the same size and type as src .
|
|
@param cameraMatrix Input camera matrix \f$A = \vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
of 4, 5, 8, 12 or 14 elements. If the vector is NULL/empty, the zero distortion coefficients are assumed.
|
|
@param newCameraMatrix Camera matrix of the distorted image. By default, it is the same as
|
|
cameraMatrix but you may additionally scale and shift the result by using a different matrix.
|
|
*/
|
|
CV_EXPORTS_W void undistort( InputArray src, OutputArray dst,
|
|
InputArray cameraMatrix,
|
|
InputArray distCoeffs,
|
|
InputArray newCameraMatrix = noArray() );
|
|
|
|
/** @brief Computes the undistortion and rectification transformation map.
|
|
|
|
The function computes the joint undistortion and rectification transformation and represents the
|
|
result in the form of maps for #remap. The undistorted image looks like original, as if it is
|
|
captured with a camera using the camera matrix =newCameraMatrix and zero distortion. In case of a
|
|
monocular camera, newCameraMatrix is usually equal to cameraMatrix, or it can be computed by
|
|
#getOptimalNewCameraMatrix for a better control over scaling. In case of a stereo camera,
|
|
newCameraMatrix is normally set to P1 or P2 computed by #stereoRectify .
|
|
|
|
Also, this new camera is oriented differently in the coordinate space, according to R. That, for
|
|
example, helps to align two heads of a stereo camera so that the epipolar lines on both images
|
|
become horizontal and have the same y- coordinate (in case of a horizontally aligned stereo camera).
|
|
|
|
The function actually builds the maps for the inverse mapping algorithm that is used by #remap. That
|
|
is, for each pixel \f$(u, v)\f$ in the destination (corrected and rectified) image, the function
|
|
computes the corresponding coordinates in the source image (that is, in the original image from
|
|
camera). The following process is applied:
|
|
\f[
|
|
\begin{array}{l}
|
|
x \leftarrow (u - {c'}_x)/{f'}_x \\
|
|
y \leftarrow (v - {c'}_y)/{f'}_y \\
|
|
{[X\,Y\,W]} ^T \leftarrow R^{-1}*[x \, y \, 1]^T \\
|
|
x' \leftarrow X/W \\
|
|
y' \leftarrow Y/W \\
|
|
r^2 \leftarrow x'^2 + y'^2 \\
|
|
x'' \leftarrow x' \frac{1 + k_1 r^2 + k_2 r^4 + k_3 r^6}{1 + k_4 r^2 + k_5 r^4 + k_6 r^6}
|
|
+ 2p_1 x' y' + p_2(r^2 + 2 x'^2) + s_1 r^2 + s_2 r^4\\
|
|
y'' \leftarrow y' \frac{1 + k_1 r^2 + k_2 r^4 + k_3 r^6}{1 + k_4 r^2 + k_5 r^4 + k_6 r^6}
|
|
+ p_1 (r^2 + 2 y'^2) + 2 p_2 x' y' + s_3 r^2 + s_4 r^4 \\
|
|
s\vecthree{x'''}{y'''}{1} =
|
|
\vecthreethree{R_{33}(\tau_x, \tau_y)}{0}{-R_{13}((\tau_x, \tau_y)}
|
|
{0}{R_{33}(\tau_x, \tau_y)}{-R_{23}(\tau_x, \tau_y)}
|
|
{0}{0}{1} R(\tau_x, \tau_y) \vecthree{x''}{y''}{1}\\
|
|
map_x(u,v) \leftarrow x''' f_x + c_x \\
|
|
map_y(u,v) \leftarrow y''' f_y + c_y
|
|
\end{array}
|
|
\f]
|
|
where \f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
are the distortion coefficients.
|
|
|
|
In case of a stereo camera, this function is called twice: once for each camera head, after
|
|
#stereoRectify, which in its turn is called after #stereoCalibrate. But if the stereo camera
|
|
was not calibrated, it is still possible to compute the rectification transformations directly from
|
|
the fundamental matrix using #stereoRectifyUncalibrated. For each camera, the function computes
|
|
homography H as the rectification transformation in a pixel domain, not a rotation matrix R in 3D
|
|
space. R can be computed from H as
|
|
\f[\texttt{R} = \texttt{cameraMatrix} ^{-1} \cdot \texttt{H} \cdot \texttt{cameraMatrix}\f]
|
|
where cameraMatrix can be chosen arbitrarily.
|
|
|
|
@param cameraMatrix Input camera matrix \f$A=\vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
of 4, 5, 8, 12 or 14 elements. If the vector is NULL/empty, the zero distortion coefficients are assumed.
|
|
@param R Optional rectification transformation in the object space (3x3 matrix). R1 or R2 ,
|
|
computed by #stereoRectify can be passed here. If the matrix is empty, the identity transformation
|
|
is assumed. In cvInitUndistortMap R assumed to be an identity matrix.
|
|
@param newCameraMatrix New camera matrix \f$A'=\vecthreethree{f_x'}{0}{c_x'}{0}{f_y'}{c_y'}{0}{0}{1}\f$.
|
|
@param size Undistorted image size.
|
|
@param m1type Type of the first output map that can be CV_32FC1, CV_32FC2 or CV_16SC2, see #convertMaps
|
|
@param map1 The first output map.
|
|
@param map2 The second output map.
|
|
*/
|
|
CV_EXPORTS_W
|
|
void initUndistortRectifyMap(InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputArray R, InputArray newCameraMatrix,
|
|
Size size, int m1type, OutputArray map1, OutputArray map2);
|
|
|
|
/** @brief Computes the projection and inverse-rectification transformation map. In essense, this is the inverse of
|
|
#initUndistortRectifyMap to accomodate stereo-rectification of projectors ('inverse-cameras') in projector-camera pairs.
|
|
|
|
The function computes the joint projection and inverse rectification transformation and represents the
|
|
result in the form of maps for #remap. The projected image looks like a distorted version of the original which,
|
|
once projected by a projector, should visually match the original. In case of a monocular camera, newCameraMatrix
|
|
is usually equal to cameraMatrix, or it can be computed by
|
|
#getOptimalNewCameraMatrix for a better control over scaling. In case of a projector-camera pair,
|
|
newCameraMatrix is normally set to P1 or P2 computed by #stereoRectify .
|
|
|
|
The projector is oriented differently in the coordinate space, according to R. In case of projector-camera pairs,
|
|
this helps align the projector (in the same manner as #initUndistortRectifyMap for the camera) to create a stereo-rectified pair. This
|
|
allows epipolar lines on both images to become horizontal and have the same y-coordinate (in case of a horizontally aligned projector-camera pair).
|
|
|
|
The function builds the maps for the inverse mapping algorithm that is used by #remap. That
|
|
is, for each pixel \f$(u, v)\f$ in the destination (projected and inverse-rectified) image, the function
|
|
computes the corresponding coordinates in the source image (that is, in the original digital image). The following process is applied:
|
|
|
|
\f[
|
|
\begin{array}{l}
|
|
\text{newCameraMatrix}\\
|
|
x \leftarrow (u - {c'}_x)/{f'}_x \\
|
|
y \leftarrow (v - {c'}_y)/{f'}_y \\
|
|
|
|
\\\text{Undistortion}
|
|
\\\scriptsize{\textit{though equation shown is for radial undistortion, function implements cv::undistortPoints()}}\\
|
|
r^2 \leftarrow x^2 + y^2 \\
|
|
\theta \leftarrow \frac{1 + k_1 r^2 + k_2 r^4 + k_3 r^6}{1 + k_4 r^2 + k_5 r^4 + k_6 r^6}\\
|
|
x' \leftarrow \frac{x}{\theta} \\
|
|
y' \leftarrow \frac{y}{\theta} \\
|
|
|
|
\\\text{Rectification}\\
|
|
{[X\,Y\,W]} ^T \leftarrow R*[x' \, y' \, 1]^T \\
|
|
x'' \leftarrow X/W \\
|
|
y'' \leftarrow Y/W \\
|
|
|
|
\\\text{cameraMatrix}\\
|
|
map_x(u,v) \leftarrow x'' f_x + c_x \\
|
|
map_y(u,v) \leftarrow y'' f_y + c_y
|
|
\end{array}
|
|
\f]
|
|
where \f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
are the distortion coefficients vector distCoeffs.
|
|
|
|
In case of a stereo-rectified projector-camera pair, this function is called for the projector while #initUndistortRectifyMap is called for the camera head.
|
|
This is done after #stereoRectify, which in turn is called after #stereoCalibrate. If the projector-camera pair
|
|
is not calibrated, it is still possible to compute the rectification transformations directly from
|
|
the fundamental matrix using #stereoRectifyUncalibrated. For the projector and camera, the function computes
|
|
homography H as the rectification transformation in a pixel domain, not a rotation matrix R in 3D
|
|
space. R can be computed from H as
|
|
\f[\texttt{R} = \texttt{cameraMatrix} ^{-1} \cdot \texttt{H} \cdot \texttt{cameraMatrix}\f]
|
|
where cameraMatrix can be chosen arbitrarily.
|
|
|
|
@param cameraMatrix Input camera matrix \f$A=\vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
of 4, 5, 8, 12 or 14 elements. If the vector is NULL/empty, the zero distortion coefficients are assumed.
|
|
@param R Optional rectification transformation in the object space (3x3 matrix). R1 or R2,
|
|
computed by #stereoRectify can be passed here. If the matrix is empty, the identity transformation
|
|
is assumed.
|
|
@param newCameraMatrix New camera matrix \f$A'=\vecthreethree{f_x'}{0}{c_x'}{0}{f_y'}{c_y'}{0}{0}{1}\f$.
|
|
@param size Distorted image size.
|
|
@param m1type Type of the first output map. Can be CV_32FC1, CV_32FC2 or CV_16SC2, see #convertMaps
|
|
@param map1 The first output map for #remap.
|
|
@param map2 The second output map for #remap.
|
|
*/
|
|
CV_EXPORTS_W
|
|
void initInverseRectificationMap( InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputArray R, InputArray newCameraMatrix,
|
|
const Size& size, int m1type, OutputArray map1, OutputArray map2 );
|
|
|
|
|
|
//! initializes maps for #remap for wide-angle
|
|
CV_EXPORTS
|
|
float initWideAngleProjMap(InputArray cameraMatrix, InputArray distCoeffs,
|
|
Size imageSize, int destImageWidth,
|
|
int m1type, OutputArray map1, OutputArray map2,
|
|
enum UndistortTypes projType = PROJ_SPHERICAL_EQRECT, double alpha = 0);
|
|
static inline
|
|
float initWideAngleProjMap(InputArray cameraMatrix, InputArray distCoeffs,
|
|
Size imageSize, int destImageWidth,
|
|
int m1type, OutputArray map1, OutputArray map2,
|
|
int projType, double alpha = 0)
|
|
{
|
|
return initWideAngleProjMap(cameraMatrix, distCoeffs, imageSize, destImageWidth,
|
|
m1type, map1, map2, (UndistortTypes)projType, alpha);
|
|
}
|
|
|
|
/** @brief Returns the default new camera matrix.
|
|
|
|
The function returns the camera matrix that is either an exact copy of the input cameraMatrix (when
|
|
centerPrinicipalPoint=false ), or the modified one (when centerPrincipalPoint=true).
|
|
|
|
In the latter case, the new camera matrix will be:
|
|
|
|
\f[\begin{bmatrix} f_x && 0 && ( \texttt{imgSize.width} -1)*0.5 \\ 0 && f_y && ( \texttt{imgSize.height} -1)*0.5 \\ 0 && 0 && 1 \end{bmatrix} ,\f]
|
|
|
|
where \f$f_x\f$ and \f$f_y\f$ are \f$(0,0)\f$ and \f$(1,1)\f$ elements of cameraMatrix, respectively.
|
|
|
|
By default, the undistortion functions in OpenCV (see #initUndistortRectifyMap, #undistort) do not
|
|
move the principal point. However, when you work with stereo, it is important to move the principal
|
|
points in both views to the same y-coordinate (which is required by most of stereo correspondence
|
|
algorithms), and may be to the same x-coordinate too. So, you can form the new camera matrix for
|
|
each view where the principal points are located at the center.
|
|
|
|
@param cameraMatrix Input camera matrix.
|
|
@param imgsize Camera view image size in pixels.
|
|
@param centerPrincipalPoint Location of the principal point in the new camera matrix. The
|
|
parameter indicates whether this location should be at the image center or not.
|
|
*/
|
|
CV_EXPORTS_W
|
|
Mat getDefaultNewCameraMatrix(InputArray cameraMatrix, Size imgsize = Size(),
|
|
bool centerPrincipalPoint = false);
|
|
|
|
/** @brief Returns the inscribed and bounding rectangles for the "undisorted" image plane.
|
|
|
|
The functions emulates undistortion of the image plane using the specified camera matrix,
|
|
distortion coefficients, the optional 3D rotation and the "new" camera matrix. In the case of
|
|
noticeable radial (or maybe pinclusion) distortion the rectangular image plane is distorted and
|
|
turns into some convex or concave shape. The function computes approximate inscribed (inner) and
|
|
bounding (outer) rectangles after such undistortion. The rectangles can be used to adjust
|
|
the newCameraMatrix so that the result image, for example, fits all the data from the original image
|
|
(at the expense of possibly big "black" areas) or, for another example, gets rid of black areas at the expense
|
|
some lost data near the original image edge. The function #getOptimalNewCameraMatrix uses this function
|
|
to compute the optimal new camera matrix.
|
|
|
|
@param cameraMatrix the original camera matrix.
|
|
@param distCoeffs distortion coefficients.
|
|
@param R the optional 3D rotation, applied before projection (see stereoRectify etc.)
|
|
@param newCameraMatrix the new camera matrix after undistortion. Usually it matches the original cameraMatrix.
|
|
@param imgSize the size of the image plane.
|
|
@param inner the output maximal inscribed rectangle of the undistorted image plane.
|
|
@param outer the output minimal bounding rectangle of the undistorted image plane.
|
|
*/
|
|
CV_EXPORTS void getUndistortRectangles(InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputArray R, InputArray newCameraMatrix, Size imgSize,
|
|
Rect_<float>& inner, Rect_<float>& outer );
|
|
|
|
/** @brief Returns the new camera intrinsic matrix based on the free scaling parameter.
|
|
|
|
@param cameraMatrix Input camera intrinsic matrix.
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$\distcoeffs\f$. If the vector is NULL/empty, the zero distortion coefficients are
|
|
assumed.
|
|
@param imageSize Original image size.
|
|
@param alpha Free scaling parameter between 0 (when all the pixels in the undistorted image are
|
|
valid) and 1 (when all the source image pixels are retained in the undistorted image). See
|
|
#stereoRectify for details.
|
|
@param newImgSize Image size after rectification. By default, it is set to imageSize .
|
|
@param validPixROI Optional output rectangle that outlines all-good-pixels region in the
|
|
undistorted image. See roi1, roi2 description in #stereoRectify .
|
|
@param centerPrincipalPoint Optional flag that indicates whether in the new camera intrinsic matrix the
|
|
principal point should be at the image center or not. By default, the principal point is chosen to
|
|
best fit a subset of the source image (determined by alpha) to the corrected image.
|
|
@return new_camera_matrix Output new camera intrinsic matrix.
|
|
|
|
The function computes and returns the optimal new camera intrinsic matrix based on the free scaling parameter.
|
|
By varying this parameter, you may retrieve only sensible pixels alpha=0 , keep all the original
|
|
image pixels if there is valuable information in the corners alpha=1 , or get something in between.
|
|
When alpha\>0 , the undistorted result is likely to have some black pixels corresponding to
|
|
"virtual" pixels outside of the captured distorted image. The original camera intrinsic matrix, distortion
|
|
coefficients, the computed new camera intrinsic matrix, and newImageSize should be passed to
|
|
#initUndistortRectifyMap to produce the maps for #remap .
|
|
*/
|
|
CV_EXPORTS_W Mat getOptimalNewCameraMatrix( InputArray cameraMatrix, InputArray distCoeffs,
|
|
Size imageSize, double alpha, Size newImgSize = Size(),
|
|
CV_OUT Rect* validPixROI = 0,
|
|
bool centerPrincipalPoint = false);
|
|
|
|
/** @brief Computes the ideal point coordinates from the observed point coordinates.
|
|
|
|
The function is similar to #undistort and #initUndistortRectifyMap but it operates on a
|
|
sparse set of points instead of a raster image. Also the function performs a reverse transformation
|
|
to #projectPoints. In case of a 3D object, it does not reconstruct its 3D coordinates, but for a
|
|
planar object, it does, up to a translation vector, if the proper R is specified.
|
|
|
|
For each observed point coordinate \f$(u, v)\f$ the function computes:
|
|
\f[
|
|
\begin{array}{l}
|
|
x^{"} \leftarrow (u - c_x)/f_x \\
|
|
y^{"} \leftarrow (v - c_y)/f_y \\
|
|
(x',y') = undistort(x^{"},y^{"}, \texttt{distCoeffs}) \\
|
|
{[X\,Y\,W]} ^T \leftarrow R*[x' \, y' \, 1]^T \\
|
|
x \leftarrow X/W \\
|
|
y \leftarrow Y/W \\
|
|
\text{only performed if P is specified:} \\
|
|
u' \leftarrow x {f'}_x + {c'}_x \\
|
|
v' \leftarrow y {f'}_y + {c'}_y
|
|
\end{array}
|
|
\f]
|
|
|
|
where *undistort* is an approximate iterative algorithm that estimates the normalized original
|
|
point coordinates out of the normalized distorted point coordinates ("normalized" means that the
|
|
coordinates do not depend on the camera matrix).
|
|
|
|
The function can be used for both a stereo camera head or a monocular camera (when R is empty).
|
|
@param src Observed point coordinates, 2xN/Nx2 1-channel or 1xN/Nx1 2-channel (CV_32FC2 or CV_64FC2) (or
|
|
vector\<Point2f\> ).
|
|
@param dst Output ideal point coordinates (1xN/Nx1 2-channel or vector\<Point2f\> ) after undistortion and reverse perspective
|
|
transformation. If matrix P is identity or omitted, dst will contain normalized point coordinates.
|
|
@param cameraMatrix Camera matrix \f$\vecthreethree{f_x}{0}{c_x}{0}{f_y}{c_y}{0}{0}{1}\f$ .
|
|
@param distCoeffs Input vector of distortion coefficients
|
|
\f$(k_1, k_2, p_1, p_2[, k_3[, k_4, k_5, k_6[, s_1, s_2, s_3, s_4[, \tau_x, \tau_y]]]])\f$
|
|
of 4, 5, 8, 12 or 14 elements. If the vector is NULL/empty, the zero distortion coefficients are assumed.
|
|
@param R Rectification transformation in the object space (3x3 matrix). R1 or R2 computed by
|
|
#stereoRectify can be passed here. If the matrix is empty, the identity transformation is used.
|
|
@param P New camera matrix (3x3) or new projection matrix (3x4) \f$\begin{bmatrix} {f'}_x & 0 & {c'}_x & t_x \\ 0 & {f'}_y & {c'}_y & t_y \\ 0 & 0 & 1 & t_z \end{bmatrix}\f$. P1 or P2 computed by
|
|
#stereoRectify can be passed here. If the matrix is empty, the identity new camera matrix is used.
|
|
@param criteria termination criteria for the iterative point undistortion algorithm
|
|
*/
|
|
CV_EXPORTS_W
|
|
void undistortPoints(InputArray src, OutputArray dst,
|
|
InputArray cameraMatrix, InputArray distCoeffs,
|
|
InputArray R = noArray(), InputArray P = noArray(),
|
|
TermCriteria criteria=TermCriteria(TermCriteria::MAX_ITER, 5, 0.01));
|
|
|
|
|
|
/** @brief Octree for 3D vision.
|
|
*
|
|
* In 3D vision filed, the Octree is used to process and accelerate the pointcloud data. The class Octree represents
|
|
* the Octree data structure. Each Octree will have a fixed depth. The depth of Octree refers to the distance from
|
|
* the root node to the leaf node.All OctreeNodes will not exceed this depth.Increasing the depth will increase
|
|
* the amount of calculation exponentially. And the small number of depth refers low resolution of Octree.
|
|
* Each node contains 8 children, which are used to divide the space cube into eight parts. Each octree node represents
|
|
* a cube. And these eight children will have a fixed order, the order is described as follows:
|
|
*
|
|
* For illustration, assume,
|
|
*
|
|
* rootNode: origin == (0, 0, 0), size == 2
|
|
*
|
|
* Then,
|
|
*
|
|
* children[0]: origin == (0, 0, 0), size == 1
|
|
*
|
|
* children[1]: origin == (1, 0, 0), size == 1, along X-axis next to child 0
|
|
*
|
|
* children[2]: origin == (0, 1, 0), size == 1, along Y-axis next to child 0
|
|
*
|
|
* children[3]: origin == (1, 1, 0), size == 1, in X-Y plane
|
|
*
|
|
* children[4]: origin == (0, 0, 1), size == 1, along Z-axis next to child 0
|
|
*
|
|
* children[5]: origin == (1, 0, 1), size == 1, in X-Z plane
|
|
*
|
|
* children[6]: origin == (0, 1, 1), size == 1, in Y-Z plane
|
|
*
|
|
* children[7]: origin == (1, 1, 1), size == 1, furthest from child 0
|
|
*/
|
|
|
|
class CV_EXPORTS Octree {
|
|
|
|
public:
|
|
|
|
//! Default constructor.
|
|
Octree();
|
|
|
|
/** @overload
|
|
* @brief Create an empty Octree and set the maximum depth.
|
|
*
|
|
* @param maxDepth The max depth of the Octree. The maxDepth > -1.
|
|
*/
|
|
explicit Octree(int maxDepth);
|
|
|
|
/** @overload
|
|
* @brief Create an Octree from the PointCloud data with the specific max depth.
|
|
*
|
|
* @param pointCloud Point cloud data.
|
|
* @param maxDepth The max depth of the Octree.
|
|
*/
|
|
Octree(const std::vector<Point3f> &pointCloud, int maxDepth);
|
|
|
|
/** @overload
|
|
* @brief Create an empty Octree.
|
|
*
|
|
* @param maxDepth Max depth.
|
|
* @param size Initial Cube size.
|
|
* @param origin Initial center coordinate.
|
|
*/
|
|
Octree(int maxDepth, double size, const Point3f& origin);
|
|
|
|
//! Default destructor
|
|
~Octree();
|
|
|
|
/** @brief Insert a point data to a OctreeNode.
|
|
*
|
|
* @param point The point data in Point3f format.
|
|
*/
|
|
void insertPoint(const Point3f& point);
|
|
|
|
/** @brief Read point cloud data and create OctreeNode.
|
|
*
|
|
* This function is only called when the octree is being created.
|
|
* @param pointCloud PointCloud data.
|
|
* @param maxDepth The max depth of the Octree.
|
|
* @return Returns whether the creation is successful.
|
|
*/
|
|
bool create(const std::vector<Point3f> &pointCloud, int maxDepth = -1);
|
|
|
|
/** @brief Determine whether the point is within the space range of the specific cube.
|
|
*
|
|
* @param point The point coordinates.
|
|
* @return If point is in bound, return ture. Otherwise, false.
|
|
*/
|
|
bool isPointInBound(const Point3f& point) const;
|
|
|
|
//! Set MaxDepth for Octree.
|
|
void setMaxDepth(int maxDepth);
|
|
|
|
//! Set Box Size for Octree.
|
|
void setSize(double size);
|
|
|
|
//! Set Origin coordinates for Octree.
|
|
void setOrigin(const Point3f& origin);
|
|
|
|
//! returns true if the rootnode is NULL.
|
|
bool empty() const;
|
|
|
|
/** @brief Reset all octree parameter.
|
|
*
|
|
* Clear all the nodes of the octree and initialize the parameters.
|
|
*/
|
|
void clear();
|
|
|
|
/** @brief Delete a given point from the Octree.
|
|
*
|
|
* Delete the corresponding element from the pointList in the corresponding leaf node. If the leaf node
|
|
* does not contain other points after deletion, this node will be deleted. In the same way,
|
|
* its parent node may also be deleted if its last child is deleted.
|
|
* @param point The point coordinates.
|
|
* @return return ture if the point is deleted successfully.
|
|
*/
|
|
bool deletePoint(const Point3f& point);
|
|
|
|
/** @brief Radius Nearest Neighbor Search in Octree
|
|
*
|
|
* Search all points that are less than or equal to radius.
|
|
* And return the number of searched points.
|
|
* @param query Query point.
|
|
* @param radius Retrieved radius value.
|
|
* @param pointSet Point output. Contains searched points, and output vector is not in order.
|
|
* @param squareDistSet Dist output. Contains searched squared distance, and output vector is not in order.
|
|
* @return the number of searched points.
|
|
*/
|
|
int radiusNNSearch(const Point3f& query, float radius, std::vector<Point3f> &pointSet, std::vector<float> &squareDistSet) const;
|
|
|
|
/** @brief K Nearest Neighbor Search in Octree.
|
|
*
|
|
* Find the K nearest neighbors to the query point.
|
|
* @param query Query point.
|
|
* @param K
|
|
* @param pointSet Point output. Contains K points, arranged in order of distance from near to far.
|
|
* @param squareDistSet Dist output. Contains K squared distance, arranged in order of distance from near to far.
|
|
*/
|
|
void KNNSearch(const Point3f& query, const int K, std::vector<Point3f> &pointSet, std::vector<float> &squareDistSet) const;
|
|
|
|
protected:
|
|
struct Impl;
|
|
Ptr<Impl> p;
|
|
};
|
|
|
|
|
|
/** @brief Loads a point cloud from a file.
|
|
*
|
|
* The function loads point cloud from the specified file and returns it.
|
|
* If the cloud cannot be read, throws an error
|
|
*
|
|
* Currently, the following file formats are supported:
|
|
* - [Wavefront obj file *.obj](https://en.wikipedia.org/wiki/Wavefront_.obj_file)
|
|
* - [Polygon File Format *.ply](https://en.wikipedia.org/wiki/PLY_(file_format))
|
|
*
|
|
* @param filename Name of the file.
|
|
* @param vertices (vector of Point3f) Point coordinates of a point cloud
|
|
* @param normals (vector of Point3f) Point normals of a point cloud
|
|
*/
|
|
CV_EXPORTS_W void loadPointCloud(const String &filename, OutputArray vertices, OutputArray normals = noArray());
|
|
|
|
/** @brief Saves a point cloud to a specified file.
|
|
*
|
|
* The function saves point cloud to the specified file.
|
|
* File format is chosen based on the filename extension.
|
|
*
|
|
* @param filename Name of the file.
|
|
* @param vertices (vector of Point3f) Point coordinates of a point cloud
|
|
* @param normals (vector of Point3f) Point normals of a point cloud
|
|
*/
|
|
CV_EXPORTS_W void savePointCloud(const String &filename, InputArray vertices, InputArray normals = noArray());
|
|
|
|
/** @brief Loads a mesh from a file.
|
|
*
|
|
* The function loads mesh from the specified file and returns it.
|
|
* If the mesh cannot be read, throws an error
|
|
*
|
|
* Currently, the following file formats are supported:
|
|
* - [Wavefront obj file *.obj](https://en.wikipedia.org/wiki/Wavefront_.obj_file) (ONLY TRIANGULATED FACES)
|
|
* @param filename Name of the file.
|
|
* @param vertices (vector of Point3f) vertex coordinates of a mesh
|
|
* @param normals (vector of Point3f) vertex normals of a mesh
|
|
* @param indices (vector of vectors of int) vertex normals of a mesh
|
|
*/
|
|
CV_EXPORTS_W void loadMesh(const String &filename, OutputArray vertices, OutputArray normals, OutputArrayOfArrays indices);
|
|
|
|
/** @brief Saves a mesh to a specified file.
|
|
*
|
|
* The function saves mesh to the specified file.
|
|
* File format is chosen based on the filename extension.
|
|
*
|
|
* @param filename Name of the file.
|
|
* @param vertices (vector of Point3f) vertex coordinates of a mesh
|
|
* @param normals (vector of Point3f) vertex normals of a mesh
|
|
* @param indices (vector of vectors of int) vertex normals of a mesh
|
|
*/
|
|
CV_EXPORTS_W void saveMesh(const String &filename, InputArray vertices, InputArray normals, InputArrayOfArrays indices);
|
|
|
|
|
|
//! @} _3d
|
|
} //end namespace cv
|
|
|
|
#endif
|