- SVO2 series depth filter DepthFilter
- svo_note
- SVO(SVO: fast semi-direct monocular visual odometry)
- SVO semi-direct visual odometry
- 【DepthFilter】Depth filter
The whole network of depth filter is pulled down in detail
14 Lectures P326-327
The function implements a depth filter, which is used to calculate the depth value of a certain pixel in the image. Meaning and implications of the algorithm steps:
- Calculate the depth by triangulating the pixels of the current frame and the pixels of the reference frame.
- Transform the transformation matrix T_C_R from the reference frame to the current frame into the transformation matrix T_R_C from the current frame to the reference frame.
- Convert the reference frame pixel point pt_ref and the current frame pixel point pt_curr into the direction vectors f_ref and f_curr in the corresponding camera coordinate system.
- Normalizes f_ref and f_curr.
- According to the depth value obtained by triangulation, the position p of the corresponding point in the reference frame and the position t of the corresponding point in the current frame are calculated.
- Calculate the depth value depth_estimation according to p and t.
- Calculate the uncertainty, which is the variance depth_cov2 of the depth values.
- Gaussian fusion, which fuses the current depth value and variance with the previous value to obtain a new depth value and variance.
Among them, steps 1-5 are the process of calculating the depth value, and steps 6-8 are the process of the depth filter. See the comments in the code for the specific formula derivation.
Mathematical derivation:
Suppose the pixels in the current frame are pcur = ( ucur , vcur ) p_{cur}=(u_{cur},v_{cur})pcur=(ucur,vcur) , the pixel in the reference frame ispref = ( uref , vref ) p_{ref}=(u_{ref},v_{ref})pref=(uref,vref) , and their corresponding depths aredcur d_{cur}dcurand dref d_{ref}dref, then their coordinates in the camera coordinate system can be expressed as:
p c u r c a m = [ u c u r v c u r 1 ] d c u r − 1 p r e f c a m = [ u r e f v r e f 1 ] d r e f − 1 p_{cur}^{cam}=\begin{bmatrix}u_{cur}\\v_{cur}\\1\end{bmatrix}d_{cur}^{-1} \quad p_{ref}^{cam}=\begin{bmatrix}u_{ref}\\v_{ref}\\1\end{bmatrix}d_{ref}^{-1} pcurcam= ucurvcur1 dcur−1prefcam= urefvref1 dref−1
Among them, pcurcam p_{cur}^{cam}pcurcam 和 p r e f c a m p_{ref}^{cam} prefcamRespectively represent the coordinates of the corresponding points in the current frame and the reference frame in the camera coordinate system.
According to the geometric relationship in binocular vision, we can get the following formula:
p c u r c a m = K [ I ∣ 0 ] [ R ∣ t ] p r e f c a m p_{cur}^{cam}=K[I|0][R|t]p_{ref}^{cam} pcurcam=K[I∣0][R∣t]prefcam
Among them, KKK represents the camera internal reference matrix,III represents the identity matrix,RRR andttt represents the rotation matrix and translation vector from the reference frame to the current frame, respectively. Expand it to get:
[ u c u r v c u r 1 ] d c u r − 1 = K [ R ∣ t ] [ R T t 0 T 1 ] K − 1 [ u r e f v r e f 1 ] d r e f − 1 \begin{bmatrix}u_{cur}\\v_{cur}\\1\end{bmatrix}d_{cur}^{-1}=K[R|t]\begin{bmatrix}R^T&t\\0^T&1\end{bmatrix}K^{-1}\begin{bmatrix}u_{ref}\\v_{ref}\\1\end{bmatrix}d_{ref}^{-1} ucurvcur1 dcur−1=K[R∣t][RT0Tt1]K−1 urefvref1 dref−1
Transpose and simplify to get:
d c u r [ u c u r v c u r 1 ] = K [ R ∣ t ] [ u r e f v r e f 1 ] d_{cur}\begin{bmatrix}u_{cur}\\v_{cur}\\1\end{bmatrix}=K[R|t]\begin{bmatrix}u_{ref}\\v_{ref}\\1\end{bmatrix} dcur ucurvcur1 =K[R∣t] urefvref1
令 f c u r = K − 1 [ u c u r v c u r 1 ] f_{cur}=K^{-1}\begin{bmatrix}u_{cur}\\v_{cur}\\1\end{bmatrix} fcur=K−1 ucurvcur1 和 f r e f = K − 1 [ u r e f v r e f 1 ] f_{ref}=K^{-1}\begin{bmatrix}u_{ref}\\v_{ref}\\1\end{bmatrix} fref=K−1 urefvref1 , then the above formula can be expressed as:
d c u r ( f c u r ) = R f r e f + t d_{cur}(f_{cur})=Rf_{ref}+t dcur(fcur)=Rfref+t
Divide both sides by ∥ fcur ∥ \|f_{cur}\|∥fcur∥ , get:
d c u r f c u r ∥ f c u r ∥ = R f r e f ∥ f c u r ∥ + t ∥ f c u r ∥ d_{cur}\frac{f_{cur}}{\|f_{cur}\|}=R\frac{f_{ref}}{\|f_{cur}\|}+\frac{t}{\|f_{cur}\|} dcur∥fcur∥fcur=R∥fcur∥fref+∥fcur∥t
令 f 2 = R f r e f ∥ f c u r ∥ f_2=R\frac{f_{ref}}{\|f_{cur}\|} f2=R∥fcur∥fref 和 t 2 = t ∥ f c u r ∥ t_2=\frac{t}{\|f_{cur}\|} t2=∥fcur∥t, then the above formula can be expressed as:
d c u r f 1 = f 2 + t 2 d_{cur}f_1=f_2+t_2 dcurf1=f2+t2
其中, f 1 = f c u r ∥ f c u r ∥ f_1=\frac{f_{cur}}{\|f_{cur}\|} f1=∥fcur∥fcur. This formula shows that the depth value of the corresponding point in the current frame can be calculated by the depth value of the corresponding point in the reference frame, the rotation matrix and translation vector from the reference frame to the current frame.
We can express the above formula in matrix form:
[ f 1 T f 2 T ] [ d c u r d r e f ] = [ f 1 T t 2 f 2 T t 2 ] \begin{bmatrix}f_1^T\\f_2^T\end{bmatrix}\begin{bmatrix}d_{cur}\\d_{ref}\end{bmatrix}=\begin{bmatrix}f_1^Tt_2\\f_2^Tt_2\end{bmatrix} [f1Tf2T][dcurdref]=[f1Tt2f2Tt2]
其中, [ f 1 T f 2 T ] \begin{bmatrix}f_1^T\\f_2^T\end{bmatrix} [f1Tf2T] 和 [ f 1 T t 2 f 2 T t 2 ] \begin{bmatrix}f_1^Tt_2\\f_2^Tt_2\end{bmatrix} [f1Tt2f2Tt2] can pass the transformation matrix TRC T_R^Cfrom the reference frame to the current frameTRCto calculate.
Therefore, we can calculate the depth value by solving this system of linear equations. Specifically, we can use Gaussian elimination method or SVD decomposition to solve this system of equations. In practical implementations, SVD decomposition is usually used to solve this system of equations.
void updateDepthFilter(
const Vector2d &pt_ref, // 参考帧像素点
const Vector2d &pt_curr, // 当前帧像素点
const SE3d &T_C_R, // 参考帧到当前帧的变换矩阵
const Vector2d &epipolar_direction, // 极线方向
Mat &depth, // 存储深度值
Mat &depth_cov2) {
// 存储深度值不确定性的平方
// 将 T_C_R 转换为当前帧到参考帧的变换矩阵 T_R_C
SE3d T_R_C = T_C_R.inverse();
// 将参考帧和当前帧的像素点转换为相机坐标系下的方向向量
Vector3d f_ref = px2cam(pt_ref);
f_ref.normalize();
Vector3d f_curr = px2cam(pt_curr);
f_curr.normalize();
// 根据三角化计算深度
Vector3d t = T_R_C.translation();
Vector3d f2 = T_R_C.so3() * f_curr;
f2.normalize();
Vector2d b = Vector2d(t.dot(f_ref), t.dot(f2));
Matrix2d A;
A(0, 0) = f_ref.dot(f_ref);
A(0, 1) = -f_ref.dot(f2);
A(1, 0) = -A(0, 1);
A(1, 1) = -f2.dot(f2);
Vector2d ans = A.inverse() * b;
Vector3d xm = ans[0] * f_ref; // ref 侧的结果
Vector3d xn = t + ans[1] * f2; // cur 结果
Vector3d p_esti = (xm + xn) / 2.0; // P 的位置,取两者的平均
double depth_estimation = p_esti.norm(); // 深度值
// 计算不确定性(以一个像素为误差)
Vector3d p = f_ref * depth_estimation;
Vector3d a = p - t;
double t_norm = t.norm();
double a_norm = a.norm();
double alpha = acos(f_ref.dot(t) / t_norm);
double beta = acos(-a.dot(t) / (a_norm * t_norm));
Vector3d f_curr_prime = px2cam(pt_curr + epipolar_direction);
f_curr_prime.normalize();
double beta_prime = acos(f_curr_prime.dot(-t) / t_norm);
double gamma = M_PI - alpha - beta_prime;
double p_prime = t_norm * sin(beta_prime) / sin(gamma);
double d_cov = p_prime - depth_estimation;
double d_cov2 = d_cov * d_cov;
// 高斯融合
double mu = depth.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))];
double sigma2 = depth_cov2.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))];
double mu_fuse = (d_cov2 * mu + sigma2 * depth_estimation) / (sigma2 + d_cov2);
double sigma_fuse2 = (sigma2 * d_cov2) / (sigma2 + d_cov2);
depth.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))] = mu_fuse;
depth_cov2.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))] = sigma_fuse2;
return true;
}
The entire code implementation:
#include <iostream>
#include <vector>
#include <fstream>
using namespace std;
#include <boost/timer.hpp>
// for sophus
#include <sophus/se3.hpp>
using Sophus::SE3d;
// for eigen
#include <Eigen/Core>
#include <Eigen/Geometry>
using namespace Eigen;
#include <opencv2/core/core.hpp>
#include <opencv2/highgui/highgui.hpp>
#include <opencv2/imgproc/imgproc.hpp>
using namespace cv;
/**********************************************
* 本程序演示了单目相机在已知轨迹下的稠密深度估计
* 使用极线搜索 + NCC 匹配的方式,与书本的 12.2 节对应
* 请注意本程序并不完美,你完全可以改进它——我其实在故意暴露一些问题(这是借口)。
***********************************************/
// ------------------------------------------------------------------
// parameters
const int boarder = 20; // 边缘宽度
const int width = 640; // 图像宽度
const int height = 480; // 图像高度
const double fx = 481.2f; // 相机内参
const double fy = -480.0f;
const double cx = 319.5f;
const double cy = 239.5f;
const int ncc_window_size = 3; // NCC 取的窗口半宽度
const int ncc_area = (2 * ncc_window_size + 1) * (2 * ncc_window_size + 1); // NCC窗口面积
const double min_cov = 0.1; // 收敛判定:最小方差
const double max_cov = 10; // 发散判定:最大方差
// ------------------------------------------------------------------
// 重要的函数
/// 从 REMODE 数据集读取数据
bool readDatasetFiles(
const string &path,
vector<string> &color_image_files,
vector<SE3d> &poses,
cv::Mat &ref_depth
);
/**
* 根据新的图像更新深度估计
* @param ref 参考图像
* @param curr 当前图像
* @param T_C_R 参考图像到当前图像的位姿
* @param depth 深度
* @param depth_cov 深度方差
* @return 是否成功
*/
void update(
const Mat &ref,
const Mat &curr,
const SE3d &T_C_R,
Mat &depth,
Mat &depth_cov2
);
/**
* 极线搜索
* @param ref 参考图像
* @param curr 当前图像
* @param T_C_R 位姿
* @param pt_ref 参考图像中点的位置
* @param depth_mu 深度均值
* @param depth_cov 深度方差
* @param pt_curr 当前点
* @param epipolar_direction 极线方向
* @return 是否成功
*/
bool epipolarSearch(
const Mat &ref,
const Mat &curr,
const SE3d &T_C_R,
const Vector2d &pt_ref,
const double &depth_mu,
const double &depth_cov,
Vector2d &pt_curr,
Vector2d &epipolar_direction
);
/**
* 更新深度滤波器
* @param pt_ref 参考图像点
* @param pt_curr 当前图像点
* @param T_C_R 位姿
* @param epipolar_direction 极线方向
* @param depth 深度均值
* @param depth_cov2 深度方向
* @return 是否成功
*/
bool updateDepthFilter(
const Vector2d &pt_ref,
const Vector2d &pt_curr,
const SE3d &T_C_R,
const Vector2d &epipolar_direction,
Mat &depth,
Mat &depth_cov2
);
/**
* 计算 NCC 评分
* @param ref 参考图像
* @param curr 当前图像
* @param pt_ref 参考点
* @param pt_curr 当前点
* @return NCC评分
*/
double NCC(const Mat &ref, const Mat &curr, const Vector2d &pt_ref, const Vector2d &pt_curr);
// 双线性灰度插值
inline double getBilinearInterpolatedValue(const Mat &img, const Vector2d &pt) {
uchar *d = &img.data[int(pt(1, 0)) * img.step + int(pt(0, 0))];
double xx = pt(0, 0) - floor(pt(0, 0));
double yy = pt(1, 0) - floor(pt(1, 0));
return ((1 - xx) * (1 - yy) * double(d[0]) +
xx * (1 - yy) * double(d[1]) +
(1 - xx) * yy * double(d[img.step]) +
xx * yy * double(d[img.step + 1])) / 255.0;
}
// ------------------------------------------------------------------
// 一些小工具
// 显示估计的深度图
void plotDepth(const Mat &depth_truth, const Mat &depth_estimate);
// 像素到相机坐标系
inline Vector3d px2cam(const Vector2d px) {
return Vector3d(
(px(0, 0) - cx) / fx,
(px(1, 0) - cy) / fy,
1
);
}
// 相机坐标系到像素
inline Vector2d cam2px(const Vector3d p_cam) {
return Vector2d(
p_cam(0, 0) * fx / p_cam(2, 0) + cx,
p_cam(1, 0) * fy / p_cam(2, 0) + cy
);
}
// 检测一个点是否在图像边框内
inline bool inside(const Vector2d &pt) {
return pt(0, 0) >= boarder && pt(1, 0) >= boarder
&& pt(0, 0) + boarder < width && pt(1, 0) + boarder <= height;
}
// 显示极线匹配
void showEpipolarMatch(const Mat &ref, const Mat &curr, const Vector2d &px_ref, const Vector2d &px_curr);
// 显示极线
void showEpipolarLine(const Mat &ref, const Mat &curr, const Vector2d &px_ref, const Vector2d &px_min_curr,
const Vector2d &px_max_curr);
/// 评测深度估计
void evaludateDepth(const Mat &depth_truth, const Mat &depth_estimate);
// ------------------------------------------------------------------
int main(int argc, char **argv) {
if (argc != 2) {
cout << "Usage: dense_mapping path_to_test_dataset" << endl;
return -1;
}
// 从数据集读取数据
vector<string> color_image_files;
vector<SE3d> poses_TWC;
Mat ref_depth;
bool ret = readDatasetFiles(argv[1], color_image_files, poses_TWC, ref_depth);
if (ret == false) {
cout << "Reading image files failed!" << endl;
return -1;
}
cout << "read total " << color_image_files.size() << " files." << endl;
// 第一张图
Mat ref = imread(color_image_files[0], 0); // gray-scale image
SE3d pose_ref_TWC = poses_TWC[0];
double init_depth = 3.0; // 深度初始值
double init_cov2 = 3.0; // 方差初始值
Mat depth(height, width, CV_64F, init_depth); // 深度图
Mat depth_cov2(height, width, CV_64F, init_cov2); // 深度图方差
for (int index = 1; index < color_image_files.size(); index++) {
cout << "*** loop " << index << " ***" << endl;
Mat curr = imread(color_image_files[index], 0);
if (curr.data == nullptr) continue;
SE3d pose_curr_TWC = poses_TWC[index];
SE3d pose_T_C_R = pose_curr_TWC.inverse() * pose_ref_TWC; // 坐标转换关系: T_C_W * T_W_R = T_C_R
update(ref, curr, pose_T_C_R, depth, depth_cov2);
evaludateDepth(ref_depth, depth);
plotDepth(ref_depth, depth);
imshow("image", curr);
waitKey(0);
}
cout << "estimation returns, saving depth map ..." << endl;
imwrite("depth.png", depth);
cout << "done." << endl;
return 0;
}
bool readDatasetFiles(
const string &path,
vector<string> &color_image_files,
std::vector<SE3d> &poses,
cv::Mat &ref_depth) {
ifstream fin(path + "/first_200_frames_traj_over_table_input_sequence.txt");
if (!fin) return false;
while (!fin.eof()) {
// 数据格式:图像文件名 tx, ty, tz, qx, qy, qz, qw ,注意是 TWC 而非 TCW
string image;
fin >> image;
double data[7];
for (double &d:data) fin >> d;
color_image_files.push_back(path + string("/images/") + image);
poses.push_back(
SE3d(Quaterniond(data[6], data[3], data[4], data[5]),
Vector3d(data[0], data[1], data[2]))
);
if (!fin.good()) break;
}
fin.close();
// load reference depth
fin.open(path + "/depthmaps/scene_000.depth");
ref_depth = cv::Mat(height, width, CV_64F);
if (!fin) return false;
for (int y = 0; y < height; y++)
for (int x = 0; x < width; x++) {
double depth = 0;
fin >> depth;
ref_depth.ptr<double>(y)[x] = depth / 100.0;
}
return true;
}
// 对整个深度图进行更新
void update(const Mat &ref, const Mat &curr, const SE3d &T_C_R, Mat &depth, Mat &depth_cov2) {
for (int x = boarder; x < width - boarder; x++)
for (int y = boarder; y < height - boarder; y++) {
// 遍历每个像素
if (depth_cov2.ptr<double>(y)[x] < min_cov || depth_cov2.ptr<double>(y)[x] > max_cov) // 深度已收敛或发散
continue;
// 在极线上搜索 (x,y) 的匹配
Vector2d pt_curr;
Vector2d epipolar_direction;
bool ret = epipolarSearch(
ref,
curr,
T_C_R,
Vector2d(x, y),
depth.ptr<double>(y)[x],
sqrt(depth_cov2.ptr<double>(y)[x]),
pt_curr,
epipolar_direction
);
if (ret == false) // 匹配失败
continue;
// 取消该注释以显示匹配
// showEpipolarMatch(ref, curr, Vector2d(x, y), pt_curr);
// 匹配成功,更新深度图
updateDepthFilter(Vector2d(x, y), pt_curr, T_C_R, epipolar_direction, depth, depth_cov2);
}
}
// 极线搜索
// 方法见书 12.2 12.3 两节
bool epipolarSearch(
const Mat &ref, const Mat &curr,
const SE3d &T_C_R, const Vector2d &pt_ref,
const double &depth_mu, const double &depth_cov,
Vector2d &pt_curr, Vector2d &epipolar_direction) {
Vector3d f_ref = px2cam(pt_ref);
f_ref.normalize();
Vector3d P_ref = f_ref * depth_mu; // 参考帧的 P 向量
Vector2d px_mean_curr = cam2px(T_C_R * P_ref); // 按深度均值投影的像素
double d_min = depth_mu - 3 * depth_cov, d_max = depth_mu + 3 * depth_cov;
if (d_min < 0.1) d_min = 0.1;
Vector2d px_min_curr = cam2px(T_C_R * (f_ref * d_min)); // 按最小深度投影的像素
Vector2d px_max_curr = cam2px(T_C_R * (f_ref * d_max)); // 按最大深度投影的像素
Vector2d epipolar_line = px_max_curr - px_min_curr; // 极线(线段形式)
epipolar_direction = epipolar_line; // 极线方向
epipolar_direction.normalize();
double half_length = 0.5 * epipolar_line.norm(); // 极线线段的半长度
if (half_length > 100) half_length = 100; // 我们不希望搜索太多东西
// 取消此句注释以显示极线(线段)
//showEpipolarLine( ref, curr, pt_ref, px_min_curr, px_max_curr );
// 在极线上搜索,以深度均值点为中心,左右各取半长度
double best_ncc = -1.0;
Vector2d best_px_curr;
for (double l = -half_length; l <= half_length; l += 0.7) {
// l+=sqrt(2)
Vector2d px_curr = px_mean_curr + l * epipolar_direction; // 待匹配点
if (!inside(px_curr))
continue;
// 计算待匹配点与参考帧的 NCC
double ncc = NCC(ref, curr, pt_ref, px_curr);
if (ncc > best_ncc) {
best_ncc = ncc;
best_px_curr = px_curr;
}
}
if (best_ncc < 0.85f) // 只相信 NCC 很高的匹配
return false;
pt_curr = best_px_curr;
return true;
}
double NCC(
const Mat &ref, const Mat &curr,
const Vector2d &pt_ref, const Vector2d &pt_curr) {
// 零均值-归一化互相关
// 先算均值
double mean_ref = 0, mean_curr = 0;
vector<double> values_ref, values_curr; // 参考帧和当前帧的均值
for (int x = -ncc_window_size; x <= ncc_window_size; x++)
for (int y = -ncc_window_size; y <= ncc_window_size; y++) {
double value_ref = double(ref.ptr<uchar>(int(y + pt_ref(1, 0)))[int(x + pt_ref(0, 0))]) / 255.0;
mean_ref += value_ref;
double value_curr = getBilinearInterpolatedValue(curr, pt_curr + Vector2d(x, y));
mean_curr += value_curr;
values_ref.push_back(value_ref);
values_curr.push_back(value_curr);
}
mean_ref /= ncc_area;
mean_curr /= ncc_area;
// 计算 Zero mean NCC
double numerator = 0, demoniator1 = 0, demoniator2 = 0;
for (int i = 0; i < values_ref.size(); i++) {
double n = (values_ref[i] - mean_ref) * (values_curr[i] - mean_curr);
numerator += n;
demoniator1 += (values_ref[i] - mean_ref) * (values_ref[i] - mean_ref);
demoniator2 += (values_curr[i] - mean_curr) * (values_curr[i] - mean_curr);
}
return numerator / sqrt(demoniator1 * demoniator2 + 1e-10); // 防止分母出现零
}
bool updateDepthFilter(
const Vector2d &pt_ref,
const Vector2d &pt_curr,
const SE3d &T_C_R,
const Vector2d &epipolar_direction,
Mat &depth,
Mat &depth_cov2) {
// 不知道这段还有没有人看
// 用三角化计算深度
SE3d T_R_C = T_C_R.inverse();
Vector3d f_ref = px2cam(pt_ref);
f_ref.normalize();
Vector3d f_curr = px2cam(pt_curr);
f_curr.normalize();
// 方程
// d_ref * f_ref = d_cur * ( R_RC * f_cur ) + t_RC
// f2 = R_RC * f_cur
// 转化成下面这个矩阵方程组
// => [ f_ref^T f_ref, -f_ref^T f2 ] [d_ref] [f_ref^T t]
// [ f_2^T f_ref, -f2^T f2 ] [d_cur] = [f2^T t ]
Vector3d t = T_R_C.translation();
Vector3d f2 = T_R_C.so3() * f_curr;
Vector2d b = Vector2d(t.dot(f_ref), t.dot(f2));
Matrix2d A;
A(0, 0) = f_ref.dot(f_ref);
A(0, 1) = -f_ref.dot(f2);
A(1, 0) = -A(0, 1);
A(1, 1) = -f2.dot(f2);
Vector2d ans = A.inverse() * b;
Vector3d xm = ans[0] * f_ref; // ref 侧的结果
Vector3d xn = t + ans[1] * f2; // cur 结果
Vector3d p_esti = (xm + xn) / 2.0; // P的位置,取两者的平均
double depth_estimation = p_esti.norm(); // 深度值
// 计算不确定性(以一个像素为误差)
Vector3d p = f_ref * depth_estimation;
Vector3d a = p - t;
double t_norm = t.norm();
double a_norm = a.norm();
double alpha = acos(f_ref.dot(t) / t_norm);
double beta = acos(-a.dot(t) / (a_norm * t_norm));
Vector3d f_curr_prime = px2cam(pt_curr + epipolar_direction);
f_curr_prime.normalize();
double beta_prime = acos(f_curr_prime.dot(-t) / t_norm);
double gamma = M_PI - alpha - beta_prime;
double p_prime = t_norm * sin(beta_prime) / sin(gamma);
double d_cov = p_prime - depth_estimation;
double d_cov2 = d_cov * d_cov;
// 高斯融合
double mu = depth.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))];
double sigma2 = depth_cov2.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))];
double mu_fuse = (d_cov2 * mu + sigma2 * depth_estimation) / (sigma2 + d_cov2);
double sigma_fuse2 = (sigma2 * d_cov2) / (sigma2 + d_cov2);
depth.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))] = mu_fuse;
depth_cov2.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))] = sigma_fuse2;
return true;
}
/*
这个函数实现了一个深度滤波器,用于计算图像中某个像素点的深度值。下面是每个步骤的含义和相关的公式推导:
1. 将当前帧的像素点和参考帧的像素点通过三角化计算深度。
2. 将参考帧到当前帧的变换矩阵 T_C_R 转换为当前帧到参考帧的变换矩阵 T_R_C。
3. 将参考帧像素点 pt_ref 和当前帧像素点 pt_curr 转换为对应的相机坐标系下的方向向量 f_ref 和 f_curr。
4. 对 f_ref 和 f_curr 进行归一化。
5. 根据三角化得到的深度值,计算出参考帧中对应点的位置 p,以及当前帧中对应点的位置 t。
6. 根据 p 和 t 计算出两个方向向量 xm 和 xn,分别是参考帧中对应点和当前帧中对应点到相机中心的向量。
7. 将 xm 和 xn 取平均得到 P 的位置 p_esti。
8. 计算 P 的深度值 depth_estimation,即 p_esti 的模长。
9. 计算深度值的不确定性 d_cov2,以一个像素为误差。
10. 将计算得到的深度值和不确定性与之前存储的深度值和不确定性进行高斯融合,得到新的深度值和不确定性。
11. 将新的深度值和不确定性存储到 depth 和 depth_cov2 中。
*/
bool updateDepthFilter2(
const Vector2d &pt_ref, // 参考帧像素点
const Vector2d &pt_curr, // 当前帧像素点
const SE3d &T_C_R, // 参考帧到当前帧的变换矩阵
const Vector2d &epipolar_direction, // 极线方向
Mat &depth, // 存储深度值
Mat &depth_cov2) {
// 存储深度值不确定性的平方
// 将 T_C_R 转换为当前帧到参考帧的变换矩阵 T_R_C
SE3d T_R_C = T_C_R.inverse();
// 将参考帧和当前帧的像素点转换为相机坐标系下的方向向量
Vector3d f_ref = px2cam(pt_ref);
f_ref.normalize();
Vector3d f_curr = px2cam(pt_curr);
f_curr.normalize();
// 根据三角化计算深度
Vector3d t = T_R_C.translation();
Vector3d f2 = T_R_C.so3() * f_curr;
f2.normalize();
Vector2d b = Vector2d(t.dot(f_ref), t.dot(f2));
Matrix2d A;
A(0, 0) = f_ref.dot(f_ref);
A(0, 1) = -f_ref.dot(f2);
A(1, 0) = -A(0, 1);
A(1, 1) = -f2.dot(f2);
Vector2d ans = A.inverse() * b;
Vector3d xm = ans[0] * f_ref; // ref 侧的结果
Vector3d xn = t + ans[1] * f2; // cur 结果
Vector3d p_esti = (xm + xn) / 2.0; // P 的位置,取两者的平均
double depth_estimation = p_esti.norm(); // 深度值
// 计算不确定性(以一个像素为误差)
Vector3d p = f_ref * depth_estimation;
Vector3d a = p - t;
double t_norm = t.norm();
double a_norm = a.norm();
double alpha = acos(f_ref.dot(t) / t_norm);
double beta = acos(-a.dot(t) / (a_norm * t_norm));
Vector3d f_curr_prime = px2cam(pt_curr + epipolar_direction);
f_curr_prime.normalize();
double beta_prime = acos(f_curr_prime.dot(-t) / t_norm);
double gamma = M_PI - alpha - beta_prime;
double p_prime = t_norm * sin(beta_prime) / sin(gamma);
double d_cov = p_prime - depth_estimation; //观测的均值 /mu_obs
double d_cov2 = d_cov * d_cov; // 观测的不确定度/sigma^2_obs
// 高斯融合
double mu = depth.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))];
double sigma2 = depth_cov2.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))];
double mu_fuse = (d_cov2 * mu + sigma2 * depth_estimation) / (sigma2 + d_cov2);
double sigma_fuse2 = (sigma2 * d_cov2) / (sigma2 + d_cov2);
depth.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))] = mu_fuse;
depth_cov2.ptr<double>(int(pt_ref(1, 0)))[int(pt_ref(0, 0))] = sigma_fuse2;
return true;
}
// 后面这些太简单我就不注释了(其实是因为懒)
void plotDepth(const Mat &depth_truth, const Mat &depth_estimate) {
imshow("depth_truth", depth_truth * 0.4);
imshow("depth_estimate", depth_estimate * 0.4);
imshow("depth_error", depth_truth - depth_estimate);
waitKey(1);
}
void evaludateDepth(const Mat &depth_truth, const Mat &depth_estimate) {
double ave_depth_error = 0; // 平均误差
double ave_depth_error_sq = 0; // 平方误差
int cnt_depth_data = 0;
for (int y = boarder; y < depth_truth.rows - boarder; y++)
for (int x = boarder; x < depth_truth.cols - boarder; x++) {
double error = depth_truth.ptr<double>(y)[x] - depth_estimate.ptr<double>(y)[x];
ave_depth_error += error;
ave_depth_error_sq += error * error;
cnt_depth_data++;
}
ave_depth_error /= cnt_depth_data;
ave_depth_error_sq /= cnt_depth_data;
cout << "Average squared error = " << ave_depth_error_sq << ", average error: " << ave_depth_error << endl;
}
void showEpipolarMatch(const Mat &ref, const Mat &curr, const Vector2d &px_ref, const Vector2d &px_curr) {
Mat ref_show, curr_show;
cv::cvtColor(ref, ref_show, CV_GRAY2BGR);
cv::cvtColor(curr, curr_show, CV_GRAY2BGR);
cv::circle(ref_show, cv::Point2f(px_ref(0, 0), px_ref(1, 0)), 5, cv::Scalar(0, 0, 250), 2);
cv::circle(curr_show, cv::Point2f(px_curr(0, 0), px_curr(1, 0)), 5, cv::Scalar(0, 0, 250), 2);
imshow("ref", ref_show);
imshow("curr", curr_show);
waitKey(1);
}
void showEpipolarLine(const Mat &ref, const Mat &curr, const Vector2d &px_ref, const Vector2d &px_min_curr,
const Vector2d &px_max_curr) {
Mat ref_show, curr_show;
cv::cvtColor(ref, ref_show, CV_GRAY2BGR);
cv::cvtColor(curr, curr_show, CV_GRAY2BGR);
cv::circle(ref_show, cv::Point2f(px_ref(0, 0), px_ref(1, 0)), 5, cv::Scalar(0, 255, 0), 2);
cv::circle(curr_show, cv::Point2f(px_min_curr(0, 0), px_min_curr(1, 0)), 5, cv::Scalar(0, 255, 0), 2);
cv::circle(curr_show, cv::Point2f(px_max_curr(0, 0), px_max_curr(1, 0)), 5, cv::Scalar(0, 255, 0), 2);
cv::line(curr_show, Point2f(px_min_curr(0, 0), px_min_curr(1, 0)), Point2f(px_max_curr(0, 0), px_max_curr(1, 0)),
Scalar(0, 255, 0), 1);
imshow("ref", ref_show);
imshow("curr", curr_show);
waitKey(1);
}