• ceres---相机重投影误差


    相机重投影误差

    相机归一化公式:

    相机归一化与外参变换公式:

    相机畸变:

     

    代码:

    // Templated pinhole camera model for used with Ceres.  The camera is
    // parameterized using 9 parameters: 3 for rotation, 3 for translation, 1 for
    // focal length and 2 for radial distortion. The principal point is not modeled
    // (i.e. it is assumed be located at the image center).
    struct SnavelyReprojectionError {
      SnavelyReprojectionError(double observed_x, double observed_y)
          : observed_x(observed_x), observed_y(observed_y) {}
    
      template <typename T>
      bool operator()(const T* const camera,
                      const T* const point,
                      T* residuals) const {
        // camera[0,1,2] are the angle-axis rotation.
        T p[3];
        AngleAxisRotatePoint(camera, point, p);
    
        // camera[3,4,5] are the translation.
        p[0] += camera[3];
        p[1] += camera[4];
        p[2] += camera[5];
    
        // Compute the center of distortion. The sign change comes from
        // the camera model that Noah Snavely's Bundler assumes, whereby
        // the camera coordinate system has a negative z axis.
        const T xp = - p[0] / p[2];
        const T yp = - p[1] / p[2];
    
        // Apply second and fourth order radial distortion.
        const T& l1 = camera[7];
        const T& l2 = camera[8];
        const T r2 = xp*xp + yp*yp;
        const T distortion = 1.0 + r2  * (l1 + l2  * r2);
    
    
        // Compute final projected point position.
        const T& focal = camera[6];
        const T predicted_x = focal * distortion * xp;
        const T predicted_y = focal * distortion * yp;
    
        // The error is the difference between the predicted and observed position.
        residuals[0] = predicted_x - observed_x;
        residuals[1] = predicted_y - observed_y;
    
        return true;
      }
    
      // Factory to hide the construction of the CostFunction object from
      // the client code.
      static ceres::CostFunction* Create(const double observed_x,
                                         const double observed_y) {
        return (new ceres::AutoDiffCostFunction<SnavelyReprojectionError, 2, 9, 3>(
                    new SnavelyReprojectionError(observed_x, observed_y)));
      }
    
      double observed_x;
      double observed_y;
    };
    
    // Templated pinhole camera model for used with Ceres.  The camera is
    // parameterized using 10 parameters. 4 for rotation, 3 for
    // translation, 1 for focal length and 2 for radial distortion. The
    // principal point is not modeled (i.e. it is assumed be located at
    // the image center).
    struct SnavelyReprojectionErrorWithQuaternions {
      // (u, v): the position of the observation with respect to the image
      // center point.
      SnavelyReprojectionErrorWithQuaternions(double observed_x, double observed_y)
          : observed_x(observed_x), observed_y(observed_y) {}
    
      template <typename T>
      bool operator()(const T* const camera,
                      const T* const point,
                      T* residuals) const {
        // camera[0,1,2,3] is are the rotation of the camera as a quaternion.
        //
        // We use QuaternionRotatePoint as it does not assume that the
        // quaternion is normalized, since one of the ways to run the
        // bundle adjuster is to let Ceres optimize all 4 quaternion
        // parameters without a local parameterization.
        T p[3];
        QuaternionRotatePoint(camera, point, p);
    
        p[0] += camera[4];
        p[1] += camera[5];
        p[2] += camera[6];
    
        // Compute the center of distortion. The sign change comes from
        // the camera model that Noah Snavely's Bundler assumes, whereby
        // the camera coordinate system has a negative z axis.
        const T xp = - p[0] / p[2];   //  x/z
        const T yp = - p[1] / p[2];    // y/z
    
        // Apply second and fourth order radial distortion.
        const T& l1 = camera[8];
        const T& l2 = camera[9];
    
        const T r2 = xp*xp + yp*yp;
        const T distortion = 1.0 + r2  * (l1 + l2  * r2);
    
        // Compute final projected point position.
        const T& focal = camera[7];
        const T predicted_x = focal * distortion * xp;
        const T predicted_y = focal * distortion * yp;
    
        // The error is the difference between the predicted and observed position.
        residuals[0] = predicted_x - observed_x;
        residuals[1] = predicted_y - observed_y;
    
        return true;
      }
    
      // Factory to hide the construction of the CostFunction object from
      // the client code.
      static ceres::CostFunction* Create(const double observed_x,
                                         const double observed_y) {
        return (new ceres::AutoDiffCostFunction<
                SnavelyReprojectionErrorWithQuaternions, 2, 10, 3>(
                    new SnavelyReprojectionErrorWithQuaternions(observed_x,
                                                                observed_y)));
      }
    
      double observed_x;
      double observed_y;
    };
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  • 原文地址:https://www.cnblogs.com/lovebay/p/14862989.html
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