examples/snavely_reprojection_error.h - ceres-solver - Git at Google

 // Ceres Solver - A fast non-linear least squares minimizer
 // Copyright 2015 Google Inc. All rights reserved.
 // http://ceres-solver.org/
 //
 // Redistribution and use in source and binary forms, with or without
 // modification, are permitted provided that the following conditions are met:
 //
 // * Redistributions of source code must retain the above copyright notice,
 //   this list of conditions and the following disclaimer.
 // * Redistributions in binary form must reproduce the above copyright notice,
 //   this list of conditions and the following disclaimer in the documentation
 //   and/or other materials provided with the distribution.
 // * Neither the name of Google Inc. nor the names of its contributors may be
 //   used to endorse or promote products derived from this software without
 //   specific prior written permission.
 //
 // THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
 // AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
 // IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
 // ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT OWNER OR CONTRIBUTORS BE
 // LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR
 // CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF
 // SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS
 // INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN
 // CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)
 // ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
 // POSSIBILITY OF SUCH DAMAGE.
 //
 // Author: sameeragarwal@google.com (Sameer Agarwal)
 //
 // Templated struct implementing the camera model and residual
 // computation for bundle adjustment used by Noah Snavely's Bundler
 // SfM system. This is also the camera model/residual for the bundle
 // adjustment problems in the BAL dataset. It is templated so that we
 // can use Ceres's automatic differentiation to compute analytic
 // jacobians.
 //
 // For details see: http://phototour.cs.washington.edu/bundler/
 // and http://grail.cs.washington.edu/projects/bal/

 #ifndef CERES_EXAMPLES_SNAVELY_REPROJECTION_ERROR_H_
 #define CERES_EXAMPLES_SNAVELY_REPROJECTION_ERROR_H_

 #include "ceres/rotation.h"

 namespace ceres {
 namespace examples {

 // 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 using a Quaternion manifold.
     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];
     const T yp = -p[1] / p[2];

     // 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;
 };

 }  // namespace examples
 }  // namespace ceres

 #endif  // CERES_EXAMPLES_SNAVELY_REPROJECTION_ERROR_H_
	// Ceres Solver - A fast non-linear least squares minimizer
	// Copyright 2015 Google Inc. All rights reserved.
	// http://ceres-solver.org/
	//
	// Redistribution and use in source and binary forms, with or without
	// modification, are permitted provided that the following conditions are met:
	//
	// * Redistributions of source code must retain the above copyright notice,
	// this list of conditions and the following disclaimer.
	// * Redistributions in binary form must reproduce the above copyright notice,
	// this list of conditions and the following disclaimer in the documentation
	// and/or other materials provided with the distribution.
	// * Neither the name of Google Inc. nor the names of its contributors may be
	// used to endorse or promote products derived from this software without
	// specific prior written permission.
	//
	// THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
	// AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
	// IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
	// ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT OWNER OR CONTRIBUTORS BE
	// LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR
	// CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF
	// SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS
	// INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN
	// CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)
	// ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
	// POSSIBILITY OF SUCH DAMAGE.
	//
	// Author: sameeragarwal@google.com (Sameer Agarwal)
	//
	// Templated struct implementing the camera model and residual
	// computation for bundle adjustment used by Noah Snavely's Bundler
	// SfM system. This is also the camera model/residual for the bundle
	// adjustment problems in the BAL dataset. It is templated so that we
	// can use Ceres's automatic differentiation to compute analytic
	// jacobians.
	//
	// For details see: http://phototour.cs.washington.edu/bundler/
	// and http://grail.cs.washington.edu/projects/bal/

	#ifndef CERES_EXAMPLES_SNAVELY_REPROJECTION_ERROR_H_
	#define CERES_EXAMPLES_SNAVELY_REPROJECTION_ERROR_H_

	#include "ceres/rotation.h"

	namespace ceres {
	namespace examples {

	// 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 using a Quaternion manifold.
	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];
	const T yp = -p[1] / p[2];

	// 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;
	};

	} // namespace examples
	} // namespace ceres

	#endif // CERES_EXAMPLES_SNAVELY_REPROJECTION_ERROR_H_