Files
ceres-solver/examples/ellipse_approximation.cc
T
Sergey Sharybin 54ba6c27b5 Fix missing declaration warnings in Ceres code
This commit includes the following:

- Changes to CMake to make it safer to see which compiler flags are supported,
  so this way we do not need to worry about version checks in CMake.

- Unix platforms (which includes both Linux and Apple as far as i can tell)
  will now enable -Wmissing-declarations warning for the whole Ceres.

- Changes in all sources to solve missing declaration warning. In most cases
  it was either matter of using static qualifier or moving functions to an
  anonymous namespace.

  In one case the function got removed, since it seems to be unused.

  Additionally, in slam examples there was a non-inlined function implementation
  in a header, which is a direct way to cause linking errors if other .cc file
  will include that helper header.

- All third party sources (which is currently only gmock) has this extra
  paranoid warning disabled.

This warning is important in the following cases:

- Detect helper functions which are not needed anymore.
- Avoid unnoticed pollution of namespace.
- Avoid bad level calls.
- Avoid missing updates in header files after changes in implementation file.
- Helps integrating Ceres into software where paranoid warnings are important.

Change-Id: I9b1044aced3910d8c6b2356cfe2bf57f3c8c58db
2019-04-23 12:16:28 +02:00

453 lines
15 KiB
C++

// 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: richie.stebbing@gmail.com (Richard Stebbing)
//
// This fits points randomly distributed on an ellipse with an approximate
// line segment contour. This is done by jointly optimizing the control points
// of the line segment contour along with the preimage positions for the data
// points. The purpose of this example is to show an example use case for
// dynamic_sparsity, and how it can benefit problems which are numerically
// dense but dynamically sparse.
#include <cmath>
#include <vector>
#include "ceres/ceres.h"
#include "glog/logging.h"
// Data generated with the following Python code.
// import numpy as np
// np.random.seed(1337)
// t = np.linspace(0.0, 2.0 * np.pi, 212, endpoint=False)
// t += 2.0 * np.pi * 0.01 * np.random.randn(t.size)
// theta = np.deg2rad(15)
// a, b = np.cos(theta), np.sin(theta)
// R = np.array([[a, -b],
// [b, a]])
// Y = np.dot(np.c_[4.0 * np.cos(t), np.sin(t)], R.T)
const int kYRows = 212;
const int kYCols = 2;
const double kYData[kYRows * kYCols] = {
+3.871364e+00, +9.916027e-01,
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+3.865424e+00, +1.028474e+00
};
ceres::ConstMatrixRef kY(kYData, kYRows, kYCols);
class PointToLineSegmentContourCostFunction : public ceres::CostFunction {
public:
PointToLineSegmentContourCostFunction(const int num_segments,
const Eigen::Vector2d& y)
: num_segments_(num_segments), y_(y) {
// The first parameter is the preimage position.
mutable_parameter_block_sizes()->push_back(1);
// The next parameters are the control points for the line segment contour.
for (int i = 0; i < num_segments_; ++i) {
mutable_parameter_block_sizes()->push_back(2);
}
set_num_residuals(2);
}
virtual bool Evaluate(const double* const* x,
double* residuals,
double** jacobians) const {
// Convert the preimage position `t` into a segment index `i0` and the
// line segment interpolation parameter `u`. `i1` is the index of the next
// control point.
const double t = ModuloNumSegments(*x[0]);
CHECK_GE(t, 0.0);
CHECK_LT(t, num_segments_);
const int i0 = floor(t), i1 = (i0 + 1) % num_segments_;
const double u = t - i0;
// Linearly interpolate between control points `i0` and `i1`.
residuals[0] = y_[0] - ((1.0 - u) * x[1 + i0][0] + u * x[1 + i1][0]);
residuals[1] = y_[1] - ((1.0 - u) * x[1 + i0][1] + u * x[1 + i1][1]);
if (jacobians == NULL) {
return true;
}
if (jacobians[0] != NULL) {
jacobians[0][0] = x[1 + i0][0] - x[1 + i1][0];
jacobians[0][1] = x[1 + i0][1] - x[1 + i1][1];
}
for (int i = 0; i < num_segments_; ++i) {
if (jacobians[i + 1] != NULL) {
ceres::MatrixRef(jacobians[i + 1], 2, 2).setZero();
if (i == i0) {
jacobians[i + 1][0] = -(1.0 - u);
jacobians[i + 1][3] = -(1.0 - u);
} else if (i == i1) {
jacobians[i + 1][0] = -u;
jacobians[i + 1][3] = -u;
}
}
}
return true;
}
static ceres::CostFunction* Create(const int num_segments,
const Eigen::Vector2d& y) {
return new PointToLineSegmentContourCostFunction(num_segments, y);
}
private:
inline double ModuloNumSegments(const double t) const {
return t - num_segments_ * floor(t / num_segments_);
}
const int num_segments_;
const Eigen::Vector2d y_;
};
class EuclideanDistanceFunctor {
public:
explicit EuclideanDistanceFunctor(const double& sqrt_weight)
: sqrt_weight_(sqrt_weight) {}
template <typename T>
bool operator()(const T* x0, const T* x1, T* residuals) const {
residuals[0] = sqrt_weight_ * (x0[0] - x1[0]);
residuals[1] = sqrt_weight_ * (x0[1] - x1[1]);
return true;
}
static ceres::CostFunction* Create(const double sqrt_weight) {
return new ceres::AutoDiffCostFunction<EuclideanDistanceFunctor, 2, 2, 2>(
new EuclideanDistanceFunctor(sqrt_weight));
}
private:
const double sqrt_weight_;
};
static bool SolveWithFullReport(ceres::Solver::Options options,
ceres::Problem* problem,
bool dynamic_sparsity) {
options.dynamic_sparsity = dynamic_sparsity;
ceres::Solver::Summary summary;
ceres::Solve(options, problem, &summary);
std::cout << "####################" << std::endl;
std::cout << "dynamic_sparsity = " << dynamic_sparsity << std::endl;
std::cout << "####################" << std::endl;
std::cout << summary.FullReport() << std::endl;
return summary.termination_type == ceres::CONVERGENCE;
}
int main(int argc, char** argv) {
google::InitGoogleLogging(argv[0]);
// Problem configuration.
const int num_segments = 151;
const double regularization_weight = 1e-2;
// Eigen::MatrixXd is column major so we define our own MatrixXd which is
// row major. Eigen::VectorXd can be used directly.
typedef Eigen::Matrix<double,
Eigen::Dynamic, Eigen::Dynamic,
Eigen::RowMajor> MatrixXd;
using Eigen::VectorXd;
// `X` is the matrix of control points which make up the contour of line
// segments. The number of control points is equal to the number of line
// segments because the contour is closed.
//
// Initialize `X` to points on the unit circle.
VectorXd w(num_segments + 1);
w.setLinSpaced(num_segments + 1, 0.0, 2.0 * M_PI);
w.conservativeResize(num_segments);
MatrixXd X(num_segments, 2);
X.col(0) = w.array().cos();
X.col(1) = w.array().sin();
// Each data point has an associated preimage position on the line segment
// contour. For each data point we initialize the preimage positions to
// the index of the closest control point.
const int num_observations = kY.rows();
VectorXd t(num_observations);
for (int i = 0; i < num_observations; ++i) {
(X.rowwise() - kY.row(i)).rowwise().squaredNorm().minCoeff(&t[i]);
}
ceres::Problem problem;
// For each data point add a residual which measures its distance to its
// corresponding position on the line segment contour.
std::vector<double*> parameter_blocks(1 + num_segments);
parameter_blocks[0] = NULL;
for (int i = 0; i < num_segments; ++i) {
parameter_blocks[i + 1] = X.data() + 2 * i;
}
for (int i = 0; i < num_observations; ++i) {
parameter_blocks[0] = &t[i];
problem.AddResidualBlock(
PointToLineSegmentContourCostFunction::Create(num_segments, kY.row(i)),
NULL,
parameter_blocks);
}
// Add regularization to minimize the length of the line segment contour.
for (int i = 0; i < num_segments; ++i) {
problem.AddResidualBlock(
EuclideanDistanceFunctor::Create(sqrt(regularization_weight)),
NULL,
X.data() + 2 * i,
X.data() + 2 * ((i + 1) % num_segments));
}
ceres::Solver::Options options;
options.max_num_iterations = 100;
options.linear_solver_type = ceres::SPARSE_NORMAL_CHOLESKY;
// First, solve `X` and `t` jointly with dynamic_sparsity = true.
MatrixXd X0 = X;
VectorXd t0 = t;
CHECK(SolveWithFullReport(options, &problem, true));
// Second, solve with dynamic_sparsity = false.
X = X0;
t = t0;
CHECK(SolveWithFullReport(options, &problem, false));
return 0;
}