// Ceres Solver - A fast non-linear least squares minimizer
// Copyright 2010, 2011, 2012 Google Inc. All rights reserved.
// http://code.google.com/p/ceres-solver/
//
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//
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// Author: sameeragarwal@google.com (Sameer Agarwal)
#include "ceres/corrector.h"
#include <cstddef>
#include <cmath>
#include "ceres/internal/eigen.h"
#include "glog/logging.h"
namespace ceres {
namespace internal {
Corrector::Corrector(double sq_norm, const double rho[3]) {
CHECK_GE(sq_norm, 0.0);
CHECK_GT(rho[1], 0.0);
sqrt_rho1_ = sqrt(rho[1]);
// If sq_norm = 0.0, the correction becomes trivial, the residual
// and the jacobian are scaled by the squareroot of the derivative
// of rho. Handling this case explicitly avoids the divide by zero
// error that would occur below.
//
// The case where rho'' < 0 also gets special handling. Technically
// it shouldn't, and the computation of the scaling should proceed
// as below, however we found in experiments that applying the
// curvature correction when rho'' < 0, which is the case when we
// are in the outlier region slows down the convergence of the
// algorithm significantly.
//
// Thus, we have divided the action of the robustifier into two
// parts. In the inliner region, we do the full second order
// correction which re-wights the gradient of the function by the
// square root of the derivative of rho, and the Gauss-Newton
// Hessian gets both the scaling and the rank-1 curvature
// correction. Normaly, alpha is upper bounded by one, but with this
// change, alpha is bounded above by zero.
//
// Empirically we have observed that the full Triggs correction and
// the clamped correction both start out as very good approximations
// to the loss function when we are in the convex part of the
// function, but as the function starts transitioning from convex to
// concave, the Triggs approximation diverges more and more and
// ultimately becomes linear. The clamped Triggs model however
// remains quadratic.
//
// The reason why the Triggs approximation becomes so poor is
// because the curvature correction that it applies to the gauss
// newton hessian goes from being a full rank correction to a rank
// deficient correction making the inversion of the Hessian fraught
// with all sorts of misery and suffering.
//
// The clamped correction retains its quadratic nature and inverting it
// is always well formed.
if ((sq_norm == 0.0) || (rho[2] <= 0.0)) {
residual_scaling_ = sqrt_rho1_;
alpha_sq_norm_ = 0.0;
return;
}
// Calculate the smaller of the two solutions to the equation
//
// 0.5 * alpha^2 - alpha - rho'' / rho' * z'z = 0.
//
// Start by calculating the discriminant D.
const double D = 1.0 + 2.0 * sq_norm*rho[2] / rho[1];
// Since both rho[1] and rho[2] are guaranteed to be positive at
// this point, we know that D > 1.0.
const double alpha = 1.0 - sqrt(D);
// Calculate the constants needed by the correction routines.
residual_scaling_ = sqrt_rho1_ / (1 - alpha);
alpha_sq_norm_ = alpha / sq_norm;
}
void Corrector::CorrectResiduals(int nrow, double* residuals) {
DCHECK(residuals != NULL);
VectorRef r_ref(residuals, nrow);
// Equation 11 in BANS.
r_ref *= residual_scaling_;
}
void Corrector::CorrectJacobian(int nrow, int ncol,
double* residuals, double* jacobian) {
DCHECK(residuals != NULL);
DCHECK(jacobian != NULL);
ConstVectorRef r_ref(residuals, nrow);
MatrixRef j_ref(jacobian, nrow, ncol);
// Equation 11 in BANS.
j_ref = sqrt_rho1_ * (j_ref - alpha_sq_norm_ *
r_ref * (r_ref.transpose() * j_ref));
}
} // namespace internal
} // namespace ceres