/usr/include/ratint.h is in libalglib-dev 2.6.0-3.
This file is owned by root:root, with mode 0o644.
The actual contents of the file can be viewed below.
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Copyright (c) 2007-2009, Sergey Bochkanov (ALGLIB project).
>>> SOURCE LICENSE >>>
This program is free software; you can redistribute it and/or modify
it under the terms of the GNU General Public License as published by
the Free Software Foundation (www.fsf.org); either version 2 of the
License, or (at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
A copy of the GNU General Public License is available at
http://www.fsf.org/licensing/licenses
>>> END OF LICENSE >>>
*************************************************************************/
#ifndef _ratint_h
#define _ratint_h
#include "ap.h"
#include "ialglib.h"
#include "tsort.h"
#include "ratinterpolation.h"
#include "blas.h"
#include "reflections.h"
#include "creflections.h"
#include "hqrnd.h"
#include "matgen.h"
#include "ablasf.h"
#include "ablas.h"
#include "trfac.h"
#include "trlinsolve.h"
#include "safesolve.h"
#include "rcond.h"
#include "matinv.h"
#include "hblas.h"
#include "sblas.h"
#include "ortfac.h"
#include "rotations.h"
#include "bdsvd.h"
#include "svd.h"
#include "xblas.h"
#include "densesolver.h"
#include "linmin.h"
#include "minlbfgs.h"
#include "minlm.h"
#include "lsfit.h"
/*************************************************************************
Barycentric interpolant.
*************************************************************************/
struct barycentricinterpolant
{
int n;
double sy;
ap::real_1d_array x;
ap::real_1d_array y;
ap::real_1d_array w;
};
/*************************************************************************
Barycentric fitting report:
TaskRCond reciprocal of task's condition number
RMSError RMS error
AvgError average error
AvgRelError average relative error (for non-zero Y[I])
MaxError maximum error
*************************************************************************/
struct barycentricfitreport
{
double taskrcond;
int dbest;
double rmserror;
double avgerror;
double avgrelerror;
double maxerror;
};
/*************************************************************************
Rational interpolation using barycentric formula
F(t) = SUM(i=0,n-1,w[i]*f[i]/(t-x[i])) / SUM(i=0,n-1,w[i]/(t-x[i]))
Input parameters:
B - barycentric interpolant built with one of model building
subroutines.
T - interpolation point
Result:
barycentric interpolant F(t)
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
double barycentriccalc(const barycentricinterpolant& b, double t);
/*************************************************************************
Differentiation of barycentric interpolant: first derivative.
Algorithm used in this subroutine is very robust and should not fail until
provided with values too close to MaxRealNumber (usually MaxRealNumber/N
or greater will overflow).
INPUT PARAMETERS:
B - barycentric interpolant built with one of model building
subroutines.
T - interpolation point
OUTPUT PARAMETERS:
F - barycentric interpolant at T
DF - first derivative
NOTE
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricdiff1(const barycentricinterpolant& b,
double t,
double& f,
double& df);
/*************************************************************************
Differentiation of barycentric interpolant: first/second derivatives.
INPUT PARAMETERS:
B - barycentric interpolant built with one of model building
subroutines.
T - interpolation point
OUTPUT PARAMETERS:
F - barycentric interpolant at T
DF - first derivative
D2F - second derivative
NOTE: this algorithm may fail due to overflow/underflor if used on data
whose values are close to MaxRealNumber or MinRealNumber. Use more robust
BarycentricDiff1() subroutine in such cases.
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricdiff2(const barycentricinterpolant& b,
double t,
double& f,
double& df,
double& d2f);
/*************************************************************************
This subroutine performs linear transformation of the argument.
INPUT PARAMETERS:
B - rational interpolant in barycentric form
CA, CB - transformation coefficients: x = CA*t + CB
OUTPUT PARAMETERS:
B - transformed interpolant with X replaced by T
-- ALGLIB PROJECT --
Copyright 19.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentriclintransx(barycentricinterpolant& b, double ca, double cb);
/*************************************************************************
This subroutine performs linear transformation of the barycentric
interpolant.
INPUT PARAMETERS:
B - rational interpolant in barycentric form
CA, CB - transformation coefficients: B2(x) = CA*B(x) + CB
OUTPUT PARAMETERS:
B - transformed interpolant
-- ALGLIB PROJECT --
Copyright 19.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentriclintransy(barycentricinterpolant& b, double ca, double cb);
/*************************************************************************
Extracts X/Y/W arrays from rational interpolant
INPUT PARAMETERS:
B - barycentric interpolant
OUTPUT PARAMETERS:
N - nodes count, N>0
X - interpolation nodes, array[0..N-1]
F - function values, array[0..N-1]
W - barycentric weights, array[0..N-1]
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricunpack(const barycentricinterpolant& b,
int& n,
ap::real_1d_array& x,
ap::real_1d_array& y,
ap::real_1d_array& w);
/*************************************************************************
Serialization of the barycentric interpolant
INPUT PARAMETERS:
B - barycentric interpolant
OUTPUT PARAMETERS:
RA - array of real numbers which contains interpolant,
array[0..RLen-1]
RLen - RA lenght
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricserialize(const barycentricinterpolant& b,
ap::real_1d_array& ra,
int& ralen);
/*************************************************************************
Unserialization of the barycentric interpolant
INPUT PARAMETERS:
RA - array of real numbers which contains interpolant,
OUTPUT PARAMETERS:
B - barycentric interpolant
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricunserialize(const ap::real_1d_array& ra,
barycentricinterpolant& b);
/*************************************************************************
Copying of the barycentric interpolant
INPUT PARAMETERS:
B - barycentric interpolant
OUTPUT PARAMETERS:
B2 - copy(B1)
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentriccopy(const barycentricinterpolant& b,
barycentricinterpolant& b2);
/*************************************************************************
Rational interpolant from X/Y/W arrays
F(t) = SUM(i=0,n-1,w[i]*f[i]/(t-x[i])) / SUM(i=0,n-1,w[i]/(t-x[i]))
INPUT PARAMETERS:
X - interpolation nodes, array[0..N-1]
F - function values, array[0..N-1]
W - barycentric weights, array[0..N-1]
N - nodes count, N>0
OUTPUT PARAMETERS:
B - barycentric interpolant built from (X, Y, W)
-- ALGLIB --
Copyright 17.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricbuildxyw(const ap::real_1d_array& x,
const ap::real_1d_array& y,
const ap::real_1d_array& w,
int n,
barycentricinterpolant& b);
/*************************************************************************
Rational interpolant without poles
The subroutine constructs the rational interpolating function without real
poles (see 'Barycentric rational interpolation with no poles and high
rates of approximation', Michael S. Floater. and Kai Hormann, for more
information on this subject).
Input parameters:
X - interpolation nodes, array[0..N-1].
Y - function values, array[0..N-1].
N - number of nodes, N>0.
D - order of the interpolation scheme, 0 <= D <= N-1.
D<0 will cause an error.
D>=N it will be replaced with D=N-1.
if you don't know what D to choose, use small value about 3-5.
Output parameters:
B - barycentric interpolant.
Note:
this algorithm always succeeds and calculates the weights with close
to machine precision.
-- ALGLIB PROJECT --
Copyright 17.06.2007 by Bochkanov Sergey
*************************************************************************/
void barycentricbuildfloaterhormann(const ap::real_1d_array& x,
const ap::real_1d_array& y,
int n,
int d,
barycentricinterpolant& b);
/*************************************************************************
Weghted rational least squares fitting using Floater-Hormann rational
functions with optimal D chosen from [0,9], with constraints and
individual weights.
Equidistant grid with M node on [min(x),max(x)] is used to build basis
functions. Different values of D are tried, optimal D (least WEIGHTED root
mean square error) is chosen. Task is linear, so linear least squares
solver is used. Complexity of this computational scheme is O(N*M^2)
(mostly dominated by the least squares solver).
SEE ALSO
* BarycentricFitFloaterHormann(), "lightweight" fitting without invididual
weights and constraints.
INPUT PARAMETERS:
X - points, array[0..N-1].
Y - function values, array[0..N-1].
W - weights, array[0..N-1]
Each summand in square sum of approximation deviations from
given values is multiplied by the square of corresponding
weight. Fill it by 1's if you don't want to solve weighted
task.
N - number of points, N>0.
XC - points where function values/derivatives are constrained,
array[0..K-1].
YC - values of constraints, array[0..K-1]
DC - array[0..K-1], types of constraints:
* DC[i]=0 means that S(XC[i])=YC[i]
* DC[i]=1 means that S'(XC[i])=YC[i]
SEE BELOW FOR IMPORTANT INFORMATION ON CONSTRAINTS
K - number of constraints, 0<=K<M.
K=0 means no constraints (XC/YC/DC are not used in such cases)
M - number of basis functions ( = number_of_nodes), M>=2.
OUTPUT PARAMETERS:
Info- same format as in LSFitLinearWC() subroutine.
* Info>0 task is solved
* Info<=0 an error occured:
-4 means inconvergence of internal SVD
-3 means inconsistent constraints
-1 means another errors in parameters passed
(N<=0, for example)
B - barycentric interpolant.
Rep - report, same format as in LSFitLinearWC() subroutine.
Following fields are set:
* DBest best value of the D parameter
* RMSError rms error on the (X,Y).
* AvgError average error on the (X,Y).
* AvgRelError average relative error on the non-zero Y
* MaxError maximum error
NON-WEIGHTED ERRORS ARE CALCULATED
IMPORTANT:
this subroitine doesn't calculate task's condition number for K<>0.
SETTING CONSTRAINTS - DANGERS AND OPPORTUNITIES:
Setting constraints can lead to undesired results, like ill-conditioned
behavior, or inconsistency being detected. From the other side, it allows
us to improve quality of the fit. Here we summarize our experience with
constrained barycentric interpolants:
* excessive constraints can be inconsistent. Floater-Hormann basis
functions aren't as flexible as splines (although they are very smooth).
* the more evenly constraints are spread across [min(x),max(x)], the more
chances that they will be consistent
* the greater is M (given fixed constraints), the more chances that
constraints will be consistent
* in the general case, consistency of constraints IS NOT GUARANTEED.
* in the several special cases, however, we CAN guarantee consistency.
* one of this cases is constraints on the function VALUES at the interval
boundaries. Note that consustency of the constraints on the function
DERIVATIVES is NOT guaranteed (you can use in such cases cubic splines
which are more flexible).
* another special case is ONE constraint on the function value (OR, but
not AND, derivative) anywhere in the interval
Our final recommendation is to use constraints WHEN AND ONLY WHEN you
can't solve your task without them. Anything beyond special cases given
above is not guaranteed and may result in inconsistency.
-- ALGLIB PROJECT --
Copyright 18.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricfitfloaterhormannwc(const ap::real_1d_array& x,
const ap::real_1d_array& y,
const ap::real_1d_array& w,
int n,
const ap::real_1d_array& xc,
const ap::real_1d_array& yc,
const ap::integer_1d_array& dc,
int k,
int m,
int& info,
barycentricinterpolant& b,
barycentricfitreport& rep);
/*************************************************************************
Rational least squares fitting, without weights and constraints.
See BarycentricFitFloaterHormannWC() for more information.
-- ALGLIB PROJECT --
Copyright 18.08.2009 by Bochkanov Sergey
*************************************************************************/
void barycentricfitfloaterhormann(const ap::real_1d_array& x,
const ap::real_1d_array& y,
int n,
int m,
int& info,
barycentricinterpolant& b,
barycentricfitreport& rep);
#endif
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