Scilab Website | Contribute with GitLab | Mailing list archives | ATOMS toolboxes
Scilab Online Help
2024.1.0 - Русский


datafit

Non linear (constrained) parametric fit of measured (weighted) data

Syntax

[p, dmin, status] = datafit(G, Data, p0)
[p, dmin, status] = datafit(G, Data, Wd, p0)
[p, dmin, status] = datafit(G, Data, Wd, 'b', p_inf, p_sup, p0)
[p, dmin, status] = datafit(G, Data, 'b', p_inf, p_sup, p0)
[p, dmin, status] = datafit(G, Data [,Wd] [,Wg][,'b',p_inf,p_sup], p0 [,algo][,stop])
[p, dmin, status] = datafit(G, DG, Data, ..)
[p, dmin, status] = datafit(iprint, ..)

Arguments

The following definitions are used:

  • ng = size(g,1): number of fitting criteria (= of gap definitions).
  • np = size(p,"*"): total number of fitting parameters.
  • nd = size(Data,2): number of data points.
  • ndc = size(Data,1): number of coordinates of each data point.

p0
Matrix of initial guess of the model parameters (np elements).

"b"
keyword heading the p_inf, p_sup sequence, where p_inf and p_sup are real matrices with the p0 shape and sizes. p_inf is the vector of lower bounds of respective p components. p_sup are upper bounds.

p
Matrix of the best fitting model parameters, with the p0 sizes.

Data
(ndc × nd) matrix of experimental data points, where Data(:,i) are the ndc coordinates of the ith measurement.

Wd
Data weights (optional). Row vector with nd elements.

G

Gap function: handle of a function in Scilab language or of a compiled external function. Computed gap(s) between the fitting model and data may be of the first order, not quadratic.

If G() does not need any own input parameters (like constants), only arguments, its syntax must be g = G(p, Data).

If G() needs some own input parameters in addition to input arguments, its syntax must be g = G(p, Data, param1, param2, .., paramN). Then, list(G, param1, param2, .., paramN) must be provided to datafit(), instead of only G.

The sizes of G arguments are the following ones:

p : fitting parameters to be optimized.
Data : (ndc × nd) matrix, as described above. If G is defined to compute gaps only for a single data point (so is not "vectorized"), datafit() automatically performs an explicit loop over the set of Data columns. This makes datafit() slower.
g : result: (ng × nd) matrix; or (ng × 1) column if G accepts only one data point per call (much slower).
  • Each column is related to a given data point and retuns its gaps to the fitting model.
  • Each row is about a gap definition. G may compute several types of gaps. For instance, the vertical gaps may be returned in g(1,:) ; the horizontal gaps in g(2,:) ; the nearest distances in g(3,:) ; etc.

DG
(optional) Handle of a function in Scilab language or of a compiled external function, computing the partial of G wrt p. Its syntax must be like S = DG(p, Data). The expected sizes of the result are (ng × np × 1) (Data-unvectorized) or (ng × np × nd) (Data-vectorized).

Wg
Optional (ng × ng) matrix of weights of gaps definitions. Default = eye(). G() defines as many types of gaps as required. Most often, a unique gap will be computed -- most often the vertical one --, but other ones can be computed (horizontal, nearest distance, etc). This matrix allows to weight the different types.

algo
Word 'qn' (quasi-Newton, default), or 'gc' (conjugate gradient), or 'nd' (non-differentiable. Then p_inf and p_sup parameters bounds are not accepted). Selects the algorithm used to perform the fitting. See optim() for more details.

stop

sequence of optional arguments controlling the convergence of the fitting algorithm:

'ar',nap, [iter [,epsg [,epsf [,epsx]]]], with

"ar" reserved keyword heading the list of stopping criteria as defined below.
nap maximum number of calls to the cost f function allowed (default: 100).
iter maximum number of iterations allowed (default: 100).
epsg threshold on gradient norm (default: %eps).
epsf threshold controlling the decreasing of f (defined in the description section). Default: 0.
epsx threshold controlling the variation of p. This vector (possibly matrix) of same size as p0 can be used to scale p. Default: 0.
dmin
Average Model-to-data residual distance. It is equal to sqrt(fmin/ng/nd) or sqrt(fmin/ng/sum(Wd)), where fmin is the quadratic residue of the cost function f (see the description).

iprint

scalar used to set the trace mode:

ValueAction
0nothing (except errors) is reported
1initial and final reports
2adds a report per iteration
>2adds reports on linear search
Most of the reports are displayed in the Scilab console.

status
return flag = termination status (only for the 'qn' default algorithm. Set to %nan otherwise): 9 is successful. Possible values are:
1: Norm of projected gradient lower than... .... 6: Optim stops: too small variations in gradient direction.
2: At last iteration, f decreases by less than... 7: Stop during calculation of descent direction.
3: Optim stops: Too small variations for p. 8: Stop during calculation of estimated hessian.
4: Optim stops: maximum number of calls to f is reached. 9: Successful completion.
5: Optim stops: maximum number of iterations is reached. 10: Linear search fails.

Other optim() input arguments such that df0, mem, or 'in' may be used with datafit(). They will be passed as is to optim().

Description

datafit is used to fit a parametrized model to given data.

A function G(p, Data) must be defined to compute the gaps between the Data points and a model whose parameters to be tuned are provided through the matrix p. An initial guess p0 of p values must also be provided.

Starting from initial values p0 of the model parameters, datafit() varies them in order to minimize the whole Model-to-Data distance defined as

f = (G(p, Data(:,1))' * Wg * G(p, Data(:,1)))* Wd(1) + ..
    (G(p, Data(:,2))' * Wg * G(p, Data(:,2)))* Wd(2) + ..
    ...
    (G(p, Data(:,nz))' * Wg * G(p,Data(:,nz)))* Wd(nz)

When Wg = eye() (default), this definition is equivalent to

f = sum(G(p, Data(:,1)).^2) * Wd(1) + ..
    sum(G(p, Data(:,2)).^2) * Wd(2) + ..
    ...
    sum(G(p, Data(:,nz)).^2) * Wd(nz)

If in addition G returns only one gap type, this even simplifies to

f = G(p, Data(:,1))^2 * Wd(1) + ..
    G(p, Data(:,2))^2 * Wd(2) + ..
    ...
    G(p, Data(:,nz))^2 * Wd(nz)

datafit() calls optim() to minimize f.

Choosing appropriately p0 may improve and faster datafit()'s convergence to the best fit.

datafit() checks whether G() is vectorized or not over Data. If G() works only with a single data point as a single column of coordinates, then datafit() loops over data=Data(:,i) points. Otherwise, G(p, Data) is called for the whole Data array of data coordinates, which is way faster if G()'s code is truly vectorized.

Examples

Simple example: Polynomial fitting (parabola = 3 parameters) of weighted data.

Data weights prevent processing this case in a straightforward way with a Vandermonde matrix and the backslash operator. An initial guess p0 is then required.

// Model (parabola)
function y=FF(x, p)
    y = (p(1)*x + p(2)).*x + p(3)
endfunction

// Data creation
pa = [2;-4;14] // parameters of the actual law, to generate data
X = 0:0.1:3.5;
Y0 = FF(X, pa);
noise = 5*(rand(Y0)-.5);   // We add some noise
Y = Y0 + noise
Data = [X ; Y];

// Gap function definition
function e=G(p, Data)
    e = Data(2,:) - FF(Data(1,:), p);  // vertical distance
endfunction

// Performing the fitting
// ----------------------
// Without weighting data:
p0 = [1;-1;10]
[p, dmin] = datafit(G, Data, p0);
// The uncertainty is identified to the noise value.
// The weight is set inversely proportional to the uncertainty
[pw, dmin] = datafit(G, Data, 1./abs(noise), p0);

// Display
// -------
scf(0);
clf()
xsetech([0 0 1 0.83])
plot2d(X, Y0, 24)       // True underlaying law
plot2d(X, Y, -1)        // Noisy data
plot2d(X, FF(X, p), 15)  // best unweighted fit
plot2d(X, FF(X, pw), 18) // best weighted fit
legend(["True law" "Noisy data" "Unweighted fit" "Weighted fit"],2)

xsetech([0 .75 1 0.25])
plot2d(X, FF(X,p)-Y0, 15)  // remaining gap <= best unweighted fit
plot2d(X, FF(X,pw)-Y0, 18) // remaining gap <= best weighted fit
ylabel("Data fit - True law")
ax = gca(); ax.x_location = "top";
tmp = ax.x_ticks.labels;
gca().x_ticks.labels = emptystr(size(tmp,"*"),1);
xgrid(color("grey70"))

Fitting a gaussian curve + sloping base (5 parameters):

function Y=model(P, X)
    Y = P(3) * exp(-(X-P(1)).^2 / (2*P(2)*P(2))) + P(4)*X + P(5);
endfunction
// -------------------------------
// Gap function
function r=gap(P, XY)
    r = XY(2,:) - model(P,XY(1,:))
endfunction
// -------------------------------
// True parameters
Pg = [3.5 1.5 7 0.4 -0.5]; // mean stDev ymax a(.x) b

// Generating data
// ---------------
X = 0:0.2:10;
Np = length(X);
Y0 = model(Pg, X);              // True law
noise = (rand(Y0)-.5)*Pg(3)/4;
Y = Y0 + noise                  // Noised data
Data = [X ; Y];

// Trying to recover original parameters from the (noisy) data:
// -----------------------------------------------------------
// Performing the fitting = parameters optimization
[v, k] = max(Y0);
P0 = [X(k) 1 v 1 1];
[P, dmin, s]  = datafit(gap, Data, P0);
Wd =  1./abs(noise);
[Pw, dminw, s] = datafit(gap, Data, Wd, P0);

// Computing fitting curves from found parameters
fY = model(P, X);
fYw = model(Pw, X);

// Display
// -------
scf(0);
clf()
xsetech([0 0 1 0.8])
plot2d(X, Y0, 24)  // True underlaying law
plot2d(X, Y,  -1)  // Noisy data
plot2d(X, fY, 15)  // best unweighted fit
plot2d(X, fYw,18)  // best weighted fit

// Legends: Average vertical Model-Data distance:
// True one v/s according to the residual cost
L_1 = "Unweighted fit (%5.2f /%5.2f)";
L_1 = msprintf(L_1, mean(abs(fY-Y0)), sqrt(dmin/Np));
L_2 = "Weighted fit (%5.2f /%5.2f)";
L_2 = msprintf(L_2, mean(abs(fYw-Y0)), sqrt(dminw/sum(Wd)));
legend(["True law", "Noisy Data", L_1, L_2],1)

// Params: row#1: true params row#2:
//  from unweighted fit row#3: from weighted fit
[xs, ys] = meshgrid(linspace(2,6,5), linspace(0.5,-0.5,3));
xnumb(xs, ys, [Pg ; P ; Pw]);
LawTxt = "$\Large p_3\,.\,"+..
         "exp\left({-(x-p_1)^2}\over{2\,p_2} \right)+p_4.x+p_5$";
xstring(2, 1.3, LawTxt)

// Plotting residus:
xsetech([0 .75 1 0.25])
plot2d(X, model(P ,X)-Y0, 15) // remaining gap with best unweighted fit
plot2d(X, model(Pw,X)-Y0, 18) // remaining gap best weighted fit
ylabel("Data fit - True law")
ax = gca();
ax.x_location = "top";
gca().x_ticks.labels = emptystr(size(ax.x_ticks.labels, "*"),1);
xgrid(color("grey70"))

Extraction of 3 overlapping gaussian curves (9 parameters): example with constrained bounds and a matrix of parameters.

// Basic gaussian component:
function Y=gauss(X, average, stDev, ymax)
    Y = ymax * exp(-(X-average).^2 / (2*stDev*stDev))
endfunction

// Model: cumulated gaussian laws
function r=model(P, X)
    // P(1,:): averages  P(2,:): standard deviation  P(3,:): ymax
    r = 0;
    for i = 1:size(P,2)
        r = r + gauss(X, P(1,i), P(2,i), P(3,i));
    end
endfunction

// Gap function:
function r=gap(P, XY)
    r = XY(2,:) - model(P, XY(1,:))
endfunction

// True parameters :
Pa = [ 1.1  4    7    // averages
        1  0.8  1.5   // standard deviations
        3   2   5.5   // ymax
     ];
Nc = size(Pa,2);      // Number of summed curves
Np = 200;             // Number of data points

// Data generation (without noise)
xmin = 0;
xmax = 10;
X = linspace(xmin-2, xmax+2, Np);
Y = model(Pa, X);
Data = [X ; Y];      // Curve to analyze / fit

// FITTING
// -------
// Fitting parameters: initial values and bounds (amplitudes must be > 0)
Po = [ linspace(xmin,xmax,Nc) ; ones(1,Nc)*0.5 ; ones(1,Nc)*max(Y)/2];
Pinf = [ones(1,Nc)*-2 ; ones(1,Nc)*0.1 ; ones(1,Nc)*1];
Psup = [ones(1,Nc)*12 ; ones(1,Nc)*3   ; ones(1,Nc)*max(Y)*1.2];
// Fitting
[P, dmin] = datafit(gap, Data, 'b',Pinf,Psup, Po, 'qn','ar',200,200);

// Display
// -------
clf()
xsetech([0 0 1 0.8]);
plot(X, Y, "-b", X, model(P,X), "-r");
gca().children.children(1:2).thickness = 2;
for i = 1:Nc
plot(X, gauss(X, Pa(1,i), Pa(2,i), Pa(3,i)), "-c"); // True gaussian components
plot(X, gauss(X, P(1,i), P(2,i), P(3,i)), "-g");    // Extracted gaussian components
end
legend("Data", "Parametric Model","True components", "Extracted components",  2);

xsetech([0 0.75 1 0.25])
plot(X, model(P,X)-Y);
gca().x_location = "top";
gca().x_ticks.labels = emptystr(size(gca().x_ticks.labels,"*"),1);
ylabel("Model - Data")
xgrid(color("grey70"))

With a parametric curve: Fitting a off-centered tilted 2D elliptical arc (5 parameters).

function g=Gap(p, Data)
    // p: a, b, center xc, yc, alpha tilt °
    C = cosd(p(5)); S = -sind(p(5));
    x = Data(1,:) - p(3);
    y = Data(2,:) - p(4);
    g = ((x*C - y*S )/p(1)).^2 + ((x*S + y*C)/p(2)).^2 - 1;
endfunction

// Generating the data
// -------------------
// Actual parameters :
Pa = [3, 1.3, -2, 1.5, 30];
Np = 30;            // Number of data points
Theta = grand(1,Np, "unf",-100, 170);
// untilted centered noisy arc
x = Pa(1)*(cosd(Theta) + grand(Theta, "unf", -0.07, 0.07));
y = Pa(2)*(sind(Theta) + grand(Theta, "unf", -0.07, 0.07));
// Tilting and off-centering the arc
A = Pa(5);
C = cosd(A); S = sind(A);
xe =  C*x + y*S + Pa(3);
ye = -S*x + y*C + Pa(4);
Data = [xe ; ye];

// Retrieving parameters from noisy data
// -------------------------------------
// Initial estimation
ab0 = (strange(xe)+strange(ye))/2;
xc0 = mean(xe);
yc0 = mean(ye);
A0 = -atand(reglin(xe,ye));
P0 = [ab0 ab0/2 xc0 yc0 A0];
// Parameters bounds
Pinf = [ 0     0     xc0-2*ab0, yc0-2*ab0 -90];
Psup = [3*ab0 3*ab0  xc0+2*ab0, yc0+2*ab0  90];// Fitting

// FITTING
[P, dmin] = datafit(Gap, Data, 'b',Pinf,Psup, P0);

// P(1) is the longest axis:
if P(1)<P(2) then
    P([1 2]) = P([2 1]);
    P(5) = 90 - P(5);
end

// DISPLAY
// -------
disp([Pa;P], dmin);
// A successful fit should lead to dmin ~ noise amplitude

clf
plot(xe, ye, "+")   // Data
// Model
Theta = 0:2:360;
x = P(1) * cosd(Theta);
y = P(2) * sind(Theta);
A = P(5);
[x, y] = (x*cosd(A)+y*sind(A)+P(3), -x*sind(A)+y*cosd(A)+P(4));
plot(x, y, "r")
isoview
// Parameters values:
Patxt = msprintf("%5.2f   %5.2f   %5.2f   %5.2f  %5.1f", Pa);
Ptxt  = msprintf("%5.2f   %5.2f   %5.2f   %5.2f  %5.1f", P);
xstring(-3.7, 1.2, ["" "    a           b        xc       yc     A°"
                    "Actual:" Patxt
                    "Fit:" Ptxt ])
xstring(-2.5, 0.9, "dmin = " + msprintf("%5.3f", dmin))

See also

  • backslash — (\) левое матричное деление: точное решение или решение по методу наименьших квадратов
  • lsqrsolve — minimize the sum of the squares of nonlinear functions, levenberg-marquardt algorithm
  • optim — non-linear optimization routine
  • leastsq — Solves non-linear least squares problems

History

ВерсияОписание
6.1
  • New option Wd to weight measured data Data.
  • The gap function G() may now be vectorized over Data points.
  • Initial parameters p0 and their bounds may now be provided as a matrix instead of a mandatory column.
  • The err output argument is replaced with dmin = average Model-to-data distance.
  • New output argument status added (for the "qn" algorithm).
Report an issue
<< Nonlinear Least Squares Nonlinear Least Squares leastsq >>

Copyright (c) 2022-2024 (Dassault Systèmes)
Copyright (c) 2017-2022 (ESI Group)
Copyright (c) 2011-2017 (Scilab Enterprises)
Copyright (c) 1989-2012 (INRIA)
Copyright (c) 1989-2007 (ENPC)
with contributors
Last updated:
Mon Jun 17 17:55:06 CEST 2024