annotate scripts/polynomial/mpoles.m @ 27985:9f9ac219896d

maint: Remove remaining "Author:" instances from code base. * __ftp__.cc, load-save.cc, urlwrite.cc, xnorm.cc, xnorm.h, cconv2.f, cdotc3.f, cmatm3.f, csconv2.f, dconv2.f, ddot3.f, dmatm3.f, sconv2.f, sdot3.f, smatm3.f, zconv2.f, zdconv2.f, zdotc3.f, zmatm3.f, crsf2csf.f, zrsf2csf.f, oct-norm.cc, oct-norm.h, lin2mu.m, mu2lin.m, bincoeff.m, blkdiag.m, deal.m, gradient.m, interpft.m, nextpow2.m, postpad.m, prepad.m, repmat.m, shift.m, xor.m, griddata.m, rotx.m, roty.m, rotz.m, voronoin.m, getappdata.m, isappdata.m, rmappdata.m, setappdata.m, colormap.m, gray.m, gray2ind.m, im2double.m, image.m, imagesc.m, imread.m, imshow.m, ind2gray.m, ind2rgb.m, ocean.m, __imread__.m, rgb2ind.m, javachk.m, ClassHelper.java, usejava.m, findstr.m, commutation_matrix.m, cross.m, gls.m, housh.m, isdefinite.m, ishermitian.m, issymmetric.m, logm.m, null.m, ols.m, orth.m, qzhess.m, rref.m, dos.m, nargoutchk.m, orderfields.m, parseparams.m, __w2mpth__.m, unix.m, untar.m, unzip.m, expand_rel_paths.m, make_rel_paths.m, daspect.m, orient.m, pbaspect.m, rticks.m, thetaticks.m, xticklabels.m, xticks.m, yticklabels.m, yticks.m, zticklabels.m, zticks.m, comet.m, contourf.m, plot3.m, cla.m, copyobj.m, findfigs.m, hdl2struct.m, linkaxes.m, __ghostscript__.m, __gnuplot_get_var__.m, __gnuplot_has_feature__.m, __gnuplot_has_terminal__.m, __gnuplot_open_stream__.m, __gnuplot_print__.m, struct2hdl.m, subplot.m, compan.m, conv.m, deconv.m, mpoles.m, poly.m, polyder.m, polyfit.m, polyint.m, polyout.m, polyreduce.m, polyval.m, polyvalm.m, residue.m, roots.m, ismember.m, __parse_movargs__.m, detrend.m, fftconv.m, fftfilt.m, fftshift.m, filter2.m, movfun.m, movslice.m, ichol.m, pcg.m, beta.m, ellipke.m, lcm.m, nchoosek.m, pow2.m, primes.m, pascal.m, rosser.m, wilkinson.m, corr.m, kurtosis.m, skewness.m, base2dec.m, bin2dec.m, blanks.m, deblank.m, dec2base.m, dec2bin.m, dec2hex.m, hex2dec.m, index.m, rindex.m, strjoin.m, substr.m, untabify.m, calendar.m, datestr.m, eomday.m, now.m, weekday.m: Remove remaining "Author:" instances from code base.
author Rik <rik@octave.org>
date Tue, 21 Jan 2020 14:35:03 -0800
parents bdad8ca48700
children 28de41192f3c 0a5b15007766
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rev   line source
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1 ########################################################################
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2 ##
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3 ## Copyright (C) 2007-2020 The Octave Project Developers
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4 ##
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5 ## See the file COPYRIGHT.md in the top-level directory of this
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6 ## distribution or <https://octave.org/copyright/>.
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7 ##
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8 ## This file is part of Octave.
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9 ##
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10 ## Octave is free software: you can redistribute it and/or modify it
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11 ## under the terms of the GNU General Public License as published by
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12 ## the Free Software Foundation, either version 3 of the License, or
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13 ## (at your option) any later version.
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14 ##
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15 ## Octave is distributed in the hope that it will be useful, but
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16 ## WITHOUT ANY WARRANTY; without even the implied warranty of
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17 ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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18 ## GNU General Public License for more details.
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19 ##
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20 ## You should have received a copy of the GNU General Public License
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21 ## along with Octave; see the file COPYING. If not, see
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22 ## <https://www.gnu.org/licenses/>.
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23 ##
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24 ########################################################################
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25
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26 ## -*- texinfo -*-
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27 ## @deftypefn {} {[@var{multp}, @var{idxp}] =} mpoles (@var{p})
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28 ## @deftypefnx {} {[@var{multp}, @var{idxp}] =} mpoles (@var{p}, @var{tol})
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29 ## @deftypefnx {} {[@var{multp}, @var{idxp}] =} mpoles (@var{p}, @var{tol}, @var{reorder})
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30 ## Identify unique poles in @var{p} and their associated multiplicity.
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31 ##
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32 ## The output is ordered from largest pole to smallest pole.
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33 ##
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34 ## If the relative difference of two poles is less than @var{tol} then they are
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35 ## considered to be multiples. The default value for @var{tol} is 0.001.
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36 ##
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37 ## If the optional parameter @var{reorder} is zero, poles are not sorted.
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38 ##
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39 ## The output @var{multp} is a vector specifying the multiplicity of the poles.
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40 ## @code{@var{multp}(n)} refers to the multiplicity of the Nth pole
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41 ## @code{@var{p}(@var{idxp}(n))}.
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42 ##
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43 ## For example:
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44 ##
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45 ## @example
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46 ## @group
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47 ## p = [2 3 1 1 2];
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48 ## [m, n] = mpoles (p)
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49 ## @result{} m = [1; 1; 2; 1; 2]
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50 ## @result{} n = [2; 5; 1; 4; 3]
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51 ## @result{} p(n) = [3, 2, 2, 1, 1]
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52 ## @end group
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53 ## @end example
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54 ##
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55 ## @seealso{residue, poly, roots, conv, deconv}
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56 ## @end deftypefn
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57
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58 function [multp, indx] = mpoles (p, tol, reorder)
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59
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60 if (nargin < 1 || nargin > 3)
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61 print_usage ();
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62 endif
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63
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64 if (nargin < 2 || isempty (tol))
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65 tol = 0.001;
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66 endif
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67
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68 if (nargin < 3 || isempty (reorder))
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69 reorder = true;
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70 endif
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71
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72 Np = numel (p);
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73
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74 ## Force the poles to be a column vector.
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75
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76 p = p(:);
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77
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78 ## Sort the poles according to their magnitidues, largest first.
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79
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80 if (reorder)
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81 ## Sort with smallest magnitude first.
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82 [p, ordr] = sort (p);
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83 ## Reverse order, largest maginitude first.
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84 n = Np:-1:1;
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85 p = p(n);
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86 ordr = ordr(n);
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87 else
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88 ordr = 1:Np;
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89 endif
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90
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91 ## Find pole multiplicity by comparing the relative difference in the
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92 ## poles.
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93
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94 multp = zeros (Np, 1);
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95 indx = [];
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96 n = find (multp == 0, 1);
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97 while (n)
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98 dp = abs (p-p(n));
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99 if (p(n) == 0.0)
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100 if (any (abs (p) > 0 & isfinite (p)))
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101 p0 = mean (abs (p(abs (p) > 0 & isfinite (p))));
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102 else
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103 p0 = 1;
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104 endif
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105 else
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106 p0 = abs (p(n));
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107 endif
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108 k = find (dp < tol * p0);
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109 ## Poles can only be members of one multiplicity group.
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110 if (numel (indx))
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111 k = k(! ismember (k, indx));
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112 endif
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113 m = 1:numel (k);
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114 multp(k) = m;
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115 indx = [indx; k];
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116 n = find (multp == 0, 1);
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117 endwhile
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118 multp = multp(indx);
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119 indx = ordr(indx);
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120
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121 endfunction
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122
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123
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124 %!test
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125 %! [mp, n] = mpoles ([0 0], 0.01);
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126 %! assert (mp, [1; 2]);