Mercurial > hg > octave-lyh
view scripts/general/interpft.m @ 14812:9d9eb9bac65e gui
Improved menu structure of file, edit and window menu. Removed ambiguous shortcuts, improved focus handling for operating the GUI with the keyboard. Added new shortcuts to focus subwindows directly.
* files-dockwidget: Set focus proxy to the current directory line edit.
* history-dockwidget: Set focus proxy to the inline search bar.
* file-editor: Removed and improved shortcuts.
* main-window: Added new slots for not only showing/hiding subwindows, but also for focussing them directly with Ctrl+0,1..4. Improved menu structure.
author | Jacob Dawid <jacob.dawid@googlemail.com> |
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date | Thu, 28 Jun 2012 11:04:37 +0200 |
parents | f3d52523cde1 |
children | bb3a1ec7cc4b |
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## Copyright (C) 2001-2012 Paul Kienzle ## ## This file is part of Octave. ## ## Octave 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; either version 3 of the License, or (at ## your option) any later version. ## ## Octave 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. ## ## You should have received a copy of the GNU General Public License ## along with Octave; see the file COPYING. If not, see ## <http://www.gnu.org/licenses/>. ## -*- texinfo -*- ## @deftypefn {Function File} {} interpft (@var{x}, @var{n}) ## @deftypefnx {Function File} {} interpft (@var{x}, @var{n}, @var{dim}) ## ## Fourier interpolation. If @var{x} is a vector, then @var{x} is ## resampled with @var{n} points. The data in @var{x} is assumed to be ## equispaced. If @var{x} is an array, then operate along each column of ## the array separately. If @var{dim} is specified, then interpolate ## along the dimension @var{dim}. ## ## @code{interpft} assumes that the interpolated function is periodic, ## and so assumptions are made about the endpoints of the interpolation. ## ## @seealso{interp1} ## @end deftypefn ## Author: Paul Kienzle ## 2001-02-11 ## * initial version ## 2002-03-17 aadler ## * added code to work on matrices as well ## 2006-05-25 dbateman ## * Make it matlab compatiable, cutting out the 2-D interpolation function z = interpft (x, n, dim) if (nargin < 2 || nargin > 3) print_usage (); endif if (! (isscalar (n) && n == fix (n))) error ("interpft: N must be a scalar integer"); endif if (nargin == 2) if (isrow (x)) dim = 2; else dim = 1; endif endif nd = ndims (x); if (dim < 1 || dim > nd) error ("interpft: invalid dimension DIM"); endif perm = [dim:nd, 1:(dim-1)]; x = permute (x, perm); m = rows (x); inc = max (1, fix (m/n)); y = fft (x) / m; k = floor (m / 2); sz = size (x); sz(1) = n * inc - m; idx = repmat ({':'}, nd, 1); idx{1} = 1:k; z = cat (1, y(idx{:}), zeros (sz)); idx{1} = k+1:m; z = cat (1, z, y(idx{:})); z = n * ifft (z); if (inc != 1) sz(1) = n; z = inc * reshape (z(1:inc:end), sz); endif z = ipermute (z, perm); endfunction %!demo %! clf; %! t = 0 : 0.3 : pi; dt = t(2)-t(1); %! n = length (t); k = 100; %! ti = t(1) + [0 : k-1]*dt*n/k; %! y = sin (4*t + 0.3) .* cos (3*t - 0.1); %! yp = sin (4*ti + 0.3) .* cos (3*ti - 0.1); %! plot (ti, yp, 'g', ti, interp1(t, y, ti, "spline"), 'b', ... %! ti, interpft (y, k), 'c', t, y, "r+"); %! legend ("sin(4t+0.3)cos(3t-0.1)", "spline", "interpft", "data"); %!shared n,y %! x = [0:10]'; y = sin(x); n = length (x); %!assert (interpft (y, n), y, 20*eps); %!assert (interpft (y', n), y', 20*eps); %!assert (interpft ([y,y],n), [y,y], 20*eps); %% Test input validation %!error interpft () %!error interpft (1) %!error interpft (1,2,3) %!error <N must be a scalar integer> interpft (1,[2,2]) %!error <N must be a scalar integer> interpft (1,2.1) %!error <invalid dimension DIM> interpft (1,2,0) %!error <invalid dimension DIM> interpft (1,2,3)