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bedmachine_3d.m
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bedmachine_3d.m
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function h = bedmachine_3d(lati_or_xi,loni_or_yi,varargin)
% bedmachine_3d creates a 3D map of BedMachine data.
%
%% Requirements
% This function requires a set of Matlab tools and a Bedmachine dataset,
% and both will depend on where you're working. Get them here:
%
% * For Greenland: *
% Arctic Mapping Tools: https://www.mathworks.com/matlabcentral/fileexchange/63324
% Greenland Bedmachine Data: https://nsidc.org/data/IDBMG4
%
% * For Antarctica: *
% Antarctic Mapping Tools: https://www.mathworks.com/matlabcentral/fileexchange/47638
% Antarctic Bedmachine Data: https://nsidc.org/data/nsidc-0756
%
%% Syntax
%
% bedmachine_3d(latlim,lonlim)
% bedmachine_3d(xlim,ylim)
% bedmachine_3d(...,'buffer',extrakm)
% bedmachine_3d(...,'alpha',iceAlpha)
% bedmachine_3d(...,'velocity',res_km)
% bedmachine_3d(...,'greenland')
% h = bedmachine_3d(...)
%
%% Description
%
% bedmachine_3d(latlim,lonlim) creates a 3D map of the region specified by
% latitude and longitude limits. latlim and lonlin can be two-element arrays
% to specify just the min and max extents, or latlim,lonlim can be a range
% of values, and the resulting map will cover the entire range. Plotting might
% be slow for very large areas, so start small and see what your computer can
% handle.
%
% bedmachine_3d(xlim,ylim) as above, but map extents are specified by polar
% stereographic meters.
%
% bedmachine_3d(...,'buffer',extrakm) adds a buffer of specified width in
% kilometers around the region of interest.
%
% bedmachine_3d(...,'alpha',iceAlpha) sets the transparency of the ice. By default,
% iceAlpha=1, meaning fully opaque. Use a value between 0 and 1 for semitransparent
% ice.
%
% bedmachine_3d(...,'velocity',res_km) overlays ITS_LIVE velocity vectors at
% the specified spatial resolution res_km in kilometers. This option might be
% somewhat slow to render, especially for large regions. Requires ITS_LIVE Matlab
% toolbox (on File Exchange and GitHub).
%
% bedmachine_3d(...,'greenland') plots Greenland instead of the default Antarctica.
%
% h = bedmachine_3d(...) returns a structure of all the object graphical handles.
%
%% Examples
% For examples with real pretty pictures, type
%
% showdemo bedmachine_3d_documentation
%
%% Citations
% If you use BedMachine data, please cite the Morlighem paper listed below.
% And if this function is useful for you, please do me a kindness and cite
% my Antarctic Mapping Tools paper.
%
% Morlighem, M., E. Rignot, T. Binder, D. D. Blankenship, R. Drews, G. Eagles,
% O. Eisen, F. Ferraccioli, R. Forsberg, P. Fretwell, V. Goel, J. S. Greenbaum,
% H. Gudmundsson, J. Guo, V. Helm, C. Hofstede, I. Howat, A. Humbert, W. Jokat,
% N. B. Karlsson, W. Lee, K. Matsuoka, R. Millan, J. Mouginot, J. Paden, F. Pattyn,
% J. L. Roberts, S. Rosier, A. Ruppel, H. Seroussi, E. C. Smith, D. Steinhage,
% B. Sun, M. R. van den Broeke, T. van Ommen, M. van Wessem, and D. A. Young. 2019.
% Deep glacial troughs and stabilizing ridges unveiled beneath the margins of the
% Antarctic ice sheet, Nature Geoscience. https://doi.org/10.1038/s41561-019-0510-8
%
% Greene, C. A., Gwyther, D. E., & Blankenship, D. D. Antarctic Mapping Tools
% for Matlab. Computers & Geosciences. 104 (2017) pp.151-157.
% http://dx.doi.org/10.1016/j.cageo.2016.08.003
%
%% Author Info
% This function was written by Chad A. Greene, October 2018.
%
% See also bedmachine_profile and bedmachine_data.
%% Input checks:
assert(nargin>=2,'Plotting the entire continent might be slow, so you must define a region of interest.')
assert(isequal(size(lati_or_xi),size(loni_or_yi)),'Dimensions of input coordinates must agree.')
assert(license('test','image_toolbox')==1,'Sorry, this function requires the image processing toolbox.')
% Set defaults:
iceAlpha = 1; % transparency of ice. 0=invisible; 1=opaque.
oceanAlpha = 0.1;
make_quiver = false;
buf = 0;
IceSheet = 'antarctica';
if nargin>2
tmp = strncmpi(varargin,'alpha',3);
if any(tmp)
iceAlpha = varargin{find(tmp)+1};
assert(iceAlpha>=0 & iceAlpha<=1,'Ice alpha value must be between 0 and 1.')
end
tmp = strncmpi(varargin,'buffer',3);
if any(tmp)
buf = varargin{find(tmp)+1};
assert(isscalar(buf) & buf<5000,'The buffer value must be a scalar in units of kilometers.')
end
if any(strncmpi(varargin,'greenland',4))
IceSheet = 'greenland';
end
tmp = strncmpi(varargin,'velocity',3);
if any(tmp)
make_quiver = true;
assert(exist('itslive_interp.m','file')==2,'Cannot find itslive_interp. To plot velocity vectors, you must have itslive installed.')
try
res_km = varargin{find(tmp)+1};
catch
error('To plot velocity vectors, specify a spatial resolution in kilometers.')
end
assert(isscalar(res_km) & res_km<1000,'The spatial resolution of the velocity arrows must be a scalar value in kilometers.')
end
end
%% Load data:
[bed,x,y] = bedmachine_data('bed',lati_or_xi,loni_or_yi,'buf',buf,IceSheet);
sfz = bedmachine_data('surface',lati_or_xi,loni_or_yi,'buf',buf,IceSheet);
base = bedmachine_data('base',lati_or_xi,loni_or_yi,'buf',buf,IceSheet);
mask = bedmachine_data('mask',lati_or_xi,loni_or_yi,'buf',buf,IceSheet);
[X,Y] = meshgrid(x,y);
%% Get the geometry of this
L = bwlabel(mask~=0);
P = regionprops(mask~=0);
ind = find([P.Area]==max([P.Area]));
icesheet = L==ind;
% Boundaries of the ice sheet:
B = bwboundaries(icesheet);
ind = sub2ind(size(X),B{1}(:,1),B{1}(:,2));
xi = X(ind);
yi = Y(ind);
sfzi = sfz(ind);
basei = base(ind);
% Boundaries of the bed:
B = bwboundaries(true(size(X)));
ind = sub2ind(size(X),B{1}(:,1),B{1}(:,2));
xb = X(ind);
yb = Y(ind);
bedb = bed(ind);
% Boundaries of the ocean:
B = bwboundaries(imdilate(mask==0,strel('disk',1)));
ind = sub2ind(size(X),B{1}(:,1),B{1}(:,2));
xo = X(ind);
yo = Y(ind);
bedo = bed(ind);
base(mask~=3) = nan;
sfz(mask==0) = nan; % ocean
sfz(mask==1) = nan; % rock
%% Plot the 3D map:
hold on
view(3)
daspect([1 1 1/30])
clear h
% Plot bed:
h.bed = surface(x,y,bed);
shading interp
axis tight off
% Set the colormap for the bed:
if exist('cmocean.m','file')
cmocean topo
caxis([-1 1]*max(abs(bed(:))))
else
disp 'I cannot find the cmocean colormap function, which is part of the Climate Data Toolbox. That''s okay; we will use Matlab''s default colormap.'
end
% Plot base:
h.base = surface(x,y,base);
h.base.EdgeColor = 'none';
h.base.FaceColor = [0.8431 1.0000 0.9961];
h.base.FaceAlpha = iceAlpha;
% Plot ice surface:
h.sfz = surface(x,y,sfz);
h.sfz.EdgeColor = 'none';
h.sfz.FaceColor = [0.8431 1.0000 0.9961];
h.sfz.FaceAlpha = iceAlpha;
% Plot ice side:
h.iceside = surface([xi xi],[yi yi],[basei sfzi]);
h.iceside.EdgeColor = 'none';
h.iceside.FaceColor = [0.8431 1.0000 0.9961];
h.iceside.FaceAlpha = iceAlpha;
% Plot bed side:
h.bedside = surface([xb xb],[yb yb],[min(bed(:))*ones(size(bedb)) bedb]);
h.bedside.EdgeColor = 'none';
h.bedside.FaceColor = 'k';
% plot ocean surface:
h.oceansfz = patch(xo,yo,zeros(size(xo)),'b');
h.oceansfz.EdgeColor = [0.0118 0.4431 0.6118];
h.oceansfz.FaceColor = [0.0118 0.4431 0.6118];
h.oceansfz.FaceAlpha = oceanAlpha;
h.oceansfz.SpecularStrength = 1;
% Plot ocean side:
h.oceanside = surface([xo xo],[yo yo],[bedo zeros(size(bedo))]);
h.oceanside.EdgeColor = 'none';
h.oceanside.FaceColor = [0.0118 0.4431 0.6118];
h.oceanside.FaceAlpha = oceanAlpha;
h.oceanside.SpecularStrength = 1;
% plot ocean corners:
if bed(1,1)<0
h.corner(1) = plot3(X(1,1)*[1 1],Y(1,1)*[1 1],[0 bed(1,1)],'color',[0.0118 0.4431 0.6118]);
end
if bed(end,1)<0
h.corner(2) = plot3(X(end,1)*[1 1],Y(end,1)*[1 1],[0 bed(end,1)],'color',[0.0118 0.4431 0.6118]);
end
if bed(1,end)<0
h.corner(3) = plot3(X(1,end)*[1 1],Y(1,end)*[1 1],[0 bed(1,end)],'color',[0.0118 0.4431 0.6118]);
end
if bed(end,end)<0
h.corner(4) = plot3(X(end,end)*[1 1],Y(end,end)*[1 1],[0 bed(end,end)],'color',[0.0118 0.4431 0.6118]);
end
if make_quiver
% Make a 100 m grid that fully covers the domain, plus 20 km on all sides:
[Xv,Yv] = meshgrid((x(1)-20e3):200:(x(end)+20e3),(y(1)+20e3):-200:(y(end)-20e3));
% Get velocity and surface elevation of the dense grid:
vx = itslive_interp('vx',Xv,Yv,'region',IceSheet(1:3));
vy = itslive_interp('vy',Xv,Yv,'region',IceSheet(1:3));
Z = bedmachine_interp('surface',Xv,Yv,IceSheet);
% Lowpass filter to ~two wavelengths to anti-alias before interpolation:
vx = filt2(vx,0.2,res_km*2,'lp'); % filt2 is a subfunction below.
vy = filt2(vy,0.2,res_km*2,'lp');
Z = filt2(Z,0.2,res_km*2,'lp');
% Grid at the user-requested resolution:
[Xr,Yr] = meshgrid((x(1)-20e3):res_km*1000:(x(end)+20e3),(y(1)+20e3):-res_km*1000:(y(end)-20e3));
% Interpolate to the user-requested grid:
vxr = interp2(Xv,Yv,vx,Xr,Yr);
vyr = interp2(Xv,Yv,vy,Xr,Yr);
Zr = interp2(Xv,Yv,Z,Xr,Yr);
Z2r = interp2(Xv,Yv,Z,Xr+vxr,Yr+vyr);
% NaN the ocean:
ocean = bedmachine_interp('mask',Xr,Yr,IceSheet)==0 | Xr<x(1) | Xr>x(end) | Yr>y(1) | Yr<y(end);
Xr(ocean) = nan;
Yr(ocean) = nan;
vxr(ocean) = nan;
vyr(ocean) = nan;
Zr(ocean) = nan;
Z2r(ocean) = nan;
% Plot vectors:
h.vel = quiver3(Xr,Yr,Zr,vxr,vyr,Z2r-Zr,'r');
end
% Set lighting parameters:
material dull
camlight
% lighting phong % phong is slow but perhaps slightly prettier
%% Clean up:
if nargout==0
clear h
end
end
function Zf = filt2(Z,res,lambda,filtertype)
% filt2 performs a highpass, lowpass, bandpass, or bandstop 2D gaussian filter on gridded data such as
% topographic, atmospheric, oceanographic, or any kind of geospatial data. This function is designed to
% make it easy to remove features longer or shorter than a given characteristic wavelength. The
% input grid can contain NaNs!
%
%% Syntax
%
% Zf = filt2(Z,res,lambda,filtertype)
%
%% Description
%
% Zf = filt2(Z,res,lambda,filtertype) filters 2D dataset Z that has resolution res,
% to an approximate wavelength lambda. If the filtertype is 'lp' or 'hp' for lowpass
% or highpass, lambda must be a scalar value. If the filtertype is 'bp' or 'bs' for
% bandpass or bandstop, lambda must be a two-element array of the two cutoff wavelengths.
%
%% Explanation of this type of filter
% For examples, type
%
% cdt filt2
%
%% Author Info
% This function was written by Chad A. Greene of the University of Texas Institute for
% Geophysics in November 2016; however, all I did was repackage Carlos Adrian Vargas Aguilera's
% superb ndnanfilter function, which can be found here: http://www.mathworks.com/matlabcentral/fileexchange/20417.
% Many thanks to Carlos for his well-thought-out code and clear documentation.
%
% See also conv2, imgaussfilt, and imfilter.
%% Input checks
narginchk(4,4)
assert(license('test','image_toolbox')==1,'Error: I''m sorry, the filt2 function requires the Image Processing Toolbox.')
assert(ismatrix(Z),'Input error: Z must be a 2d matrix.')
assert(isscalar(res),'Input error: res must be a scalar value.')
assert(ismember(lower(filtertype),{'lp','hp','bp','bs'}),'Input error: filtertype must be ''hp'', ''lp'', ''bp'', or ''bs''.')
if lambda<=(2*res)
warning('Nyquist says the wavelength should exceed two times the resolution of the dataset, which is an unmet condition based on these inputs. I''ll give you some numbers, but I would''t trust ''em if I were you.')
end
if ismember(lower(filtertype),{'bp','bs'})
assert(numel(lambda)==2,'Input error: Wavelength lambda must be a two-element array for a bandpass filter.')
else
assert(isscalar(lambda),'Input error: Wavelength lambda must be a scalar for lowpass or bandpass filters.')
end
%% Design filter:
% 2*pi*sigma is the wavelength at which the amplitude is multiplied by a factor of about 0.6 (more exactly, exp(-0.5))
sigma = (lambda(1)/res) /(2*pi);
f = fspecial('gaussian',2*ceil(2.6*sigma)+1,sigma);
%% Now filter the data
switch lower(filtertype)
case 'lp'
Zf = ndnanfilter(Z,f,'replicate'); % ndnanfilter is Carlos Adrian Vargas Aguilera's excellent function, which is included as a subfunction below.
case 'hp'
Zf = Z - ndnanfilter(Z,f,'replicate');
case 'bp'
Zf = filt2(filt2(Z,res,max(lambda),'hp'),res,min(lambda),'lp');
case 'bs'
Zf = filt2(Z,res,max(lambda),'lp') - filt2(Z,res,min(lambda),'hp');
otherwise
error('No such filter type.')
end
end
function [Y,W] = ndnanfilter(X,HWIN,F,DIM,WINOPT,PADOPT,WNAN)
% NDNANFILTER N-dimensional zero-phase digital filter, ignoring NaNs.
%
% Syntax:
% Y = ndnanfilter(X,HWIN,F);
% Y = ndnanfilter(X,HWIN,F,DIM);
% Y = ndnanfilter(X,HWIN,F,DIM,WINOPT);
% Y = ndnanfilter(X,HWIN,F,DIM,WINOPT,PADOPT);
% Y = ndnanfilter(X,HWIN,F,DIM,WINOPT,PADOPT,WNAN);
% [Y,W] = ndnanfilter(...);
%
% Input:
% X - Data to be filtered with/without NaNs.
% HWIN - Window function handle (or name) or numeric multidimensional
% window to be used (without NaNs). See WINDOW for details.
% Default: @rectwin or 'rectwin' (moving average).
% F - A vector specifying the semi-width of the window for each
% dimension. The final window's width will be 2*F+1.
% Default: 3 (i.e. a 1-dimensional window of width 6).
% DIM - If F is a single scalar, the window will be applied through
% this dimension; otherwise, this will be ignored.
% Default: columns (or the first non-singleton dimension).
% WINOPT - Cell array specifying optional arguments for the window
% function HWIN (in addition to the width).
% Default: {} (window's defaults).
% PADOPT - Cell array specifying the optional arguments for the
% PADARRAY MATLAB's function (in addition to the array X and
% the padsize: 2*F+1). If the function is not found, data is
% padded with zeros or the specified value: try {mean(X(:))}
% for example.
% Default: {'replicate'} (repeats border elements of X).
% Default: {0} (pads with zeros if PADARRAY not found).
% WNAN - Integer indicating NaNs treatment and program behaviour!:
% 0: Filters data and interpolates NaNs (default).
% 1: Filters data but do not interpolates NaNs
% 2: "Do not filters data" but interpolates NaNs!
% See the NOTEs below
%
% Output:
% Y - Filtered X data (same size as X!).
% W - N-dimensional window with central symmetry generated by a
% special subfunction called NDWIND. See the description below
% for details.
%
% Description:
% This function applies a N-dimensional convolution of X with W, using
% the MATLAB's IMFILTER or CONVN function. One important aspect of the
% function is the generation of the N-dimensional window (W) from the
% specified function and width, which cannot be done with MATLAB's
% functions. Besides, unlike MATLAB's FILTER, FILTER2 and IMFILTER,
% NaNs elements are taken into account (ignored).
%
% The N-dimensional window is generated from rotating the 1-dimensional
% output of the HWIN function, through each of the N-dimensions, and
% then shrinking it through each of its axes in order to fit the
% specified semi-widths (F). This is done in the included subfunction
% named NDWIND. In this way, the window has central symmetry and do not
% produce a phase shift on X data.
%
% By default, the edges are padded with the values of X at the borders
% with the PADARRAY MATLAB's function. In this way, the edges are
% treated smoothly. When PADARRAY is not found, the program performs
% zero-padding.
%
% Notes:
% * The use of semi-widths F's is to force the generated window to be
% even and, therefore, the change of phase is null.
% * The window function HWIN should output an even function, otherwise,
% it won't generate an error but the user should be aware that this
% program will consider only the last half of it.
% * The function window should return a monotonically decreasing
% result, this restriction is because I try to avoid the use of FZERO
% function, for example, to find the expanding/shrinking factors.
% * If the user has an already generated window, it can be used in HWIN
% instead of a function handle or name.
% * Accepts empty value for any input. When X is empty, the program can
% be used as a N-dimensional window generator.
% * NaNs elements surrounded by no-NaNs elements (which will depend on
% window width) are the ones that will be interpolated. The others
% are leaved untouched.
% * When WNAN=2, the programs acts like an NAN-interpolat/GAP-filling,
% leaving untouched the no-NaNs elements but the filtering is
% perfomed anyway. I recomend the default behaviour (WNAN=0) in order
% to keep the filtered data in the workspace, and then use the code
% at the end of this function to get/remove the interpolated NaNs
% (see the example).
% * The program looks for the IMFILTER and PADARRAY functions from the
% Image Processing Toolbox. If not found, then CONVN is used instead
% (slower) and pads with zeros or the given value. In this latter
% case, if border elements are NaNs, the window won't work properly.
%
% Example:
% FWIN = 'hamming';
% F = [13 8];
% N = 100;
% Pnoise = 0.30;
% PNaNs = 0.20;
% X = peaks(N); % original
% Y = X + ((rand(size(X))-0.5)*2)*max(X(:))*Pnoise; % add noise
% Y(round(1 + (N^2-1).*rand(N^2*PNaNs,1))) = NaN; % add NaNs
% [Z0,W] = ndnanfilter(Y,FWIN,F); % filters
% Z1 = Z0; Z2 = Y; inan = isnan(Y);
% Z1(inan) = NaN;
% Z2(inan) = Z0(inan);
% subplot(231), imagesc(X), clim = caxis; axis equal tight
% title('Original data')
% subplot(232), imagesc(Y), caxis(clim), axis equal tight
% title('Data + NOISE + NaNs')
% subplot(234), imagesc(Z0), caxis(clim), axis equal tight
% title('FILTERS + NaNs interpolation')
% subplot(235), imagesc(Z1), caxis(clim), axis equal tight
% title('FILTERS ignoring NaNs')
% subplot(236), imagesc(Z2), caxis(clim), axis equal tight
% title('GAP-filling with interpolated NaNs')
% subplot(233), imagesc(-F(1):F(1),-F(2):F(2),W), axis equal tight,
% title([upper(FWIN) ' 2D window']), view(2)
%
% See also: FILTER, FILTER2 and CONVN; WINDOW from the Signal Processing
% Toolbox; and FWIND1, FWIND2, FSPECIAL, IMFILTER and PADARRAY from the
% Image Processing Toolbox.
% Copyright 2008 Carlos Adrian Vargas Aguilera
% $Revision: 1.2 $ $Date: 2008/06/30 18:00:00 $
% Written by
% M.S. Carlos Adrian Vargas Aguilera
% Physical Oceanography PhD candidate
% CICESE
% Mexico, 2008
% nubeobscura@hotmail.com
%
% Download from:
% http://www.mathworks.com/matlabcentral/fileexchange/loadAuthor.do?objec
% tType=author&objectId=1093874
% 1.0 Release (2008/06/23 10:30:00)
% 1.1 Fixed Bug adding an extra dimension of unitary width.
% 1.2 Fixed Bug with ynan.
% Use the IMFILTER function? (faster than CONVN):
yimfilter = (exist('imfilter','file')==2);
% Use the PADARRAY function (or zero padding):
ypadarray = (exist('padarray','file')==2);
% Check inputs and sets defaults of principal arguments:
if nargin<3 || nargin>7
error('Filtern:IncorrectNumberOfInputs',...
'At least three inputs are needed and less than 7.')
end
if isempty(HWIN)
HWIN = 'rectwin';
end
if isempty(F)
F = 3;
end
N = length(F);
S = size(X);
% Secondary arguments:
if N && (nargin<4 || isempty(DIM))
DIM = find(S~=1,1); % DIM = min(find(S~=1));
if isempty(DIM), DIM = 1; end
end
if nargin<5 || isempty(WINOPT)
WINOPT = {};
end
if nargin<6 || isempty(PADOPT)
if ypadarray
PADOPT = {'replicate'};
else
PADOPT = {0};
end
elseif ~ypadarray && ~isnumeric(PADOPT{1})
PADOPT = {0};
end
if nargin<7 || isempty(WNAN)
WNAN = 0;
end
% Selects the 1-dimensional filter or set a row vector:
if N==1
a = zeros(1,DIM);
a(DIM) = F;
F = a;
clear a
end
% Checks if the window input is a function or an array:
if ~isa(HWIN,'function_handle') && ~ischar(HWIN)
W = HWIN;
else
W = [];
end
% If no input data but two outputs then generates the window only:
if isempty(X)
Y = [];
if nargout==2 && ~isempty(W)
W = ndwind(HWIN,F,WINOPT{:});
end
return
end
% Generates the window:
if isempty(W)
W = ndwind(HWIN,F,WINOPT{:});
end
% Check for NaN's:
inan = isnan(X);
ynan = any(inan(:)); % Bug fixed 30/jun/2008
if ynan
X(inan) = 0;
else
factor = sum(W(:));
end
% Filtering:
if yimfilter % Use IMFILTER (faster)
if ~isfloat(X)
X = double(X);
end
if ~isfloat(W)
W = double(W);
end
if ynan
Y = imfilter(X,W ,PADOPT{:},'conv');
else
Y = imfilter(X,W/factor,PADOPT{:},'conv');
end
else % Use CONVN
% Sets F and S of equal sizes.
F = reshape(F,1,N);
Nx = numel(S);
if N<Nx
F(N+1:Nx) = 0;
elseif N>Nx
S(Nx+1:N) = 1;
end
F2 = 2*F;
% Pads the borders:
if ypadarray
ind = padarray(false(S),F2,true ); % Index of the padding.
Y = padarray(X ,F2,PADOPT{:});
elseif length(PADOPT{1})==1
ind2 = cell(N,1);
for n = 1:N
ind2{n} = F2(n) + (1:S(n)).';
end
ind = repmat(true ,2*F2+S);
Y = repmat(PADOPT{1},2*F2+S);
ind(ind2{:}) = false;
Y(ind2{:}) = X;
else % No padding at all
Y = X;
ind = repmat(false,S);
warning('Ndnanfilter:PaddingOption','Do not perfom any padding.')
end
% Convolutes both arrays:
if ynan
Y = convn(Y,W ,'same');
else
Y = convn(Y,W/factor,'same');
end
% Eliminates the padding:
Y(ind) = [];
Y = reshape(Y,S);
end
% Estimates the averages when NaNs are present:
if ynan
if yimfilter
factor = imfilter(double(~inan),W,PADOPT{:},'conv');
else
if ypadarray
factor = padarray(~inan,F2,PADOPT{:});
elseif length(PADOPT{1})==1 % (won't work properly with NaNs at borders)
factor = ind;
factor(ind2{:}) = ~inan;
else
factor = ~inan;
end
factor = convn(factor,W,'same');
factor(ind) = [];
factor = reshape(factor,S);
end
Y = Y./factor;
end
% What about NaNs?:
if WNAN == 1 % Leave NaNs elements untouched!
Y(inan) = NaN;
elseif WNAN == 2 % Leave no-NaNs elements untouched!!!
X(inan) = Y(inan);
Y = X;
end
end
function W = ndwind(HWIN,F,varargin)
% NDWIND Generate a N-Dimensional zero-phase window.
%
% Syntax:
% W = ndwind(HWIN,F);
% W = ndwind(HWIN,F,OPT);
%
% Input:
% HWIN - Window function handle. See WINDOW for details. By default
% uses: @rectwin (a rectangular window).
% F - A vector specifying the semiwidth of the window for each
% dimension. The window's width will be 2*F+1. By default uses:
% 3 (i.e. a window of width 6).
% OPT - Cell array specifying optional arguments for the window
% function. By default uses: {[]} (window's defaults).
%
% Output:
% W - N-Dimensional window with central symmetry.
%
% Description:
% In the axes of each dimension, W has a 1-D window defined as
% feval(HWIN,2*F(n)+1), n = 1,...,N.
% That is, they are defined by the same window function but have
% different widths. So, this program creates another widther window (at
% least 201 points), with the same definition, and finds how much the
% former windows should be expanded in order to fit the latter one.
%
% Afterwards, the coordinates of every point are expanded accordingly
% and the value of the window in those points are found by linear
% interpolation with the bigger window.
%
% In resume, it is like rotating this big window through every
% dimension and then shrinking it through each of its axes to fix the
% specified widths.
%
% Notes:
% * Because of the use of the semi-widths F's, all the generated
% windows are even. Therefore the change of phase is null.
% * The window function HWIN should output an even function, otherwise,
% it won't generate an error but this program will consider only the
% last half of it.
% * The window should be monotonically decreasing.
% * Instead of the handle window, it can be given as a string:
% 'hamming' instead of @hamming, for example.
% * Uses the MATLAB's function FUNC2STR.
%
% Example:
% W = ndwind(@hamming,[3 2])
% % Results:
% W =
%
% 0 0 0.0800 0 0
% 0 0.1417 0.3100 0.1417 0
% 0 0.3966 0.7700 0.3966 0
% 0.0800 0.5400 1.0000 0.5400 0.0800
% 0 0.3966 0.7700 0.3966 0
% 0 0.1417 0.3100 0.1417 0
% 0 0 0.0800 0 0
%
%
% See also: WINDOW from the Signal Processing Toolbox; and FWIND1,
% FWIND2, and FSPECIAL from the Image Processing Toolbox.
% Copyright 2008 Carlos Adrian Vargas Aguilera
% $Revision: 1.1 $ $Date: 2008/06/26 19:30:00 $
% Written by
% M.S. Carlos Adrian Vargas Aguilera
% Physical Oceanography PhD candidate
% CICESE
% Mexico, 2008
% nubeobscura@hotmail.com
%
% Download from:
% http://www.mathworks.com/matlabcentral/fileexchange/loadAuthor.do?objec
% tType=author&objectId=1093874
% 1.0 Release (2008/06/23 10:30:00)
% 1.1 Fixed Bug adding an extra dimension of unitary width.
% Check inputs:
if nargin<1 || isempty(HWIN)
HWIN = 'rectwin';
end
if nargin<2 || isempty(F)
F = 3;
end
% Rectangular wind?:
if isa(HWIN,'function_handle')
HWIN = func2str(HWIN);
end
if strcmpi(HWIN,'rectwin')
W = ones([2*F(:).'+1 1]);
return
end
% Generate the BIG window (only the last half):
FBIG = max([100; F(:)]);
BIGw = feval(HWIN,2*FBIG+1,varargin{:});
BIGw(1:FBIG) = []; % Deletes the first half.
rBIGw = 0:FBIG; % Window argument (distance).
% Axial windows widths:
N = numel(F);
F = reshape(F,1,N);
F = [F 0]; % BUG fixed by adding an extra dimension.
N = N+1;
F2 = 2*F+1;
% Pre-allocates the final window and the expanded axis:
W = zeros(F2);
An = cell(N,1);
Ae = An;
% Generates the index and expanded axes:
for n = 1:N
% Generate temporally the window in the n-axis:
wn = feval(HWIN,F2(n),varargin{:});
% Finds the expansion factors (Note: the window should tends to zero):
if F(n)
piv = wn(end);
ind = (BIGw == piv);
if ~any(ind)
ind1 = (BIGw >= piv); ind1 = length(ind1(ind1));
ind2 = (BIGw <= piv); ind2 = length(ind2(~ind2))+1;
if ind2>FBIG+1
r = rBIGw(ind1);
else
r = interp1(BIGw([ind1 ind2]), rBIGw([ind1 ind2]),piv);
end
else
r = rBIGw(ind);
end
Ef = r/F(n);
else
Ef = 1;
end
% Reversed index and expanded n-axis (for the following grid):
An{n} = (F(n):-1:0);
Ae{n} = An{n}*Ef;
end
% Estimates the expanded distances outside the axes (only at the 1st
% quarter):
% Note: In a 2-Dimensional matrix, by the 1st quarter of a matrix I mean
% the first 1/4 piece of the matrix after you divided it throuh the middle
% row and column. In N-dimensions it would be the 1st 1/2^N part.
gride4 = cell(N,1);
[gride4{:}] = ndgrid(Ae{:});
R4 = sqrt(sum(reshape([gride4{:}],prod(F+1),N).^2,2));
% Generates the window and linear index in the 1st quarter:
grid4 = cell(N,1);
[grid4{:}]= ndgrid(An{:});
in = (R4<=rBIGw(end)); % Looks for elements inside window.
W4 = zeros(F+1); % 1st quarter of the window.
W4(in) = interp1(rBIGw,BIGw,R4(in)); % Interpolates the window values.
for n=1:N % Linear index on the 1st quarter.
grid4{n} = flipdim(grid4{n}+1,n);
end
ind4 = sub2ind(F2,grid4{:});
% Index of permutations to fill the N-D window:
np = 2^N-1;
ip = zeros(1,np);
for n = 1:N
ini = 2^(n-1);
step = ini*2;
ip(ini:step:np) = n;
end
% Fills the N-D window by flipping W4 and the index:
ones4 = repmat(false,F2); % Avoids using new FALSE function
ones4(ind4) = true;
W(ones4) = W4;
for kp = ip
W4 = flipdim(W4,kp);
ones4 = flipdim(ones4,kp);
W(ones4) = W4;
end
end