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If I have a nxnxn grid of values, say 32x32x32, and I want to rotate this cube grid of values by some rotation angle in either the x, y, or z axes, and interpolate missing values, what would be the best way to go about doing this without using any existing algorithms from packages (such as Scipy)?
I'm familiar with applying a 3D rotation matrix to a 3D grid of points when it's represented as a [n, 3] matrix, but I'm not sure how to go about applying a rotation when the representation is given in its 3D form as nxnxn.
I found a prior Stack Overflow post about this topic, but it uses three for loops for its approach, which doesn't really scale in terms of speed. Is there a more vectorized approach that can accomplish a similar task?
Thanks in advance!
One way I could think of would look like this:
reshape nxnxn matrix to an array containing n-dimensional points
apply rotation on this array
reshape array back to nxnxn
Here is some code:
import numpy as np
#just a way to create some nxnxn matrix
n = 4
a = np.arange(n)
b = np.array([a]*n)
mat = np.array([b]*n)
#creating an array containg n-dimensional points
flat_mat = mat.reshape((int(mat.size/n),n))
#just a random matrix we will use as a rotation
rot = np.eye(n) + 2
#apply the rotation on each n-dimensional point
result = np.array([rot.dot(x) for x in flat_mat])
#return to original shape
result=result.reshape((n,n,n))
print(result)
I want to plot a 2d hanning window function for a picture with N=512 pixels with a colorbar as vector graphics (*.svg, *.eps, (vectorized!) *.pdf or so)...
So I need to plot a 2d function
w(x,y) = sin(x*pi/N)^2 * sin(y*pi/N)^2
My solution for this was python first:
import numpy as np
from PIL import Image
im_hanning = Image.new("F", (N, N))
pix_hanning = im_hanning.load()
for x in range(0, N):
for y in range(0, N):
pix_hanning[x,y] = np.sin(x*np.pi/N)**2 * np.sin(y*np.pi/N)**2 * 255
im_hanning = Image.fromarray(array)
The result is this picture:
But this is a raster graphics of course.
So I tried it with gnuplot. This seemed better until I saw the result:
set xrange [0:1]
set yrange [0:1]
unset xtics
unset ytics
set pm3d map
set size square
set samples 512
set isosamples 512
set palette gray
splot sin(x*pi)**2 * sin(y*pi)**2
I had to increase the samples, else it looked terrible... The result looks fine:
I especially like the colorbar on the right. But this produces (no matter what terminal I set) raster graphics again.
Is there a possibility to plot a 2d function as vector graphics?
With a PDF, SVG or EPS terminal, gnuplot does give you vector graphics. But the function has to be represented in some way, and what gnuplot does is a piecewise linear interpolation, that is, the surface is represented by small portions of plane (triangles or quadrangles), the number of which is set by the sampling rate.
If you want an infinitely scalable colour map, the way to produce it has to be a primitive of the scalable vector language you are using, e.g. SVG. So this is your real question: is there an SVG/PDF/EPS primitive to represent the gradient sin(x*pi)**2 * sin(y*pi)**2. I believe this is not the case, colour gradients are also piecewise linear AFAIK, but asked in this way you may attract answers from specialists.
As the title suggests, how would one create a numpy array of 3D coordinates of a geometric shape?
Currently, I have the easiest shape already figured out:
latva = 6
latvb = 6
latvc = 6
latdiv = 20
latvadiv = latva / latdiv
latvbdiv = latvb / latdiv
latvcdiv = latvc / latdiv
lol = np.zeros((latdiv**3,4),dtype=np.float64)
lol[:,:3] = (np.arange(latdiv**3)[:,None]//(latdiv**2,latdiv,1)*(latvadiv,latvbdiv,latvcdiv)%(latva,latvb,latvc))
creates an array of (8000,4). If you then split the array along the 1,2,3 column (Ignoring the 4th as it's meaningless in this question) and plot it (Personally, I use pyplot) you get a Cube!
Easy enough. Also works for a rectangle.
But I've not the foggiest idea of how to get any further - say plotting a rhombus.
I'm not interested in black magic like spheres, ovals or shapes whose sides do not change following a line. Just things like your standard rhombus/Rhomboid/Parallelepiped/Whatever_you_want_to_call_it.
Any ideas on how to accomplish this?
Because you already have convenient method to generate points in square or cube, the simplest way to make rhombus, parallelogram for 2D case and parallelepiped for 3D case is to apply affine transform to calculate new point coordinates.
For example, to make rhombus, you can find matrix as combination of translation by (-centerX, -centerY), rotation by Pi/4, scaling along axes (if needed) and translation to needed position.
AffMatrix = ShiftMatrix * RotateMatrix * ScaleMatrix * BackShiftMatrix
for each point coordinates:
(NewX, NewY) = (AffMatrix) * (X, Y)
Rhomboid will include also shear transform.
I think that numpy has ready-to-use routines to create and combine (multiply) affine matrices.
I'm trying to get python to return, as close as possible, the center of the most obvious clustering in an image like the one below:
In my previous question I asked how to get the global maximum and the local maximums of a 2d array, and the answers given worked perfectly. The issue is that the center estimation I can get by averaging the global maximum obtained with different bin sizes is always slightly off than the one I would set by eye, because I'm only accounting for the biggest bin instead of a group of biggest bins (like one does by eye).
I tried adapting the answer to this question to my problem, but it turns out my image is too noisy for that algorithm to work. Here's my code implementing that answer:
import numpy as np
from scipy.ndimage.filters import maximum_filter
from scipy.ndimage.morphology import generate_binary_structure, binary_erosion
import matplotlib.pyplot as pp
from os import getcwd
from os.path import join, realpath, dirname
# Save path to dir where this code exists.
mypath = realpath(join(getcwd(), dirname(__file__)))
myfile = 'data_file.dat'
x, y = np.loadtxt(join(mypath,myfile), usecols=(1, 2), unpack=True)
xmin, xmax = min(x), max(x)
ymin, ymax = min(y), max(y)
rang = [[xmin, xmax], [ymin, ymax]]
paws = []
for d_b in range(25, 110, 25):
# Number of bins in x,y given the bin width 'd_b'
binsxy = [int((xmax - xmin) / d_b), int((ymax - ymin) / d_b)]
H, xedges, yedges = np.histogram2d(x, y, range=rang, bins=binsxy)
paws.append(H)
def detect_peaks(image):
"""
Takes an image and detect the peaks usingthe local maximum filter.
Returns a boolean mask of the peaks (i.e. 1 when
the pixel's value is the neighborhood maximum, 0 otherwise)
"""
# define an 8-connected neighborhood
neighborhood = generate_binary_structure(2,2)
#apply the local maximum filter; all pixel of maximal value
#in their neighborhood are set to 1
local_max = maximum_filter(image, footprint=neighborhood)==image
#local_max is a mask that contains the peaks we are
#looking for, but also the background.
#In order to isolate the peaks we must remove the background from the mask.
#we create the mask of the background
background = (image==0)
#a little technicality: we must erode the background in order to
#successfully subtract it form local_max, otherwise a line will
#appear along the background border (artifact of the local maximum filter)
eroded_background = binary_erosion(background, structure=neighborhood, border_value=1)
#we obtain the final mask, containing only peaks,
#by removing the background from the local_max mask
detected_peaks = local_max - eroded_background
return detected_peaks
#applying the detection and plotting results
for i, paw in enumerate(paws):
detected_peaks = detect_peaks(paw)
pp.subplot(4,2,(2*i+1))
pp.imshow(paw)
pp.subplot(4,2,(2*i+2) )
pp.imshow(detected_peaks)
pp.show()
and here's the result of that (varying the bin size):
Clearly my background is too noisy for that algorithm to work, so the question is: how can I make that algorithm less sensitive? If an alternative solution exists then please let me know.
EDIT
Following Bi Rico advise I attempted smoothing my 2d array before passing it on to the local maximum finder, like so:
H, xedges, yedges = np.histogram2d(x, y, range=rang, bins=binsxy)
H1 = gaussian_filter(H, 2, mode='nearest')
paws.append(H1)
These were the results with a sigma of 2, 4 and 8:
EDIT 2
A mode ='constant' seems to work much better than nearest. It converges to the right center with a sigma=2 for the largest bin size:
So, how do I get the coordinates of the maximum that shows in the last image?
Answering the last part of your question, always you have points in an image, you can find their coordinates by searching, in some order, the local maximums of the image. In case your data is not a point source, you can apply a mask to each peak in order to avoid the peak neighborhood from being a maximum while performing a future search. I propose the following code:
import matplotlib.image as mpimg
import matplotlib.pyplot as plt
import numpy as np
import copy
def get_std(image):
return np.std(image)
def get_max(image,sigma,alpha=20,size=10):
i_out = []
j_out = []
image_temp = copy.deepcopy(image)
while True:
k = np.argmax(image_temp)
j,i = np.unravel_index(k, image_temp.shape)
if(image_temp[j,i] >= alpha*sigma):
i_out.append(i)
j_out.append(j)
x = np.arange(i-size, i+size)
y = np.arange(j-size, j+size)
xv,yv = np.meshgrid(x,y)
image_temp[yv.clip(0,image_temp.shape[0]-1),
xv.clip(0,image_temp.shape[1]-1) ] = 0
print xv
else:
break
return i_out,j_out
#reading the image
image = mpimg.imread('ggd4.jpg')
#computing the standard deviation of the image
sigma = get_std(image)
#getting the peaks
i,j = get_max(image[:,:,0],sigma, alpha=10, size=10)
#let's see the results
plt.imshow(image, origin='lower')
plt.plot(i,j,'ro', markersize=10, alpha=0.5)
plt.show()
The image ggd4 for the test can be downloaded from:
http://www.ipac.caltech.edu/2mass/gallery/spr99/ggd4.jpg
The first part is to get some information about the noise in the image. I did it by computing the standard deviation of the full image (actually is better to select an small rectangle without signal). This is telling us how much noise is present in the image.
The idea to get the peaks is to ask for successive maximums, which are above of certain threshold (let's say, 3, 4, 5, 10, or 20 times the noise). This is what the function get_max is actually doing. It performs the search of maximums until one of them is below the threshold imposed by the noise. In order to avoid finding the same maximum many times it is necessary to remove the peaks from the image. In the general way, the shape of the mask to do so depends strongly on the problem that one want to solve. for the case of stars, it should be good to remove the star by using a Gaussian function, or something similar. I have chosen for simplicity a square function, and the size of the function (in pixels) is the variable "size".
I think that from this example, anybody can improve the code by adding more general things.
EDIT:
The original image looks like:
While the image after identifying the luminous points looks like this:
Too much of a n00b on Stack Overflow to comment on Alejandro's answer elsewhere here. I would refine his code a bit to use a preallocated numpy array for output:
def get_max(image,sigma,alpha=3,size=10):
from copy import deepcopy
import numpy as np
# preallocate a lot of peak storage
k_arr = np.zeros((10000,2))
image_temp = deepcopy(image)
peak_ct=0
while True:
k = np.argmax(image_temp)
j,i = np.unravel_index(k, image_temp.shape)
if(image_temp[j,i] >= alpha*sigma):
k_arr[peak_ct]=[j,i]
# this is the part that masks already-found peaks.
x = np.arange(i-size, i+size)
y = np.arange(j-size, j+size)
xv,yv = np.meshgrid(x,y)
# the clip here handles edge cases where the peak is near the
# image edge
image_temp[yv.clip(0,image_temp.shape[0]-1),
xv.clip(0,image_temp.shape[1]-1) ] = 0
peak_ct+=1
else:
break
# trim the output for only what we've actually found
return k_arr[:peak_ct]
In profiling this and Alejandro's code using his example image, this code about 33% faster (0.03 sec for Alejandro's code, 0.02 sec for mine.) I expect on images with larger numbers of peaks, it would be even faster - appending the output to a list will get slower and slower for more peaks.
I think the first step needed here is to express the values in H in terms of the standard deviation of the field:
import numpy as np
H = H / np.std(H)
Now you can put a threshold on the values of this H. If the noise is assumed to be Gaussian, picking a threshold of 3 you can be quite sure (99.7%) that this pixel can be associated with a real peak and not noise. See here.
Now the further selection can start. It is not exactly clear to me what exactly you want to find. Do you want the exact location of peak values? Or do you want one location for a cluster of peaks which is in the middle of this cluster?
Anyway, starting from this point with all pixel values expressed in standard deviations of the field, you should be able to get what you want. If you want to find clusters you could perform a nearest neighbour search on the >3-sigma gridpoints and put a threshold on the distance. I.e. only connect them when they are close enough to each other. If several gridpoints are connected you can define this as a group/cluster and calculate some (sigma-weighted?) center of the cluster.
Hope my first contribution on Stackoverflow is useful for you!
The way I would do it:
1) normalize H between 0 and 1.
2) pick a threshold value, as tcaswell suggests. It could be between .9 and .99 for example
3) use masked arrays to keep only the x,y coordinates with H above threshold:
import numpy.ma as ma
x_masked=ma.masked_array(x, mask= H < thresold)
y_masked=ma.masked_array(y, mask= H < thresold)
4) now you can weight-average on the masked coordinates, with weight something like (H-threshold)^2, or any other power greater or equal to one, depending on your taste/tests.
Comment:
1) This is not robust with respect to the type of peaks you have, since you may have to adapt the thresold. This is the minor problem;
2) This DOES NOT work with two peaks as it is, and will give wrong results if the 2nd peak is above threshold.
Nonetheless, it will always give you an answer without crashing (with pros and cons of the thing..)
I'm adding this answer because it's the solution I ended up using. It's a combination of Bi Rico's comment here (May 30 at 18:54) and the answer given in this question: Find peak of 2d histogram.
As it turns out using the peak detection algorithm from this question Peak detection in a 2D array only complicates matters. After applying the Gaussian filter to the image all that needs to be done is to ask for the maximum bin (as Bi Rico pointed out) and then obtain the maximum in coordinates.
So instead of using the detect-peaks function as I did above, I simply add the following code after the Gaussian 2D histogram is obtained:
# Get 2D histogram.
H, xedges, yedges = np.histogram2d(x, y, range=rang, bins=binsxy)
# Get Gaussian filtered 2D histogram.
H1 = gaussian_filter(H, 2, mode='nearest')
# Get center of maximum in bin coordinates.
x_cent_bin, y_cent_bin = np.unravel_index(H1.argmax(), H1.shape)
# Get center in x,y coordinates.
x_cent_coor , y_cent_coord = np.average(xedges[x_cent_bin:x_cent_bin + 2]), np.average(yedges[y_cent_g:y_cent_g + 2])
So, I have three numpy arrays which store latitude, longitude, and some property value on a grid -- that is, I have LAT(y,x), LON(y,x), and, say temperature T(y,x), for some limits of x and y. The grid isn't necessarily regular -- in fact, it's tripolar.
I then want to interpolate these property (temperature) values onto a bunch of different lat/lon points (stored as lat1(t), lon1(t), for about 10,000 t...) which do not fall on the actual grid points. I've tried matplotlib.mlab.griddata, but that takes far too long (it's not really designed for what I'm doing, after all). I've also tried scipy.interpolate.interp2d, but I get a MemoryError (my grids are about 400x400).
Is there any sort of slick, preferably fast way of doing this? I can't help but think the answer is something obvious... Thanks!!
Try the combination of inverse-distance weighting and
scipy.spatial.KDTree
described in SO
inverse-distance-weighted-idw-interpolation-with-python.
Kd-trees
work nicely in 2d 3d ..., inverse-distance weighting is smooth and local,
and the k= number of nearest neighbours can be varied to tradeoff speed / accuracy.
There is a nice inverse distance example by Roger Veciana i Rovira along with some code using GDAL to write to geotiff if you're into that.
This is of coarse to a regular grid, but assuming you project the data first to a pixel grid with pyproj or something, all the while being careful what projection is used for your data.
A copy of his algorithm and example script:
from math import pow
from math import sqrt
import numpy as np
import matplotlib.pyplot as plt
def pointValue(x,y,power,smoothing,xv,yv,values):
nominator=0
denominator=0
for i in range(0,len(values)):
dist = sqrt((x-xv[i])*(x-xv[i])+(y-yv[i])*(y-yv[i])+smoothing*smoothing);
#If the point is really close to one of the data points, return the data point value to avoid singularities
if(dist<0.0000000001):
return values[i]
nominator=nominator+(values[i]/pow(dist,power))
denominator=denominator+(1/pow(dist,power))
#Return NODATA if the denominator is zero
if denominator > 0:
value = nominator/denominator
else:
value = -9999
return value
def invDist(xv,yv,values,xsize=100,ysize=100,power=2,smoothing=0):
valuesGrid = np.zeros((ysize,xsize))
for x in range(0,xsize):
for y in range(0,ysize):
valuesGrid[y][x] = pointValue(x,y,power,smoothing,xv,yv,values)
return valuesGrid
if __name__ == "__main__":
power=1
smoothing=20
#Creating some data, with each coodinate and the values stored in separated lists
xv = [10,60,40,70,10,50,20,70,30,60]
yv = [10,20,30,30,40,50,60,70,80,90]
values = [1,2,2,3,4,6,7,7,8,10]
#Creating the output grid (100x100, in the example)
ti = np.linspace(0, 100, 100)
XI, YI = np.meshgrid(ti, ti)
#Creating the interpolation function and populating the output matrix value
ZI = invDist(xv,yv,values,100,100,power,smoothing)
# Plotting the result
n = plt.normalize(0.0, 100.0)
plt.subplot(1, 1, 1)
plt.pcolor(XI, YI, ZI)
plt.scatter(xv, yv, 100, values)
plt.title('Inv dist interpolation - power: ' + str(power) + ' smoothing: ' + str(smoothing))
plt.xlim(0, 100)
plt.ylim(0, 100)
plt.colorbar()
plt.show()
There's a bunch of options here, which one is best will depend on your data...
However I don't know of an out-of-the-box solution for you
You say your input data is from tripolar data. There are three main cases for how this data could be structured.
Sampled from a 3d grid in tripolar space, projected back to 2d LAT, LON data.
Sampled from a 2d grid in tripolar space, projected into 2d LAT LON data.
Unstructured data in tripolar space projected into 2d LAT LON data
The easiest of these is 2. Instead of interpolating in LAT LON space, "just" transform your point back into the source space and interpolate there.
Another option that works for 1 and 2 is to search for the cells that maps from tripolar space to cover your sample point. (You can use a BSP or grid type structure to speed up this search) Pick one of the cells, and interpolate inside it.
Finally there's a heap of unstructured interpolation options .. but they tend to be slow.
A personal favourite of mine is to use a linear interpolation of the nearest N points, finding those N points can again be done with gridding or a BSP. Another good option is to Delauney triangulate the unstructured points and interpolate on the resulting triangular mesh.
Personally if my mesh was case 1, I'd use an unstructured strategy as I'd be worried about having to handle searching through cells with overlapping projections. Choosing the "right" cell would be difficult.
I suggest you taking a look at GRASS (an open source GIS package) interpolation features (http://grass.ibiblio.org/gdp/html_grass62/v.surf.bspline.html). It's not in python but you can reimplement it or interface with C code.
Am I right in thinking your data grids look something like this (red is the old data, blue is the new interpolated data)?
alt text http://www.geekops.co.uk/photos/0000-00-02%20%28Forum%20images%29/DataSeparation.png
This might be a slightly brute-force-ish approach, but what about rendering your existing data as a bitmap (opengl will do simple interpolation of colours for you with the right options configured and you could render the data as triangles which should be fairly fast). You could then sample pixels at the locations of the new points.
Alternatively, you could sort your first set of points spatially and then find the closest old points surrounding your new point and interpolate based on the distances to those points.
There is a FORTRAN library called BIVAR, which is very suitable for this problem. With a few modifications you can make it usable in python using f2py.
From the description:
BIVAR is a FORTRAN90 library which interpolates scattered bivariate data, by Hiroshi Akima.
BIVAR accepts a set of (X,Y) data points scattered in 2D, with associated Z data values, and is able to construct a smooth interpolation function Z(X,Y), which agrees with the given data, and can be evaluated at other points in the plane.