fisher's linear discriminant in Python - python

I have the fisher's linear discriminant that i need to use it to reduce my examples A and B that are high dimensional matrices to simply 2D, that is exactly like LDA, each example has classes A and B, therefore if i was to have a third example they also have classes A and B, fourth, fifth and n examples would always have classes A and B, therefore i would like to separate them in a simple use of fisher's linear discriminant. Im pretty much new to machine learning, so i dont know how to separate my classes, i've been following the formula by eye and coding on the go. From what i was reading, i need to apply a linear transformation to my data so i can find a good threshold for it, but first i'd need to find the maximization function. For such task, i managed to find Sw and Sb, but i don't know how to go from there...
Where i also need to find the maximization function.
That maximization function gives me an eigen value solution:
What i have for each classes are matrices 5x2 of 2 examples. For instance:
Example 1
Class_A = [
201, 103,
40, 43,
23, 50,
12, 123,
99, 78
]
Class_B = [
201, 129,
114, 195,
180, 90,
69, 62,
76, 90
]
Example 2
Class_A = [
68, 98,
201, 203,
78, 212,
49, 5,
204, 78
]
Class_B = [
52, 19,
220, 219,
159, 195,
99, 23,
46, 50
]
I tried finding Sw for the example above like this:
Example_1_Class_A = np.dot(Example_1_Class_A, np.transpose(Example_1_Class_A))
Example_1_Class_B = np.dot(Example_1_Class_B, np.transpose(Example_1_Class_B))
Example_2_Class_A = np.dot(Example_2_Class_A, np.transpose(Example_2_Class_A))
Example_2_Class_B = np.dot(Example_2_Class_B, np.transpose(Example_2_Class_B))
Sw = sum([Example_1_Class_A, Example_1_Class_B, Example_2_Class_A, Example_2_Class_B], axis=0)
As for Sb, i tried like this:
Example_1_Class_A_mean = Example_1_Class_A.mean(axis=0)
Example_1_Class_B_mean = Example_1_Class_B.mean(axis=0)
Example_2_Class_A_mean = Example_2_Class_A.mean(axis=0)
Example_2_Class_B_mean = Example_2_Class_B.mean(axis=0)
Example_1_Class_A_Sb = np.dot(Example_1_Class_A_mean, np.transpose(Example_1_Class_A_mean))
Example_1_Class_B_Sb = np.dot(Example_1_Class_B_mean, np.transpose(Example_1_Class_B_mean))
Example_2_Class_A_Sb = np.dot(Example_2_Class_A_mean, np.transpose(Example_2_Class_A_mean))
Example_2_Class_B_Sb = np.dot(Example_2_Class_B_mean, np.transpose(Example_2_Class_B_mean))
Sb = sum([Example_1_Class_A_Sb, Example_1_Class_B_Sb, Example_2_Class_A_Sb, Example_2_Class_B_Sb], axis=0)
The problem is, i have no idea what else to do with my Sw and Sb, i am completely lost. Basically, what i need to do is get from here to this:
How for given Example A and Example B, do i separate a cluster only for classes As and only for classes b

Before answering your question, I will first touch the basic difference between PCA and (F)LDA. In PCA you don't know anything about underlying classes, but you assume that the information about classes separability lies in the variance of data. So you rotate your original axes (sometimes it is called projecting all the data onto new ones) in such way that your first new axis is pointing to the direction of most variance, second one is perpendicular to the first one and pointing to the direction of most residiual variance, and so on. This way a PCA transformation results in a (sub)space of the same dimensionality as the original one. Than you can take only first 2 dimensions, rejecting the rest, hence getting a dimensionality reduction from k dimensions to only 2.
LDA works a bit differently. In this case you know in advance how many classes there are in your data, and you can find their mean and covariance matrices. What Fisher criterion does it finds a direction in which the mean between classes is maximized, while at the same time total variability is minimized (total variability is a mean of within-class covariance matrices). And for each two classes there is only one such line. This is why when your data has C classes, LDA can provide you at most C-1 dimensions, regardless of the original data dimensionality. In your case this means that as you have only 2 classes A and B, you will get a one-dimensional projection, i.e. a line. And this is exactly what you have in your picture: original 2d data is projected on to a line. The direction of the line is the solution of the eigenproblem.
Let's generate data that is similar to your picture:
a = np.random.multivariate_normal((1.5, 3), [[0.5, 0], [0, .05]], 30)
b = np.random.multivariate_normal((4, 1.5), [[0.5, 0], [0, .05]], 30)
plt.plot(a[:,0], a[:,1], 'b.', b[:,0], b[:,1], 'r.')
mu_a, mu_b = a.mean(axis=0).reshape(-1,1), b.mean(axis=0).reshape(-1,1)
Sw = np.cov(a.T) + np.cov(b.T)
inv_S = np.linalg.inv(Sw)
res = inv_S.dot(mu_a-mu_b) # the trick
####
# more general solution
#
# Sb = (mu_a-mu_b)*((mu_a-mu_b).T)
# eig_vals, eig_vecs = np.linalg.eig(inv_S.dot(Sb))
# res = sorted(zip(eig_vals, eig_vecs), reverse=True)[0][1] # take only eigenvec corresponding to largest (and the only one) eigenvalue
# res = res / np.linalg.norm(res)
plt.plot([-res[0], res[0]], [-res[1], res[1]]) # this is the solution
plt.plot(mu_a[0], mu_a[1], 'cx')
plt.plot(mu_b[0], mu_b[1], 'yx')
plt.gca().axis('square')
# let's project data point on it
r = res.reshape(2,)
n2 = np.linalg.norm(r)**2
for pt in a:
prj = r * r.dot(pt) / n2
plt.plot([prj[0], pt[0]], [prj[1], pt[1]], 'b.:', alpha=0.2)
for pt in b:
prj = r * r.dot(pt) / n2
plt.plot([prj[0], pt[0]], [prj[1], pt[1]], 'r.:', alpha=0.2)
The resulting projection is calculated using a neat trick for two class problem. You can read details on it here in section 1.6.
Regarding the "examples" you mention in your question. I believe you need to repeat the process for each example, as it is a different set of data point probably with different distributions. Also, put attention that estimated mean (mu_a, mu_b) and class covariance matrices would be slightly different from the ones that data was generated with, especially for small sample size.

Mathematics
See https://sebastianraschka.com/Articles/2014_python_lda.html#lda-in-5-steps for more information.
Implementation using Iris
Since you want to use LDA for dimensionality reduction but provide only 2d data I am showing how to perform this procedure on the iris dataset.
Let's import libraries
import pandas as pd
import numpy as np
import sklearn as sk
from collections import Counter
from sklearn import datasets
# load dataset and transform to pandas df
X, y = datasets.load_iris(return_X_y=True)
X = pd.DataFrame(X, columns=[f'feat_{i}' for i in range(4)])
y = pd.DataFrame(y, columns=['labels'])
tot = pd.concat([X,y], axis=1)
# calculate class means
class_means = tot.groupby('labels').mean()
total_mean = X.mean()
The class_means are given by:
class_means
feat_0 feat_1 feat_2 feat_3
labels
0 5.006 3.428 1.462 0.246
1 5.936 2.770 4.260 1.326
2 6.588 2.974 5.552 2.026
To do this, we first subtract the class means from each observation (basically we calculate x - m_i from the equation above).
Subtract the corresponding class mean from each observation. Since we want to calculate
x_mi = tot.transform(lambda x: x - class_means.loc[x['labels']], axis=1).drop('labels', 1)
def kronecker_and_sum(df, weights):
S = np.zeros((df.shape[1], df.shape[1]))
for idx, row in df.iterrows():
x_m = row.as_matrix().reshape(df.shape[1],1)
S += weights[idx]*np.dot(x_m, x_m.T)
return S
# Each x_mi is weighted with 1. Now we use the kronecker_and_sum function to calculate the within-class scatter matrix S_w
S_w = kronecker_and_sum(x_mi, 150*[1])
mi_m = class_means.transform(lambda x: x - total_mean, axis=1)
# Each mi_m is weighted with the number of observations per class which is 50 for each class in this example. We use kronecker_and_sum to calculate the between-class scatter matrix.
S_b=kronecker_and_sum(mi_m, 3*[50])
eig_vals, eig_vecs = np.linalg.eig(np.linalg.inv(S_w).dot(S_b))
We only need to consider the eigenvalues which are remarkably different from zero (in this case only the first two)
eig_vals
array([ 3.21919292e+01, 2.85391043e-01, 6.53468167e-15, -2.24877550e-15])
Transform X with the matrix of the two eigenvectors which correspond to the highest eigenvalues
W = eig_vecs[:, :2]
X_trafo = np.dot(X, W)
tot_trafo = pd.concat([pd.DataFrame(X_trafo, index=range(len(X_trafo))), y], 1)
# plot the result
tot_trafo.plot.scatter(x=0, y=1, c='labels', colormap='viridis')
We have reduced the dimensions from 4 to 2 and chosen the space in such a way, that the classes can be well seperated.
Scikit-learn usage
Scikit has LDA support aswell. What we did in dozens of lines can be done with the following lines of code:
from sklearn import discriminant_analysis
lda = discriminant_analysis.LinearDiscriminantAnalysis(n_components=2)
X_trafo_sk = lda.fit_transform(X,y)
pd.DataFrame(np.hstack((X_trafo_sk, y))).plot.scatter(x=0, y=1, c=2, colormap='viridis')
I'm not giving a plot here, cause it is the same as in our derived example (except for a 180 degree rotation).

Related

Principle Component Analysis, add a line to the 3d graph showing the first principal component

I am conducting PCA on a dataset. I am attempting to add a line in my 3d graph which shows the first principal component. I have tried a few methods but have not been able to display the first principal component as a line in my 3d graph. Any help is greatly appreciated. My code is as follows:
import numpy as np
np.set_printoptions (suppress=True, precision=5, linewidth=150)
import pandas as pd
from sklearn.decomposition import PCA
from sklearn.preprocessing import LabelEncoder
from mpl_toolkits.mplot3d import Axes3D
import matplotlib.pyplot as plt
file_name = 'C:/Users/data'
input_data = pd.read_csv (file_name + '.csv', header=0, index_col=0)
A = input_data.A.values.astype(float)
B = input_data.B.values.astype(float)
C = input_data.C.values.astype(float)
D = input_data.D.values.astype(float)
E = input_data.E.values.astype(float)
F = input_data.F.values.astype(float)
X = np.column_stack((A, B, C, D, E, F))
ncompo = int (input ("Number of components to study: "))
print("")
pca = PCA (n_components = ncompo)
pcafit = pca.fit(X)
cov_mat = np.cov(X, rowvar=0)
eig_vals, eig_vecs = np.linalg.eig(cov_mat)
perc = pcafit.explained_variance_ratio_
perc_x = range(1, len(perc)+1)
plt.plot(perc_x, perc)
plt.xlabel('Components')
plt.ylabel('Percentage of Variance Explained')
plt.show()
#3d Graph
plt.clf()
le = LabelEncoder()
le.fit(input_data.Grade)
number = le.transform(input_data.Grade)
colormap = np.array(['green', 'blue', 'red', 'yellow'])
fig = plt.figure()
ax = fig.add_subplot(111, projection='3d')
ax.scatter(D, E, F, c=colormap[number])
ax.set_xlabel('D')
ax.set_ylabel('E')
ax.set_zlabel('F')
plt.title('PCA')
plt.show()
Some remarks to begin with:
You are computing PCA twice! To compute PCA is to compute eigen values and eigen vectors of the covariance matrix. So, either you use the sklearn function pca.fit, either you do it yourself. But you don't need to do both, unless you want to discover pca.fit and see for yourself that it does exactly what you expect it to do (if this is what you wanted, fine. It is a good thing to do that king of checking. I did this once also). Of course pca.fit has another advantage: once you have it, it also provides pca.predict to project points in the components space. But that also is simply a base change using eigenvectors matrix (that is matrix to change base)
pca object let you get the eigenvectors (pca.components_) and eigen values (pca.explained_variance_)
pca.fit is a 'inplace' method. It does not return a new PCA object. It just fit the one you have. So, no need to get pcafit and use it.
This is not a minimal reproducible exemple as required on SO. We should be able to copy and paste it, and run it, so see exactly your problem. Not to guess what kind of secret data you have. And in the meantime, it should be minimal. So, contains data example generation (it doesn't matter if those data doesn't make sense. Sometimes it is even better, since it allows some testing. In my following code, I generate my own noisy data along an axis, which allow me to verify that, indeed, I am able to "guess" what was that axis). Plus, since your problem concerns only 3d plot, there is no need to include ploting of explained variance here. That part is not part of your question.
Now, to print the principal component, well, you already did the hard part. Twice. That is to compute it. It is the eigenvector associated with the highest eigenvalue.
With pca object no need to search for it, they are already sorted. So it is simply pca.components_[0]. And since you want to plot in the space D,E,F, you simply need to draw vector pca.components_[0][3:].
With correct scaling.
You can do that with plot providing just 2 points (first and last)
Here is my version (which, by the way, shows also what a minimal reproducible example is)
import numpy as np
np.set_printoptions (suppress=True, precision=5, linewidth=150)
import pandas as pd
from sklearn.decomposition import PCA
from sklearn.preprocessing import LabelEncoder
from mpl_toolkits.mplot3d import Axes3D
import matplotlib.pyplot as plt
# Generation of random data along a given vector
vec=np.array([1, -1, 0.5, -0.5, 0.75, 0.75]).reshape(-1,1)
# 10000 random data, that are U[0,10]×vec + gaussian noise std=1
X=(vec*np.random.rand(10000)*10 + np.random.normal(0,1,(6,10000))).T
(A,B,C,D,E,F)=X.T
input_data = pd.DataFrame({'A':A,'B':B,'C':C,'D':D,'E':E, 'F':F, 'Grade':np.random.randint(1,5, (10000,))})
ncompo=6
pca = PCA (n_components = ncompo)
pca.fit(X)
# Redundant
cov_mat = np.cov(X, rowvar=0)
eig_vals, eig_vecs = np.linalg.eig(cov_mat)
# See
print("Eigen values")
print(eig_vals)
print(pca.explained_variance_)
print("Eigen vec")
print(eig_vecs)
print(pca.components_)
# Note, compare first components to
print("Main component")
print(vec/np.linalg.norm(vec))
print(pca.components_[0])
#3d Graph
le = LabelEncoder()
le.fit(input_data.Grade)
number = le.transform(input_data.Grade)
fig = plt.figure()
colormap = np.array(['green', 'blue', 'red', 'yellow'])
ax = fig.add_subplot(111, projection='3d')
ax.scatter(D, E, F, c=colormap[number])
U=pca.components_[0]
sc1=max(D)/U[3]
sc2=min(D)/U[3]
# Draw the 1st principal component as a blue line
ax.plot([sc1*U[3],sc2*U[3]], [sc1*U[4], sc2*U[4]], [sc1*U[5], sc2*U[5]], linewidth=3)
ax.set_xlabel('D')
ax.set_ylabel('E')
ax.set_zlabel('F')
plt.title('PCA')
plt.show()
My example is not that minimal, because I took advantage of it to illustrate my first remark, and also computed PCA twice, to compare both result.
So, here I print, eigenvalues
Eigen values
[30.88941 1.01334 0.99512 0.96493 0.97692 0.98101]
[30.88941 1.01334 0.99512 0.98101 0.97692 0.96493]
(1st being your computation by diagonalisation of covariance matrix, 2nd pca.explained_variance_)
As you can see, they are the same, except sorting for the 1st one
Like wise,
Eigen vec
[[-0.52251 -0.27292 0.40863 -0.06321 0.26699 0.6405 ]
[ 0.52521 0.07577 -0.34211 0.27583 -0.04161 0.72357]
[-0.26266 -0.41332 -0.60091 0.38027 0.47573 -0.16779]
[ 0.26354 -0.52548 0.47284 0.59159 -0.24029 -0.15204]
[-0.39493 0.63946 0.07496 0.64966 -0.08619 0.00252]
[-0.3959 -0.25276 -0.35452 -0.0572 -0.79718 0.12217]]
[[ 0.52251 -0.52521 0.26266 -0.26354 0.39493 0.3959 ]
[-0.27292 0.07577 -0.41332 -0.52548 0.63946 -0.25276]
[-0.40863 0.34211 0.60091 -0.47284 -0.07496 0.35452]
[-0.6405 -0.72357 0.16779 0.15204 -0.00252 -0.12217]
[-0.26699 0.04161 -0.47573 0.24029 0.08619 0.79718]
[-0.06321 0.27583 0.38027 0.59159 0.64966 -0.0572 ]]
Also the same, but for sorting and transpose.
Eigen vectors are presented column wise when you diagonalize a matrix.
Where as for pca.components_ each line is an eigen vector.
But you can see that in the 1st matrix, the eigen vector associated to the biggest eigen value, that is, since biggest eigen value was the 1st one, the 1st column (-0.52, 0.52, etc.)
is also the same as the first line of pca.components_.
Like wise, the 4th biggest eigen value in your diagonalisation was the last one.
And if you look at the last column of your eigen vectors (0.64, 0.72, -0.76...), it is the same as the 4th line of pca.components_ (with a irrelevant ×-1 factor)
So, long story short, you already have eigenvals in pca.explained_variance_ sorted from the biggest to the smallest. And eigen vectors in pca_components_, in the same order.
Last thing I print here, is comparison between the first component (pca.components_[0]) and the vector I used to generate the data in the first place (my data are all colinear to a vector vec, + a gaussian noise).
Main component
[[ 0.52523]
[-0.52523]
[ 0.26261]
[-0.26261]
[ 0.39392]
[ 0.39392]]
[ 0.52251 -0.52521 0.26266 -0.26354 0.39493 0.3959 ]
As expected, PCA did find correctly that main axis.
So, that was just side comments.
What is really what you were looking for is
ax.plot([sc1*U[3],sc2*U[3]], [sc1*U[4], sc2*U[4]], [sc1*U[5], sc2*U[5]], linewidth=3)
sc1 and sc2 being just scaling factors (here I choose it so that it scales approx like the data. Another way would have been to set ax.set_xlim, ax.set_ylim, ax.set_zlim from D.min(), D.max(), E.min(), E.max(), etc.
And then just use big values for sc1 and sc2, like
sc1=1000
sc2=-1000

How to interpolate a line between two other lines in python

Note: I asked this question before but it was closed as a duplicate, however, I, along with several others believe it was unduely closed, I explain why in an edit in my original post. So I would like to re-ask this question here again.
Does anyone know of a python library that can interpolate between two lines. For example, given the two solid lines below, I would like to produce the dashed line in the middle. In other words, I'd like to get the centreline. The input is a just two numpy arrays of coordinates with size N x 2 and M x 2 respectively.
Furthermore, I'd like to know if someone has written a function for this in some optimized python library. Although optimization isn't exactly a necessary.
Here is an example of two lines that I might have, you can assume they do not overlap with each other and an x/y can have multiple y/x coordinates.
array([[ 1233.87375018, 1230.07095987],
[ 1237.63559365, 1253.90749041],
[ 1240.87500801, 1264.43925132],
[ 1245.30875975, 1274.63795396],
[ 1256.1449357 , 1294.48254424],
[ 1264.33600095, 1304.47893299],
[ 1273.38192911, 1313.71468591],
[ 1283.12411536, 1322.35942538],
[ 1293.2559388 , 1330.55873344],
[ 1309.4817002 , 1342.53074698],
[ 1325.7074616 , 1354.50276051],
[ 1341.93322301, 1366.47477405],
[ 1358.15898441, 1378.44678759],
[ 1394.38474581, 1390.41880113]])
array([[ 1152.27115094, 1281.52899302],
[ 1155.53345506, 1295.30515742],
[ 1163.56506781, 1318.41642169],
[ 1168.03497425, 1330.03181319],
[ 1173.26135672, 1341.30559949],
[ 1184.07110925, 1356.54121651],
[ 1194.88086178, 1371.77683353],
[ 1202.58908737, 1381.41765447],
[ 1210.72465255, 1390.65097106],
[ 1227.81309742, 1403.2904646 ],
[ 1244.90154229, 1415.92995815],
[ 1261.98998716, 1428.56945169],
[ 1275.89219696, 1438.21626352],
[ 1289.79440676, 1447.86307535],
[ 1303.69661656, 1457.50988719],
[ 1323.80994319, 1470.41028655],
[ 1343.92326983, 1488.31068591],
[ 1354.31738934, 1499.33260989],
[ 1374.48879779, 1516.93734053],
[ 1394.66020624, 1534.54207116]])
Visualizing this we have:
So my attempt at this has been using the skeletonize function in the skimage.morphology library by first rasterizing the coordinates into a filled in polygon. However, I get branching at the ends like this:
First of all, pardon the overkill; I had fun with your question. If the description is too long, feel free to skip to the bottom, I defined a function that does everything I describe.
Your problem would be relatively straightforward if your arrays were the same length. In that case, all you would have to do is find the average between the corresponding x values in each array, and the corresponding y values in each array.
So what we can do is create arrays of the same length, that are more or less good estimates of your original arrays. We can do this by fitting a polynomial to the arrays you have. As noted in comments and other answers, the midline of your original arrays is not specifically defined, so a good estimate should fulfill your needs.
Note: In all of these examples, I've gone ahead and named the two arrays that you posted a1 and a2.
Step one: Create new arrays that estimate your old lines
Looking at the data you posted:
These aren't particularly complicated functions, it looks like a 3rd degree polynomial would fit them pretty well. We can create those using numpy:
import numpy as np
# Find the range of x values in a1
min_a1_x, max_a1_x = min(a1[:,0]), max(a1[:,0])
# Create an evenly spaced array that ranges from the minimum to the maximum
# I used 100 elements, but you can use more or fewer.
# This will be used as your new x coordinates
new_a1_x = np.linspace(min_a1_x, max_a1_x, 100)
# Fit a 3rd degree polynomial to your data
a1_coefs = np.polyfit(a1[:,0],a1[:,1], 3)
# Get your new y coordinates from the coefficients of the above polynomial
new_a1_y = np.polyval(a1_coefs, new_a1_x)
# Repeat for array 2:
min_a2_x, max_a2_x = min(a2[:,0]), max(a2[:,0])
new_a2_x = np.linspace(min_a2_x, max_a2_x, 100)
a2_coefs = np.polyfit(a2[:,0],a2[:,1], 3)
new_a2_y = np.polyval(a2_coefs, new_a2_x)
The result:
That's not bad so bad! If you have more complicated functions, you'll have to fit a higher degree polynomial, or find some other adequate function to fit to your data.
Now, you've got two sets of arrays of the same length (I chose a length of 100, you can do more or less depending on how smooth you want your midpoint line to be). These sets represent the x and y coordinates of the estimates of your original arrays. In the example above, I named these new_a1_x, new_a1_y, new_a2_x and new_a2_y.
Step two: calculate the average between each x and each y in your new arrays
Then, we want to find the average x and average y value for each of our estimate arrays. Just use np.mean:
midx = [np.mean([new_a1_x[i], new_a2_x[i]]) for i in range(100)]
midy = [np.mean([new_a1_y[i], new_a2_y[i]]) for i in range(100)]
midx and midy now represent the midpoint between our 2 estimate arrays. Now, just plot your original (not estimate) arrays, alongside your midpoint array:
plt.plot(a1[:,0], a1[:,1],c='black')
plt.plot(a2[:,0], a2[:,1],c='black')
plt.plot(midx, midy, '--', c='black')
plt.show()
And voilà:
This method still works with more complex, noisy data (but you have to fit the function thoughtfully):
As a function:
I've put the above code in a function, so you can use it easily. It returns an array of your estimated midpoints, in the format you had your original arrays in.
The arguments: a1 and a2 are your 2 input arrays, poly_deg is the degree polynomial you want to fit, n_points is the number of points you want in your midpoint array, and plot is a boolean, whether you want to plot it or not.
import matplotlib.pyplot as plt
import numpy as np
def interpolate(a1, a2, poly_deg=3, n_points=100, plot=True):
min_a1_x, max_a1_x = min(a1[:,0]), max(a1[:,0])
new_a1_x = np.linspace(min_a1_x, max_a1_x, n_points)
a1_coefs = np.polyfit(a1[:,0],a1[:,1], poly_deg)
new_a1_y = np.polyval(a1_coefs, new_a1_x)
min_a2_x, max_a2_x = min(a2[:,0]), max(a2[:,0])
new_a2_x = np.linspace(min_a2_x, max_a2_x, n_points)
a2_coefs = np.polyfit(a2[:,0],a2[:,1], poly_deg)
new_a2_y = np.polyval(a2_coefs, new_a2_x)
midx = [np.mean([new_a1_x[i], new_a2_x[i]]) for i in range(n_points)]
midy = [np.mean([new_a1_y[i], new_a2_y[i]]) for i in range(n_points)]
if plot:
plt.plot(a1[:,0], a1[:,1],c='black')
plt.plot(a2[:,0], a2[:,1],c='black')
plt.plot(midx, midy, '--', c='black')
plt.show()
return np.array([[x, y] for x, y in zip(midx, midy)])
[EDIT]:
I was thinking back on this question, and I overlooked a simpler way to do this, by "densifying" both arrays to the same number of points using np.interp. This method follows the same basic idea as the line-fitting method above, but instead of approximating lines using polyfit / polyval, it just densifies:
min_a1_x, max_a1_x = min(a1[:,0]), max(a1[:,0])
min_a2_x, max_a2_x = min(a2[:,0]), max(a2[:,0])
new_a1_x = np.linspace(min_a1_x, max_a1_x, 100)
new_a2_x = np.linspace(min_a2_x, max_a2_x, 100)
new_a1_y = np.interp(new_a1_x, a1[:,0], a1[:,1])
new_a2_y = np.interp(new_a2_x, a2[:,0], a2[:,1])
midx = [np.mean([new_a1_x[i], new_a2_x[i]]) for i in range(100)]
midy = [np.mean([new_a1_y[i], new_a2_y[i]]) for i in range(100)]
plt.plot(a1[:,0], a1[:,1],c='black')
plt.plot(a2[:,0], a2[:,1],c='black')
plt.plot(midx, midy, '--', c='black')
plt.show()
The "line between two lines" is not so well defined. You can obtain a decent though simple solution by triangulating between the two curves (you can triangulate by progressing from vertex to vertex, choosing the diagonals that produce the less skewed triangle).
Then the interpolated curve joins the middles of the sides.
I work with rivers, so this is a common problem. One of my solutions is exactly like the one you showed in your question--i.e. skeletonize the blob. You see that the boundaries have problems, so what I've done that seems to work well is to simply mirror the boundaries. For this approach to work, the blob must not intersect the corners of the image.
You can find my implementation in RivGraph; this particular algorithm is in rivers/river_utils.py called "mask_to_centerline".
Here's an example output showing how the ends of the centerline extend to the desired edge of the object:
sacuL's solution almost worked for me, but I needed to aggregate more than just two curves.
Here is my generalization for sacuL's solution:
def interp(*axis_list):
min_max_xs = [(min(axis[:,0]), max(axis[:,0])) for axis in axis_list]
new_axis_xs = [np.linspace(min_x, max_x, 100) for min_x, max_x in min_max_xs]
new_axis_ys = [np.interp(new_x_axis, axis[:,0], axis[:,1]) for axis, new_x_axis in zip(axis_list, new_axis_xs)]
midx = [np.mean([new_axis_xs[axis_idx][i] for axis_idx in range(len(axis_list))]) for i in range(100)]
midy = [np.mean([new_axis_ys[axis_idx][i] for axis_idx in range(len(axis_list))]) for i in range(100)]
for axis in axis_list:
plt.plot(axis[:,0], axis[:,1],c='black')
plt.plot(midx, midy, '--', c='black')
plt.show()
If we now run an example:
a1 = np.array([[x, x**2+5*(x%4)] for x in range(10)])
a2 = np.array([[x-0.5, x**2+6*(x%3)] for x in range(10)])
a3 = np.array([[x+0.2, x**2+7*(x%2)] for x in range(10)])
interp(a1, a2, a3)
we get the plot:

How to create an SVM with multiple features for classification?

I am writing a piece of code to identify different 2D shapes using opencv. I get 4 sets of data from each image of a 2D shape and these are stored in the multidimensional array featureVectors.
I am trying to write an svm/svc that takes into account all 4 features obtained from the image. I have been able to make it work with just 2 features but when i try all 4 my graph comes out looking like this.
My Graph which is incorrect
My values for featureVectors are:
[[ 4.00000000e+00 1.74371349e-03 6.49705560e-01 9.07957236e+01]
[ 4.00000000e+00 4.60937436e-02 1.97642179e-01 9.02041472e+01]
[ 1.00000000e+00 1.18553450e-03 3.03491372e-01 6.03489082e+01]
[ 1.00000000e+00 1.54552898e-02 8.38091425e-01 1.09021207e+02]
[ 3.00000000e+00 1.69961646e-02 4.13691915e+01 1.36838300e+02]]
And my Labels are:
[[2]
[2]
[0]
[0]
[1]]
Here is my code for the SVM:
#Saving featureVectors to a csv file
values1 = featureVectors
header1 = ["Number of Sides", "Standard Deviation of Number of Sides/Perimeter",
"Standard Deviation of the Angles", "Largest Angle"]
my_df = pd.DataFrame(featureVectors)
my_df.to_csv('featureVectors.csv', index=True, header=header1)
#Saving labels to a csv file
values2 = labels
header2 = ["Label"]
my_df = pd.DataFrame(labels)
my_df.to_csv('labels.csv', index=True, header=header2)
#Writing the SVM
def Build_Data_Set(features = header1, features1 = header2):
data_df = pd.DataFrame.from_csv("featureVectors.csv")
#data_df = data_df[:250]
X = np.array(data_df[features].values)
data_df2 = pd.DataFrame.from_csv("labels.csv")
y = np.array(data_df2[features1].values)
#print(X)
#print(y)
return X,y
def Analysis():
X,y = Build_Data_Set()
clf = svm.SVC(kernel = 'linear', C = 1.0)
clf.fit(X, y)
w = clf.coef_[0]
a = -w[0] / w[1]
xx = np.linspace(0,5)
yy = np.linspace(0,185)
h0 = plt.plot(xx,yy, "k-", label="non weighted")
plt.scatter(X[:, 0],X[:, 1],c=y)
plt.ylabel("Maximum Angle (Degrees)")
plt.xlabel("Number Of Sides")
plt.title('Shapes')
plt.legend()
plt.show()
Analysis()
I have only used 5 data sets(shapes) so far because I knew it wasn't working correctly.
The SVM part of your code is actually correct. The plotting part around it is not, and given the code I'll try to give you some pointers.
First of all:
another example I found(i cant find the link again) said to do that
Copying code without understanding it will probably cause more problems than it solves. Given your code, I'm assuming you used this example as a starter.
plt.scatter(X[:, 0],X[:, 1],c=y)
In the sk-learn example, this snippet is used to plot data points, coloring them according to their label. This works because in the example we're dealing with 2-dimensional data, so this is fine. The data you're dealing with is 4-dimensional, so you're actually just plotting the first two dimensions.
plt.scatter(X[:, 0], y, c=y)
on the other hand makes no sense.
xx = np.linspace(0,5)
yy = np.linspace(0,185)
h0 = plt.plot(xx,yy, "k-", label="non weighted")
Your decision boundary has actually nothing to do with the actual decision boundary. It's just a plot of y over x of your coordinate system.
(In addition to that, you're dealing with multi class data, so you'll have as much decision boundaries as you have classes.)
Now your actual problem is data dimensionality. You're trying to plot 4-dimensional data in a 2d plot, which simply won't work.
A possible approach would be to perform dimensionality reduction to map your 4d data into a lower dimensional space, so if you want to, I'd suggest you reading e.g. the excellent sklearn documentation for an introduction to SVMs and in addition something about dimensionality reduction.

NumPy or SciPy to calculate weighted median

I'm trying to automate a process that JMP does (Analyze->Distribution, entering column A as the "Y value", using subsequent columns as the "weight" value). In JMP you have to do this one column at a time - I'd like to use Python to loop through all of the columns and create an array showing, say, the median of each column.
For example, if the mass array is [0, 10, 20, 30], and the weight array for column 1 is [30, 191, 9, 0], the weighted median of the mass array should be 10. However, I'm not sure how to arrive at this answer.
So far I've
imported the csv showing the weights as an array, masking values of 0, and
created an array of the "Y value" the same shape and size as the weights array (113x32). I'm not entirely sure I need to do this, but thought it would be easier than a for loop for the purpose of weighting.
I'm not sure exactly where to go from here. Basically the "Y value" is a range of masses, and all of the columns in the array represent the number of data points found for each mass. I need to find the median mass, based on the frequency with which they were reported.
I'm not an expert in Python or statistics, so if I've omitted any details that would be useful let me know!
Update: here's some code for what I've done so far:
#Boilerplate & Import files
import csv
import scipy as sp
from scipy import stats
from scipy.stats import norm
import numpy as np
from numpy import genfromtxt
import pandas as pd
import matplotlib.pyplot as plt
inputFile = '/Users/cl/prov.csv'
origArray = genfromtxt(inputFile, delimiter = ",")
nArray = np.array(origArray)
dimensions = nArray.shape
shape = np.asarray(dimensions)
#Mask values ==0
maTest = np.ma.masked_equal(nArray,0)
#Create array of masses the same shape as the weights (nArray)
fieldLength = shape[0]
rowLength = shape[1]
for i in range (rowLength):
createArr = np.arange(0, fieldLength*10, 10)
nCreateArr = np.array(createArr)
massArr.append(nCreateArr)
nCreateArr = np.array(massArr)
nmassArr = nCreateArr.transpose()
What we can do, if i understood your problem correctly. Is to sum up the observations, dividing by 2 would give us the observation number corresponding to the median. From there we need to figure out what observation this number was.
One trick here, is to calculate the observation sums with np.cumsum. Which gives us a running cumulative sum.
Example:
np.cumsum([1,2,3,4]) -> [ 1, 3, 6, 10]
Each element is the sum of all previously elements and itself. We have 10 observations here. so the mean would be the 5th observation. (We get 5 by dividing the last element by 2).
Now looking at the cumsum result, we can easily see that that must be the observation between the second and third elements (observation 3 and 6).
So all we need to do, is figure out the index of where the median (5) will fit.
np.searchsorted does exactly what we need. It will find the index to insert an elements into an array, so that it stays sorted.
The code to do it like so:
import numpy as np
#my test data
freq_count = np.array([[30, 191, 9, 0], [10, 20, 300, 10], [10,20,30,40], [100,10,10,10], [1,1,1,100]])
c = np.cumsum(freq_count, axis=1)
indices = [np.searchsorted(row, row[-1]/2.0) for row in c]
masses = [i * 10 for i in indices] #Correct if the masses are indeed 0, 10, 20,...
#This is just for explanation.
print "median masses is:", masses
print freq_count
print np.hstack((c, c[:, -1, np.newaxis]/2.0))
Output will be:
median masses is: [10 20 20 0 30]
[[ 30 191 9 0] <- The test data
[ 10 20 300 10]
[ 10 20 30 40]
[100 10 10 10]
[ 1 1 1 100]]
[[ 30. 221. 230. 230. 115. ] <- cumsum results with median added to the end.
[ 10. 30. 330. 340. 170. ] you can see from this where they fit in.
[ 10. 30. 60. 100. 50. ]
[ 100. 110. 120. 130. 65. ]
[ 1. 2. 3. 103. 51.5]]
wquantiles is a small python package that will do exactly what you need. It just uses np.cumsum() and np.interp() under the hood.
Since this is the top hit on Google for weighted median in NumPy, I will add my minimal function to select the weighted median from two arrays without changing their contents, and with no assumptions about the order of the values (on the off-chance that anyone else comes here looking for a quick recipe for the same exact pre-conditions).
def weighted_median(values, weights):
i = np.argsort(values)
c = np.cumsum(weights[i])
return values[i[np.searchsorted(c, 0.5 * c[-1])]]
Using argsort lets us maintain the alignment between the two arrays without changing or copying their content. It should be straight-forward to extend is to an arbitrary number of arbitrary quantiles.
Update
Since it may not be fully obvious at first blush exactly how easy it is to extend to arbitrary quantiles, here is the code:
def weighted_quantiles(values, weights, quantiles=0.5):
i = np.argsort(values)
c = np.cumsum(weights[i])
return values[i[np.searchsorted(c, np.array(quantiles) * c[-1])]]
This defaults to median, but you can pass in any quantile, or a list of quantiles. The return type is equivalent to what you pass in as quantiles, with lists promoted to NumPy arrays. With enough uniformly distributed values, you can indeed approximate the input poorly:
>>> weighted_quantiles(np.random.rand(10000), np.random.rand(10000), [0.01, 0.05, 0.25, 0.50, 0.75, 0.95, 0.99])
array([0.01235101, 0.05341077, 0.25355715, 0.50678338, 0.75697424,0.94962936, 0.98980785])
>>> weighted_quantiles(np.random.rand(10000), np.random.rand(10000), 0.5)
0.5036283072043176
>>> weighted_quantiles(np.random.rand(10000), np.random.rand(10000), [0.5])
array([0.49851076])
Update 2
In small data sets where the median/quantile is not actually observed, it may be important to be able to interpolate a point between two observations. This can be fairly easily added by calculating the mid point between two number in the case where the weight mass is equally (or quantile/1-quantile) divided between them. Due to the need for a conditional, this function always returns a NumPy array, even when quantiles is a single scalar. The inputs also need to be NumPy arrays now (except quantiles that may still be a single number).
def weighted_quantiles_interpolate(values, weights, quantiles=0.5):
i = np.argsort(values)
c = np.cumsum(weights[i])
q = np.searchsorted(c, quantiles * c[-1])
return np.where(c[q]/c[-1] == quantiles, 0.5 * (values[i[q]] + values[i[q+1]]), values[i[q]])
This function will fail with arrays smaller than 2 (the original would handle non-empty arrays).
>>> weighted_quantiles_interpolate(np.array([2, 1]), np.array([1, 1]), 0.5)
array(1.5)
Note that this extension is fairly unlikely to be needed when working with actual data sets where we typically have (a) large data sets, and (b) real-values weights that make the odds of ending up exactly at a quantile edge very long, and probably due to rounding errors when it does happen. Including it for completeness nonetheless.
I ended up writing that function based on #muzzle and #maesers replies:
def weighted_quantiles(values, weights, quantiles=0.5, interpolate=False):
i = values.argsort()
sorted_weights = weights[i]
sorted_values = values[i]
Sn = sorted_weights.cumsum()
if interpolate:
Pn = (Sn - sorted_weights/2 ) / Sn[-1]
return np.interp(quantiles, Pn, sorted_values)
else:
return sorted_values[np.searchsorted(Sn, quantiles * Sn[-1])]
The difference between interpolate True and False is as follows:
weighted_quantiles(np.array([1, 2, 3, 4]), np.ones(4))
> 2
weighted_quantiles(np.array([1, 2, 3, 4]), np.ones(4), interpolate=True)
> 2.5
(there is no difference for uneven arrays such as [1, 2, 3, 4, 5])
Speed tests show it is just as performant as #maesers' function in the uninterpolated case, and it is twice as performant in the interpolated case.
Sharing some code that I got a hand with. This allows you to run stats on each column of an excel spreadsheet.
import xlrd
import sys
import csv
import numpy as np
import itertools
from itertools import chain
book = xlrd.open_workbook('/filepath/workbook.xlsx')
sh = book.sheet_by_name("Sheet1")
ofile = '/outputfilepath/workbook.csv'
masses = sh.col_values(0, start_rowx=1) # first column has mass
age = sh.row_values(0, start_colx=1) # first row has age ranges
count = 1
mass = []
for a in ages:
age.append(sh.col_values(count, start_rowx=1))
count += 1
stats = []
count = 0
for a in ages:
expanded = []
# create a tuple with the mass vector
age_mass = zip(masses, age[count])
count += 1
# replicate element[0] for element[1] times
expanded = list(list(itertools.repeat(am[0], int(am[1]))) for am in age_mass)
# separate into one big list
medianlist = [x for t in expanded for x in t]
# convert to array and mask out zeroes
npa = np.array(medianlist)
npa = np.ma.masked_equal(npa,0)
median = np.median(npa)
meanMass = np.average(npa)
maxMass = np.max(npa)
minMass = np.min(npa)
stdev = np.std(npa)
stats1 = [median, meanMass, maxMass, minMass, stdev]
print stats1
stats.append(stats1)
np.savetxt(ofile, (stats), fmt="%d")

cv2.kmeans usage in Python

I am considering to use OpenCV's Kmeans implementation since it says to be faster...
Now I am using package cv2 and function kmeans,
I can not understand the parameters' description in their reference:
Python: cv2.kmeans(data, K, criteria, attempts, flags[, bestLabels[, centers]]) → retval, bestLabels, centers
samples – Floating-point matrix of input samples, one row per sample.
clusterCount – Number of clusters to split the set by.
labels – Input/output integer array that stores the cluster indices for every sample.
criteria – The algorithm termination criteria, that is, the maximum number of iterations and/or the desired accuracy. The accuracy is specified as criteria.epsilon. As soon as each of the cluster centers moves by less than criteria.epsilon on some iteration, the algorithm stops.
attempts – Flag to specify the number of times the algorithm is executed using different initial labelings. The algorithm returns the labels that yield the best compactness (see the last function parameter).
flags –
Flag that can take the following values:
KMEANS_RANDOM_CENTERS Select random initial centers in each attempt.
KMEANS_PP_CENTERS Use kmeans++ center initialization by Arthur and Vassilvitskii [Arthur2007].
KMEANS_USE_INITIAL_LABELS During the first (and possibly the only) attempt, use the user-supplied labels instead of computing them from the initial centers. For the second and further attempts, use the random or semi-random centers. Use one of KMEANS_*_CENTERS flag to specify the exact method.
centers – Output matrix of the cluster centers, one row per each cluster center.
what is the argument flags[, bestLabels[, centers]]) mean? and what about his one: → retval, bestLabels, centers ?
Here's my code:
import cv, cv2
import scipy.io
import numpy
# read data from .mat file
mat = scipy.io.loadmat('...')
keys = mat.keys()
values = mat.viewvalues()
data_1 = mat[keys[0]]
nRows = data_1.shape[1]
nCols = data_1.shape[0]
samples = cv.CreateMat(nRows, nCols, cv.CV_32FC1)
labels = cv.CreateMat(nRows, 1, cv.CV_32SC1)
centers = cv.CreateMat(nRows, 100, cv.CV_32FC1)
#centers = numpy.
for i in range(0, nCols):
for j in range(0, nRows):
samples[j, i] = data_1[i, j]
cv2.kmeans(data_1.transpose,
100,
criteria=(cv2.TERM_CRITERIA_EPS | cv2.TERM_CRITERIA_MAX_ITER, 0.1, 10),
attempts=cv2.KMEANS_PP_CENTERS,
flags=cv2.KMEANS_PP_CENTERS,
)
And I encounter such error:
flags=cv2.KMEANS_PP_CENTERS,
TypeError: <unknown> is not a numpy array
How should I understand the parameter list and the usage of cv2.kmeans? Thanks
the documentation on this function is almost impossible to find. I wrote the following Python code in a bit of a hurry, but it works on my machine. It generates two multi-variate Gaussian Distributions with different means and then classifies them using cv2.kmeans(). You may refer to this blog post to get some idea of the parameters.
Handle imports:
import cv
import cv2
import numpy as np
import numpy.random as r
Generate some random points and shape them appropriately:
samples = cv.CreateMat(50, 2, cv.CV_32FC1)
random_points = r.multivariate_normal((100,100), np.array([[150,400],[150,150]]), size=(25))
random_points_2 = r.multivariate_normal((300,300), np.array([[150,400],[150,150]]), size=(25))
samples_list = np.append(random_points, random_points_2).reshape(50,2)
random_points_list = np.array(samples_list, np.float32)
samples = cv.fromarray(random_points_list)
Plot the points before and after classification:
blank_image = np.zeros((400,400,3))
blank_image_classified = np.zeros((400,400,3))
for point in random_points_list:
cv2.circle(blank_image, (int(point[0]),int(point[1])), 1, (0,255,0),-1)
temp, classified_points, means = cv2.kmeans(data=np.asarray(samples), K=2, bestLabels=None,
criteria=(cv2.TERM_CRITERIA_EPS | cv2.TERM_CRITERIA_MAX_ITER, 1, 10), attempts=1,
flags=cv2.KMEANS_RANDOM_CENTERS) #Let OpenCV choose random centers for the clusters
for point, allocation in zip(random_points_list, classified_points):
if allocation == 0:
color = (255,0,0)
elif allocation == 1:
color = (0,0,255)
cv2.circle(blank_image_classified, (int(point[0]),int(point[1])), 1, color,-1)
cv2.imshow("Points", blank_image)
cv2.imshow("Points Classified", blank_image_classified)
cv2.waitKey()
Here you can see the original points:
Here are the points after they have been classified:
I hope that this answer may help you, it is not a complete guide to k-means, but it will at least show you how to pass the parameters to OpenCV.
The problem here is your data_1.transpose is not a numpy array.
OpenCV 2.3.1 and higher python bindings do not take anything except numpy array as image/array parameters. so, data_1.transpose has to be a numpy array.
Generally, all the points in OpenCV are of type numpy.ndarray
eg.
array([[[100., 433.]],
[[157., 377.]],
.
.
[[147., 247.]], dtype=float32)
where each element of array is
array([[100., 433.]], dtype=float32)
and the element of that array is
array([100., 433.], dtype=float32)

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