I am trying to compute the tensor rank aka CP rank (https://en.wikipedia.org/wiki/Tensor_rank_decomposition#Tensor_rank) for a specific sparse tensor that is 8 x 8 x 8.
I am new to Tensorly and have only just installed. After reading the documentation on the parafac function (http://tensorly.org/stable/modules/generated/tensorly.decomposition.parafac.html), it seems I need to specify a particular tensor rank in order to find a tensor rank decomposition of that particular rank. How can one compute the tensor rank using this software? Is there perhaps a different function which yields the tensor rank when given a specific tensor?
Determining the rank of a tensor is, in general, NP-hard. Typically, the CP decomposition takes a tensor and the desired rank as input.
If you use the latest version of TensorLy from Github, you can set rank='same' or any floating value between 0 and 1 to set the rank so as to keep either the same number of parameters as the original tensor, or a fraction of the parameters.
Related
tensor3 = tf.Variable([["hi", "hello","yo"],["hi","hello","hi"],["yo","whats","up"]], tf.string)
My understanding is this should be a rank 3 tensor but turns out its a rank 2 tensor. I'm new to machine learning so I'm not sure if I'm missing something here.
A tensor rank is the number of its dimensions, not the maximal size along a dimension.
C_ijkl would be a rank 4 tensor (see e.g. tensor formulation of Hooke's law). Yours has only 2 dimensions. You must be confusing it with a matrix rank. Straight from TF documentation:
Note: The rank of a tensor is not the same as the rank of a matrix.
The rank of a tensor is the number of indices required to uniquely
select each element of the tensor. Rank is also known as "order",
"degree", or "ndims."
When I implement target in in-batch multi-class classification on PyTorch (version 1.6), I have the following problem.
I got a variable D <class 'torch.Tensor'> （related to label description) of size as torch.Size([16, 128]), i.e. [data_size,token_id_size].
The original idea was to generate a target tensor of torch.Size([16]), each value is unique, corresponding to the rows in D, from 0 to 16 as [0,1,2,...,15], for in-batch multi-class classification.
This can be done using target = torch.LongTensor(torch.arange(16))
But there maybe repeated, non-unique rows in D, so I would like that the same, unique row in D has the its unique index in target. For example D has row0, row1, row8 the same token_ids or vector and the other rows are all different from each other, then target should be [0,0,2,3,4,5,6,0,8,9,10,11,12,13,14,15] or [0,0,1,2,3,4,5,0,6,7,8,9,10,11,12,13], wher the former has still indexes 0-15 (but no 1 and 7) and the latter has indexes of all in 0-13.
How can I implement this?
See answers of the simplified question (i) generate 1D tensor as unique index of rows of an 2D tensor and (ii) generate 1D tensor as unique index of rows of an 2D tensor (keeping the order and the original index), which address the problem of this question.
But these seem not useful to improve the contrastive multi-class classification.
I've been playing with some SVM implementations and I am wondering - what is the best way to normalize feature values to fit into one range? (from 0 to 1)
Let's suppose I have 3 features with values in ranges of:
3 - 5.
0.02 - 0.05
10-15.
How do I convert all of those values into range of [0,1]?
What If, during training, the highest value of feature number 1 that I will encounter is 5 and after I begin to use my model on much bigger datasets, I will stumble upon values as high as 7? Then in the converted range, it would exceed 1...
How do I normalize values during training to account for the possibility of "values in the wild" exceeding the highest(or lowest) values the model "seen" during training? How will the model react to that and how I make it work properly when that happens?
Besides scaling to unit length method provided by Tim, standardization is most often used in machine learning field. Please note that when your test data comes, it makes more sense to use the mean value and standard deviation from your training samples to do this scaling. If you have a very large amount of training data, it is safe to assume they obey the normal distribution, so the possibility that new test data is out-of-range won't be that high. Refer to this post for more details.
You normalise a vector by converting it to a unit vector. This trains the SVM on the relative values of the features, not the magnitudes. The normalisation algorithm will work on vectors with any values.
To convert to a unit vector, divide each value by the length of the vector. For example, a vector of [4 0.02 12] has a length of 12.6491. The normalised vector is then [4/12.6491 0.02/12.6491 12/12.6491] = [0.316 0.0016 0.949].
If "in the wild" we encounter a vector of [400 2 1200] it will normalise to the same unit vector as above. The magnitudes of the features is "cancelled out" by the normalisation and we are left with relative values between 0 and 1.
I developed a image processing program that identifies what a number is given an image of numbers. Each image was 27x27 pixels = 729 pixels. I take each R, G and B value which means I have 2187 variables from each image (+1 for the intercept = total of 2188).
I used the below gradient descent formula:
Repeat {
θj = θj−α/m∑(hθ(x)−y)xj
}
Where θj is the coefficient on variable j; α is the learning rate; hθ(x) is the hypothesis; y is real value and xj is the value of variable j. m is the number of training sets. hθ(x), y are for each training set (i.e. that's what the summation sign is for). Further the hypothesis is defined as:
hθ(x) = 1/(1+ e^-z)
z= θo + θ1X1+θ2X2 +θ3X3...θnXn
With this, and 3000 training images, I was able to train my program in just over an hour and when tested on a cross validation set, it was able to identify the correct image ~ 67% of the time.
I wanted to improve that so I decided to attempt a polynomial of degree 2.
However the number of variables jumps from 2188 to 2,394,766 per image! It takes me an hour just to do 1 step of gradient descent.
So my question is, how is this vast number of variables handled in machine learning? On the one hand, I don't have enough space to even hold that many variables for each training set. On the other hand, I am currently storing 2188 variables per training sample, but I have to perform O(n^2) just to get the values of each variable multiplied by another variable (i.e. the polynomial to degree 2 values).
So any suggestions / advice is greatly appreciated.
try to use some dimensionality reduction first (PCA, kernel PCA, or LDA if you are classifying the images)
vectorize your gradient descent - with most math libraries or in matlab etc. it will run much faster
parallelize the algorithm and then run in on multiple CPUs (but maybe your library for multiplying vectors already supports parallel computations)
Along with Jirka-x1's answer, I would first say that this is one of the key differences in working with image data than say text data for ML: high dimensionality.
Second... this is a duplicate, see How to approach machine learning problems with high dimensional input space?
I have data set n x m where there are n observations and each observation consists of m values for m attributes. Each observation has also observed result assigned to it. m is big, too big for my task. I am trying to find a best and smallest subset of m attributes that still represents the whole dataset quite well, so that I could use only these attributes for teaching a neural network.
I want to use genetic algorithm for this. The problem is the fittness function. It should tell how well the generated model (subset of attributes) still reflects the original data. And I don't know how to evaluate certain subset of attributes against the whole set.
Of course I could use the neural network(that will later use this selected data anyway) for checking how good the subset is - the smaller the error, the better the subset. BUT, this takes a looot of time in my case and I do not want to use this solution. I am looking for some other way that would preferably operate only on the data set.
What I thought about was: having subset S (found by genetic algorithm), trim data set so that it contains values only for subset S and check how many observations in this data ser are no longer distinguishable (have same values for same attributes) while having different result values. The bigger the number is, the worse subset it is. But this seems to me like a bit too computationally exhausting.
Are there any other ways to evaluate how well a subset of attributes still represents the whole data set?
This cost function should do what you want: sum the factor loadings that correspond to the features comprising each subset.
The higher that sum, the greater the share of variability in the response variable that is explained with just those features. If i understand the OP, this cost function is a faithful translation of "represents the whole set quite well" from the OP.
Reducing to code is straightforward:
Calculate the covariance matrix of your dataset (first remove the
column that holds the response variable, i.e., probably the last
one). If your dataset is m x n (columns x rows), then this
covariance matrix will be n x n, with "1"s down the main diagonal.
Next, perform an eigenvalue decomposition on this covariance
matrix; this will give you the proportion of the total variability
in the response variable, contributed by that eigenvalue (each
eigenvalue corresponds to a feature, or column). [Note,
singular-value decomposition (SVD) is often used for this step, but
it's unnecessary--an eigenvalue decomposition is much simpler, and
always does the job as long as your matrix is square, which
covariance matrices always are].
Your genetic algorithm will, at each iteration, return a set of
candidate solutions (features subsets, in your case). The next task
in GA, or any combinatorial optimization, is to rank those candiate
solutions by their cost function score. In your case, the cost
function is a simple summation of the eigenvalue proportion for each
feature in that subset. (I guess you would want to scale/normalize
that calculation so that the higher numbers are the least fit
though.)
A sample calculation (using python + NumPy):
>>> # there are many ways to do an eigenvalue decomp, this is just one way
>>> import numpy as NP
>>> import numpy.linalg as LA
>>> # calculate covariance matrix of the data set (leaving out response variable column)
>>> C = NP.corrcoef(d3, rowvar=0)
>>> C.shape
(4, 4)
>>> C
array([[ 1. , -0.11, 0.87, 0.82],
[-0.11, 1. , -0.42, -0.36],
[ 0.87, -0.42, 1. , 0.96],
[ 0.82, -0.36, 0.96, 1. ]])
>>> # now calculate eigenvalues & eivenvectors of the covariance matrix:
>>> eva, evc = LA.eig(C)
>>> # now just get value proprtions of each eigenvalue:
>>> # first, sort the eigenvalues, highest to lowest:
>>> eva1 = NP.sort(eva)[::-1]
>>> # get value proportion of each eigenvalue:
>>> eva2 = NP.cumsum(eva1/NP.sum(eva1)) # "cumsum" is just cumulative sum
>>> title1 = "ev value proportion"
>>> print( "{0}".format("-"*len(title1)) )
-------------------
>>> for row in q :
print("{0:1d} {1:3f} {2:3f}".format(int(row[0]), row[1], row[2]))
ev value proportion
1 2.91 0.727
2 0.92 0.953
3 0.14 0.995
4 0.02 1.000
so it's the third column of values just above (one for each feature) that are summed (selectively, depending on which features are present in a given subset you are evaluating with the cost function).