bundles / scipy 1.17.1 / scipy / cluster / vq / whiten
function
scipy.cluster.vq:whiten
source: /scipy/cluster/vq.py :88
Signature
def whiten ( obs , check_finite = None ) Summary
Normalize a group of observations on a per feature basis.
Extended Summary
Before running k-means, it is beneficial to rescale each feature dimension of the observation set by its standard deviation (i.e. "whiten" it - as in "white noise" where each frequency has equal power). Each feature is divided by its standard deviation across all observations to give it unit variance.
Parameters
obs: ndarrayEach row of the array is an observation. The columns are the features seen during each observation
# f0 f1 f2 obs = [[ 1., 1., 1.], #o0 [ 2., 2., 2.], #o1 [ 3., 3., 3.], #o2 [ 4., 4., 4.]] #o3
check_finite: bool, optionalWhether to check that the input matrices contain only finite numbers. Disabling may give a performance gain, but may result in problems (crashes, non-termination) if the inputs do contain infinities or NaNs. Default: True for eager backends and False for lazy ones.
Returns
result: ndarrayContains the values in
obsscaled by the standard deviation of each column.
Notes
Array API Standard Support
whiten has experimental support for Python Array API Standard compatible backends in addition to NumPy. Please consider testing these features by setting an environment variable SCIPY_ARRAY_API=1 and providing CuPy, PyTorch, JAX, or Dask arrays as array arguments. The following combinations of backend and device (or other capability) are supported.
==================== ==================== ==================== Library CPU GPU ==================== ==================== ==================== NumPy ✅ n/a CuPy n/a ✅ PyTorch ✅ ✅ JAX ✅ ✅ Dask ✅ n/a ==================== ==================== ====================
See
dev-arrayapifor more information.
Examples
import numpy as np from scipy.cluster.vq import whiten features = np.array([[1.9, 2.3, 1.7], [1.5, 2.5, 2.2], [0.8, 0.6, 1.7,]])✓
whiten(features)
✗Aliases
-
scipy.cluster.vq.whiten