polarcbo.noise.normal_noise
- class polarcbo.noise.normal_noise(tau=0.1)[source]
Bases:
noise_model
Model for normal distributed noise
This class implements a normal noise model with zero mean and covariance matrix \(\tau I_d\) where \(\tau\) is a parameter of the class. Given the vector \(x_i - \mathsf{m}(x_i)\), the noise vector is computed as
\[n_i = \tau \sqrt{\|x_i - \mathsf{m}(x_i)\|_2}\ \mathcal{N}(0,1)\]- Parameters:
tau (float, optional) – The parameter \(\tau\) of the noise model. The default is 0.1.
Examples
>>> import numpy as np >>> from polarcbo.noise import normal_noise >>> m_diff = np.array([[2,3], [4,5], [1,4.]]) >>> noise = normal_noise(tau=0.1) >>> noise(m_diff) array([[-2.4309445 , 1.34997294], [-1.08502177, 0.24030935], [ 0.1794014 , -1.09228077]])
- __call__(m_diff)[source]
Call method for classes that inherit from
noise_model
- Parameters:
m_diff (array_like, shape (J, d)) – For a system of \(J\) particles, the i-th row of this array
m_diff[i,:]
represents the vector \(x_i - \mathsf{m}(x_i)\) where \(x\in\R^d\) denotes the position of the i-th particle and \(\mathsf{m}(x_i)\) its weighted mean.- Returns:
n – The random vector that is computed by the repspective noise model.
- Return type:
array_like, shape (J,d)