mars.tensor.std¶

mars.tensor.
std
(a, axis=None, dtype=None, out=None, ddof=0, keepdims=None, combine_size=None)[source]¶ Compute the standard deviation along the specified axis.
Returns the standard deviation, a measure of the spread of a distribution, of the tensor elements. The standard deviation is computed for the flattened tensor by default, otherwise over the specified axis.
 Parameters
a (array_like) – Calculate the standard deviation of these values.
axis (None or int or tuple of ints, optional) –
Axis or axes along which the standard deviation is computed. The default is to compute the standard deviation of the flattened tensor.
If this is a tuple of ints, a standard deviation is performed over multiple axes, instead of a single axis or all the axes as before.
dtype (dtype, optional) – Type to use in computing the standard deviation. For tensors of integer type the default is float64, for tensors of float types it is the same as the array type.
out (Tensor, optional) – Alternative output tensor in which to place the result. It must have the same shape as the expected output but the type (of the calculated values) will be cast if necessary.
ddof (int, optional) – Means Delta Degrees of Freedom. The divisor used in calculations is
N  ddof
, whereN
represents the number of elements. By default ddof is zero.keepdims (bool, optional) –
If this is set to True, the axes which are reduced are left in the result as dimensions with size one. With this option, the result will broadcast correctly against the input tensor.
If the default value is passed, then keepdims will not be passed through to the std method of subclasses of Tensor, however any nondefault value will be. If the subclasses sum method does not implement keepdims any exceptions will be raised.
combine_size (int, optional) – The number of chunks to combine.
 Returns
standard_deviation – If out is None, return a new tensor containing the standard deviation, otherwise return a reference to the output array.
 Return type
Tensor, see dtype parameter above.
Notes
The standard deviation is the square root of the average of the squared deviations from the mean, i.e.,
std = sqrt(mean(abs(x  x.mean())**2))
.The average squared deviation is normally calculated as
x.sum() / N
, whereN = len(x)
. If, however, ddof is specified, the divisorN  ddof
is used instead. In standard statistical practice,ddof=1
provides an unbiased estimator of the variance of the infinite population.ddof=0
provides a maximum likelihood estimate of the variance for normally distributed variables. The standard deviation computed in this function is the square root of the estimated variance, so even withddof=1
, it will not be an unbiased estimate of the standard deviation per se.Note that, for complex numbers, std takes the absolute value before squaring, so that the result is always real and nonnegative.
For floatingpoint input, the std is computed using the same precision the input has. Depending on the input data, this can cause the results to be inaccurate, especially for float32 (see example below). Specifying a higheraccuracy accumulator using the dtype keyword can alleviate this issue.
Examples
>>> import mars.tensor as mt
>>> a = mt.array([[1, 2], [3, 4]]) >>> mt.std(a).execute() 1.1180339887498949 >>> mt.std(a, axis=0).execute() array([ 1., 1.]) >>> mt.std(a, axis=1).execute() array([ 0.5, 0.5])
In single precision, std() can be inaccurate:
>>> a = mt.zeros((2, 512*512), dtype=mt.float32) >>> a[0, :] = 1.0 >>> a[1, :] = 0.1 >>> mt.std(a).execute() 0.45000005
Computing the standard deviation in float64 is more accurate:
>>> mt.std(a, dtype=mt.float64).execute() 0.44999999925494177