where \(i\) is the imaginary unit and \(|z|\) gives the length
of the complex number \(z\). \(|z|\) in the above expression
is known as the mean resultant length.
Parameters:
samplesarray_like
Input array of angle observations. The value of a full angle is
equal to (high-low).
highfloat, optional
Upper boundary of the principal value of an angle. Default is 2*pi.
lowfloat, optional
Lower boundary of the principal value of an angle. Default is 0.
normalizeboolean, optional
If False (the default), the return value is computed from the
above formula with the input scaled by (2*pi)/(high-low) and
the output scaled (back) by (high-low)/(2*pi). If True,
the output is not scaled and is returned directly.
axisint or None, default: None
If an int, the axis of the input along which to compute the statistic.
The statistic of each axis-slice (e.g. row) of the input will appear in a
corresponding element of the output.
If None, the input will be raveled before computing the statistic.
nan_policy{‘propagate’, ‘omit’, ‘raise’}
Defines how to handle input NaNs.
propagate: if a NaN is present in the axis slice (e.g. row) along
which the statistic is computed, the corresponding entry of the output
will be NaN.
omit: NaNs will be omitted when performing the calculation.
If insufficient data remains in the axis slice along which the
statistic is computed, the corresponding entry of the output will be
NaN.
raise: if a NaN is present, a ValueError will be raised.
keepdimsbool, default: False
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 array.
Returns:
circstdfloat
Circular standard deviation, optionally normalized.
In the limit of small angles, the circular standard deviation is close
to the ‘linear’ standard deviation if normalize is False.
Beginning in SciPy 1.9, np.matrix inputs (not recommended for new
code) are converted to np.ndarray before the calculation is performed. In
this case, the output will be a scalar or np.ndarray of appropriate shape
rather than a 2D np.matrix. Similarly, while masked elements of masked
arrays are ignored, the output will be a scalar or np.ndarray rather than a
masked array with mask=False.
Array API Standard Support
circstd 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.