dpnp.blackman
- dpnp.blackman(M, device=None, usm_type=None, sycl_queue=None)[source]
Return the Blackman window.
The Blackman window is a taper formed by using the first three terms of a summation of cosines. It was designed to have close to the minimal leakage possible. It is close to optimal, only slightly worse than a Kaiser window.
For full documentation refer to
numpy.blackman
.- Parameters:
M (int) -- Number of points in the output window. If zero or less, an empty array is returned.
device ({None, string, SyclDevice, SyclQueue, Device}, optional) --
An array API concept of device where the output array is created. device can be
None
, a oneAPI filter selector string, an instance ofdpctl.SyclDevice
corresponding to a non-partitioned SYCL device, an instance ofdpctl.SyclQueue
, or adpctl.tensor.Device
object returned bydpnp.ndarray.device
.Default:
None
.usm_type ({None, "device", "shared", "host"}, optional) --
The type of SYCL USM allocation for the output array.
Default:
None
.sycl_queue ({None, SyclQueue}, optional) --
A SYCL queue to use for output array allocation and copying. The sycl_queue can be passed as
None
(the default), which means to get the SYCL queue from device keyword if present or to use a default queue.Default:
None
.
- Returns:
out -- The window, with the maximum value normalized to one (the value one appears only if the number of samples is odd).
- Return type:
dpnp.ndarray of shape (M,)
See also
dpnp.bartlett
Return the Bartlett window.
dpnp.hamming
Return the Hamming window.
dpnp.hanning
Return the Hanning window.
dpnp.kaiser
Return the Kaiser window.
Notes
The Blackman window is defined as
\[w(n) = 0.42 - 0.5\cos\left(\frac{2\pi{n}}{M-1}\right) + 0.08\cos\left(\frac{4\pi{n}}{M-1}\right) \qquad 0 \leq n \leq M-1\]Examples
>>> import dpnp as np >>> np.blackman(12) array([-1.38777878e-17, 3.26064346e-02, 1.59903635e-01, 4.14397981e-01, 7.36045180e-01, 9.67046769e-01, 9.67046769e-01, 7.36045180e-01, 4.14397981e-01, 1.59903635e-01, 3.26064346e-02, -1.38777878e-17])
Creating the output array on a different device or with a specified usm_type:
>>> x = np.blackman(3) # default case >>> x, x.device, x.usm_type (array([-1.38777878e-17, 1.00000000e+00, -1.38777878e-17]), Device(level_zero:gpu:0), 'device')
>>> y = np.blackman(3, device="cpu") >>> y, y.device, y.usm_type (array([-1.38777878e-17, 1.00000000e+00, -1.38777878e-17]), Device(opencl:cpu:0), 'device')
>>> z = np.blackman(3, usm_type="host") >>> z, z.device, z.usm_type (array([-1.38777878e-17, 1.00000000e+00, -1.38777878e-17]), Device(level_zero:gpu:0), 'host')