idst — SciPy v1.15.3 Manual (original) (raw)
scipy.fft.
scipy.fft.idst(x, type=2, n=None, axis=-1, norm=None, overwrite_x=False, workers=None, orthogonalize=None)[source]#
Return the Inverse Discrete Sine Transform of an arbitrary type sequence.
Parameters:
xarray_like
The input array.
type{1, 2, 3, 4}, optional
Type of the DST (see Notes). Default type is 2.
nint, optional
Length of the transform. If n < x.shape[axis]
, x is truncated. If n > x.shape[axis]
, x is zero-padded. The default results in n = x.shape[axis]
.
axisint, optional
Axis along which the idst is computed; the default is over the last axis (i.e., axis=-1
).
norm{“backward”, “ortho”, “forward”}, optional
Normalization mode (see Notes). Default is “backward”.
overwrite_xbool, optional
If True, the contents of x can be destroyed; the default is False.
workersint, optional
Maximum number of workers to use for parallel computation. If negative, the value wraps around from os.cpu_count()
. See fft for more details.
orthogonalizebool, optional
Whether to use the orthogonalized IDST variant (see Notes). Defaults to True
when norm="ortho"
and False
otherwise.
Added in version 1.8.0.
Returns:
idstndarray of real
The transformed input array.
Notes
Warning
For type in {2, 3}
, norm="ortho"
breaks the direct correspondence with the inverse direct Fourier transform.
For norm="ortho"
both the dst and idst are scaled by the same overall factor in both directions. By default, the transform is also orthogonalized which for types 2 and 3 means the transform definition is modified to give orthogonality of the DST matrix (see dst for the full definitions).
‘The’ IDST is the IDST-II, which is the same as the normalized DST-III.
The IDST is equivalent to a normal DST except for the normalization and type. DST type 1 and 4 are their own inverse and DSTs 2 and 3 are each other’s inverses.