mirror of
https://github.com/wassname/scikit-image.git
synced 2026-07-28 11:25:42 +08:00
DOC: Revert to old
This commit is contained in:
@@ -213,7 +213,7 @@ def wiener(data, impulse_response=None, filter_params={}, K=0.25,
|
||||
data : (M,N) ndarray
|
||||
Input data.
|
||||
K : float or (M,N) ndarray
|
||||
Ratio between power spectrum of noise and undergraded
|
||||
Ratio between power spectrum of noise and undegraded
|
||||
image.
|
||||
impulse_response : callable `f(r, c, **filter_params)`
|
||||
Impulse response of the filter. See LPIFilter2D.__init__.
|
||||
|
||||
@@ -29,7 +29,7 @@ def frt2(a):
|
||||
|
||||
Notes
|
||||
-----
|
||||
The FRT has a unique inverse if n is prime. [FRT]
|
||||
The FRT has a unique inverse iff n is prime. [FRT]
|
||||
The idea for this algorithm is due to Vlad Negnevitski.
|
||||
|
||||
Examples
|
||||
@@ -88,7 +88,7 @@ def ifrt2(a):
|
||||
|
||||
Notes
|
||||
-----
|
||||
The FRT has a unique inverse if n is prime.
|
||||
The FRT has a unique inverse iff n is prime.
|
||||
See [1]_ for an overview.
|
||||
The idea for this algorithm is due to Vlad Negnevitski.
|
||||
|
||||
|
||||
Reference in New Issue
Block a user