Merge pull request #148 from amueller/doc_error_message

DOC: Some sphinx and rst fixes.
This commit is contained in:
Stefan van der Walt
2012-02-21 09:58:34 -08:00
10 changed files with 42 additions and 44 deletions
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@@ -46,7 +46,7 @@ Test coverage
Tests for a module should ideally cover all code in that module,
i.e. statement coverage should be at 100%.
To measure the test coverage, install
To measure the test coverage, install
`coverage.py <http://nedbatchelder.com/code/coverage/>`__
(using ``easy_install coverage``) and then run::
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@@ -32,10 +32,10 @@ is not rocket science.
.. [4] http://en.wikipedia.org/wiki/K-means_clustering
.. [5] http://en.wikipedia.org/wiki/Lateral_geniculate_nucleus
.. [6] D. H. Hubel and T. N. Wiesel Receptive Fields of Single Neurones
in the Cat's Striate Cortex J. Physiol. pp. 574-591 (148) 1959
in the Cat's Striate Cortex J. Physiol. pp. 574-591 (148) 1959
.. [7] D. H. Hubel and T. N. Wiesel Receptive Fields, Binocular
Interaction and Functional Architecture in the Cat's Visual Cortex J.
Physiol. 160 pp. 106-154 1962
Interaction and Functional Architecture in the Cat's Visual Cortex J.
Physiol. 160 pp. 106-154 1962
"""
import numpy as np
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@@ -1,8 +1,8 @@
.. _forking:
==========================================
============================================
Making your own copy (fork) of scikits-image
==========================================
============================================
You need to do this only once. The instructions here are very similar
to the instructions at http://help.github.com/forking/ |emdash| please see
@@ -10,7 +10,7 @@ that page for more detail. We're repeating some of it here just to give the
specifics for the scikits-image_ project, and to suggest some default names.
Set up and configure a github account
=====================================
======================================
If you don't have a github account, go to the github page, and make one.
@@ -18,7 +18,7 @@ You then need to configure your account to allow write access |emdash| see
the ``Generating SSH keys`` help on `github help`_.
Create your own forked copy of scikits-image_
===========================================
=============================================
#. Log into your github account.
#. Go to the scikits-image_ github home at `scikits-image github`_.
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@@ -1,7 +1,7 @@
.. _using-git:
Working with *scikits-image* source code
======================================
========================================
Contents:
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@@ -127,9 +127,9 @@ def greycoprops(P, prop='contrast'):
- 'homogeneity': :math:`\\sum_{i,j=0}^{levels-1}\\frac{P_{i,j}}{1+(i-j)^2}`
- 'ASM': :math:`\\sum_{i,j=0}^{levels-1} P_{i,j}^2`
- 'energy': :math:`\\sqrt{ASM}`
- 'correlation':
.. math:: \\sum_{i,j=0}^{levels-1} P_{i,j}\\left[\\frac{(i-\\mu_i) \\
(j-\\mu_j)}{\\sqrt{(\\sigma_i^2)(\\sigma_j^2)}}\\right]
- 'correlation':
.. math:: \\sum_{i,j=0}^{levels-1} P_{i,j}\\left[\\frac{(i-\\mu_i) \\
(j-\\mu_j)}{\\sqrt{(\\sigma_i^2)(\\sigma_j^2)}}\\right]
Parameters
@@ -140,6 +140,7 @@ def greycoprops(P, prop='contrast'):
`P[i,j,d,theta]` is the number of times that grey-level j
occurs at a distance d and at an angle theta from
grey-level i.
prop : {'contrast', 'dissimilarity', 'homogeneity', 'energy', \
'correlation', 'ASM'}, optional
The property of the GLCM to compute. The default is 'contrast'.
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@@ -7,11 +7,12 @@ def hog(image, orientations=9, pixels_per_cell=(8, 8),
"""Extract Histogram of Oriented Gradients (HOG) for a given image.
Compute a Histogram of Oriented Gradients (HOG) by
1) (optional) global image normalisation
2) computing the gradient image in x and y
3) computing gradient histograms
3) normalising across blocks
4) flattening into a feature vector
1. (optional) global image normalisation
2. computing the gradient image in x and y
3. computing gradient histograms
4. normalising across blocks
5. flattening into a feature vector
Parameters
----------
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@@ -21,15 +21,6 @@ class MultiImage(object):
Whether to conserve memory by only caching a single frame. Default is
True.
Attributes
----------
filename : str
The complete path to the image file.
conserve_memory : bool
Whether memory is conserved by only caching a single frame.
numframes : int
The number of frames in the image.
Notes
-----
If ``conserve_memory=True`` the memory footprint can be reduced, however
@@ -182,22 +182,22 @@ def random_walker(data, labels, beta=130, mode='bf', tol=1.e-3, copy=True):
Mode for solving the linear system in the random walker
algorithm.
- 'bf' (brute force, default): an LU factorization of the
Laplacian is computed. This is fast for small images (<1024x1024),
but very slow (due to the memory cost) and memory-consuming for
big images (in 3-D for example).
- 'bf' (brute force, default): an LU factorization of the Laplacian is
computed. This is fast for small images (<1024x1024), but very slow
(due to the memory cost) and memory-consuming for big images (in 3-D
for example).
- 'cg' (conjugate gradient): the linear system is solved
iteratively using the Conjugate Gradient method from
scipy.sparse.linalg. This is less memory-consuming than the
brute force method for large images, but it is quite slow.
- 'cg' (conjugate gradient): the linear system is solved iteratively
using the Conjugate Gradient method from scipy.sparse.linalg. This is
less memory-consuming than the brute force method for large images,
but it is quite slow.
- 'cg_mg' (conjugate gradient with multigrid preconditioner):
a preconditioner is computed using a multigrid solver, then
the solution is computed with the Conjugate Gradient method.
This mode requires that the pyamg module
(http://code.google.com/p/pyamg/) is installed. For images of
size > 512x512, this is the recommended (fastest) mode.
- 'cg_mg' (conjugate gradient with multigrid preconditioner): a
preconditioner is computed using a multigrid solver, then the
solution is computed with the Conjugate Gradient method. This mode
requires that the pyamg module (http://code.google.com/p/pyamg/) is
installed. For images of size > 512x512, this is the recommended
(fastest) mode.
tol : float
tolerance to achieve when solving the linear system, in
@@ -240,18 +240,20 @@ def random_walker(data, labels, beta=130, mode='bf', tol=1.e-3, copy=True):
the other coefficients are looked for). Each pixel is attributed the label
for which it has a maximal value of x. The Laplacian L of the image
is defined as:
- L_ii = d_i, the number of neighbors of pixel i (the degree of i)
- L_ij = -w_ij if i and j are adjacent pixels
The weight w_ij is a decreasing function of the norm of the local gradient.
This ensures that diffusion is easier between pixels of similar values.
When the Laplacian is decomposed into blocks of marked and unmarked pixels
When the Laplacian is decomposed into blocks of marked and unmarked pixels::
L = M B.T
B A
with first indices corresponding to marked pixels, and then to unmarked
pixels, minimizing x.T L x for one phase amount to solving
pixels, minimizing x.T L x for one phase amount to solving::
A x = - B x_m
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@@ -97,7 +97,7 @@ def ifrt2(a):
Notes
-----
The FRT has a unique inverse iff n is prime.
See [FRT] for an overview.
See [1]_ for an overview.
The idea for this algorithm is due to Vlad Negnevitski.
Examples
@@ -120,7 +120,7 @@ def ifrt2(a):
References
----------
.. [FRT] A. Kingston and I. Svalbe, "Projective transforms on periodic
.. [1] A. Kingston and I. Svalbe, "Projective transforms on periodic
discrete image arrays," in P. Hawkes (Ed), Advances in Imaging
and Electron Physics, 139 (2006)
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@@ -17,6 +17,9 @@ import numpy as np
from scipy.fftpack import fftshift, fft, ifft
from ._project import homography
__all__ = ["radon", "iradon"]
def radon(image, theta=None):
"""
Calculates the radon transform of an image given specified