Minor corrections

This commit is contained in:
emmanuelle
2014-12-15 21:45:02 +01:00
parent 7cb3071781
commit 1a536905f1
@@ -108,7 +108,7 @@ values over a larger range.
A first class of methods compute a nonlinear function of the intensity,
that is independent of the pixel values of a specific image. Such methods
are often used for correcting a known non-linearity of sensors, or
receptors such as the human eye. A well-known example is the `Gamma
receptors such as the human eye. A well-known example is `Gamma
correction <http://en.wikipedia.org/wiki/Gamma_correction>`_, implemented
in :func:`adjust_gamma`.
@@ -120,14 +120,14 @@ the image. The histogram of pixel values is computed with
>>> exposure.histogram(image)
(array([3, 0, 1]), array([1, 2, 3]))
that returns the number of pixels for each value bin, and the centers of
the bins. The behavior of :func:`histogram` is therefore slightly
different from the one of :func:`np.histogram`, which returns the
boundaries of the bins.
:func:`histogram` returns the number of pixels for each value bin, and
the centers of the bins. The behavior of :func:`histogram` is therefore
slightly different from the one of :func:`np.histogram`, which returns
the boundaries of the bins.
The simplest contrast enhancement :func:`rescale_intensity` consists in
stretching pixel values to the whole allowed range, using a linear
transformation.::
transformation::
>>> from skimage import exposure
>>> text = data.text()
@@ -141,14 +141,14 @@ Even if an image uses the whole value range, sometimes there is very
little weight at the ends of the value range. In such a case, clipping
pixel values using percentiles of the image improves the contrast (at the
expense of some loss of information, because some pixels are saturated by
this operation).::
this operation)::
>>> moon = data.moon()
>>> v_min, v_max = np.percentile(moon, (0.2, 99.8))
>>> v_min, v_max
(10.0, 186.0)
>>> better_contrast = exposure.rescale_intensity(moon,
... in_range=(v_min, v_max))
>>> better_contrast = exposure.rescale_intensity(
... moon, in_range=(v_min, v_max))
The function :func:`equalize_hist` maps the cumulative distribution
function (cdf) of pixel values onto a linear cdf, ensuring that all parts