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| .. _astropy-visualization-stretchnorm: | |
| ********************************** | |
| Image stretching and normalization | |
| ********************************** | |
| The `astropy.visualization` module provides a framework for | |
| transforming values in images (and more generally any arrays), | |
| typically for the purpose of visualization. Two main types of | |
| transformations are provided: | |
| * Normalization to the [0:1] range using lower and upper limits where | |
| :math:`x` represents the values in the original image: | |
| .. math:: | |
| y = \frac{x - v_{\rm min}}{v_{\rm max} - v_{\rm min}} | |
| * *Stretching* of values in the [0:1] range to the [0:1] range using a | |
| linear or non-linear function: | |
| .. math:: | |
| z = f(y) | |
| In addition, classes are provided in order to identify lower and upper | |
| limits for a dataset based on specific algorithms (such as using | |
| percentiles). | |
| Identifying lower and upper limits, as well as re-normalizing, is | |
| described in the `Intervals and Normalization`_ section, while | |
| stretching is described in the `Stretching`_ section. | |
| Intervals and Normalization | |
| =========================== | |
| Several classes are provided for determining intervals and for | |
| normalizing values in this interval to the [0:1] range. One of the | |
| simplest examples is the | |
| which determines the | |
| limits of the values based on the minimum and maximum values in the | |
| array. The class is instantiated with no arguments:: | |
| >>> from astropy.visualization import MinMaxInterval | |
| >>> interval = MinMaxInterval() | |
| and the limits can be determined by calling the | |
| method, which | |
| takes the array of values:: | |
| >>> interval.get_limits([1, 3, 4, 5, 6]) | |
| (1, 6) | |
| The ``interval`` instance can also be called like a function to | |
| actually normalize values to the range:: | |
| >>> interval([1, 3, 4, 5, 6]) # doctest: +FLOAT_CMP | |
| array([0. , 0.4, 0.6, 0.8, 1. ]) | |
| Other interval classes include | |
| and | |
| For these, values in | |
| the array can fall outside of the limits given by the interval. A | |
| ``clip`` argument is provided to control the behavior of the | |
| normalization when values fall outside the limits:: | |
| >>> from astropy.visualization import PercentileInterval | |
| >>> interval = PercentileInterval(50.) | |
| >>> interval.get_limits([1, 3, 4, 5, 6]) | |
| (3.0, 5.0) | |
| >>> interval([1, 3, 4, 5, 6]) # default is clip=True # doctest: +FLOAT_CMP | |
| array([0. , 0. , 0.5, 1. , 1. ]) | |
| >>> interval([1, 3, 4, 5, 6], clip=False) # doctest: +FLOAT_CMP | |
| array([-1. , 0. , 0.5, 1. , 1.5]) | |
| Stretching | |
| ========== | |
| In addition to classes that can scale values to the [0:1] range, a | |
| number of classes are provided to 'stretch' the values using different | |
| functions. These map a [0:1] range onto a transformed [0:1] range. A | |
| simple example is the :class:`~astropy.visualization.SqrtStretch` | |
| class:: | |
| >>> from astropy.visualization import SqrtStretch | |
| >>> stretch = SqrtStretch() | |
| >>> stretch([0., 0.25, 0.5, 0.75, 1.]) # doctest: +FLOAT_CMP | |
| array([0. , 0.5 , 0.70710678, 0.8660254 , 1. ]) | |
| As for the intervals, values outside the [0:1] range can be treated | |
| differently depending on the ``clip`` argument. By default, output | |
| values are clipped to the [0:1] range:: | |
| >>> stretch([-1., 0., 0.5, 1., 1.5]) # doctest: +FLOAT_CMP | |
| array([0. , 0. , 0.70710678, 1. , 1. ]) | |
| but this can be disabled:: | |
| >>> stretch([-1., 0., 0.5, 1., 1.5], clip=False) # doctest: +FLOAT_CMP | |
| array([ nan, 0. , 0.70710678, 1. , 1.22474487]) | |
| .. note:: | |
| The stretch functions are similar but not always strictly | |
| identical to those used in e.g. `DS9 | |
| <http://ds9.si.edu/site/Home.html>`_ (although they should have | |
| the same behavior). The equations for the DS9 stretches can be | |
| found `here <http://ds9.si.edu/doc/ref/how.html>`_ and can be | |
| compared to the equations for our stretches provided in the | |
| `astropy.visualization` API section. The main difference between | |
| our stretches and DS9 is that we have adjusted them so that the | |
| [0:1] range always maps exactly to the [0:1] range. | |
| Combining transformations | |
| ========================= | |
| Any intervals and stretches can be chained by using the ``+`` | |
| operator, which returns a new transformation. When combining intervals | |
| and stretches, the stretch object must come before the interval | |
| object. For example, to apply normalization based on a percentile | |
| value, followed by a square root stretch, you can do:: | |
| >>> transform = SqrtStretch() + PercentileInterval(90.) | |
| >>> transform([1, 3, 4, 5, 6]) # doctest: +FLOAT_CMP | |
| array([0. , 0.60302269, 0.76870611, 0.90453403, 1. ]) | |
| As before, the combined transformation can also accept a ``clip`` | |
| argument (which is `True` by default). | |
| Matplotlib normalization | |
| ======================== | |
| Matplotlib allows a custom normalization and stretch to be used when | |
| displaying data by passing a :class:`matplotlib.colors.Normalize` | |
| object, e.g. to :meth:`~matplotlib.axes.Axes.imshow`. The | |
| `astropy.visualization` module provides an | |
| class | |
| that wraps the interval (see `Intervals and Normalization`_) and | |
| stretch (see `Stretching`_) objects into an object Matplotlib | |
| understands. | |
| The inputs to the | |
| class are | |
| the data and the interval and stretch objects: | |
| .. plot:: | |
| :include-source: | |
| :align: center | |
| import numpy as np | |
| import matplotlib.pyplot as plt | |
| from astropy.visualization import (MinMaxInterval, SqrtStretch, | |
| ImageNormalize) | |
| # Generate a test image | |
| image = np.arange(65536).reshape((256, 256)) | |
| # Create an ImageNormalize object | |
| norm = ImageNormalize(image, interval=MinMaxInterval(), | |
| stretch=SqrtStretch()) | |
| # or equivalently using positional arguments | |
| # norm = ImageNormalize(image, MinMaxInterval(), SqrtStretch()) | |
| # Display the image | |
| fig = plt.figure() | |
| ax = fig.add_subplot(1, 1, 1) | |
| im = ax.imshow(image, origin='lower', norm=norm) | |
| fig.colorbar(im) | |
| As shown above, the colorbar ticks are automatically adjusted. | |
| The input image to :class:`~astropy.visualization.mpl_normalize.ImageNormalize` | |
| is typically the one to be displayed, so there is a convenience function | |
| :func:`~astropy.visualization.mpl_normalize.imshow_norm` to ease this use case: | |
| .. plot:: | |
| :include-source: | |
| :align: center | |
| import numpy as np | |
| import matplotlib.pyplot as plt | |
| from astropy.visualization import imshow_norm, MinMaxInterval, SqrtStretch | |
| # Generate a test image | |
| image = np.arange(65536).reshape((256, 256)) | |
| # Display the exact same thing as the above plot | |
| fig = plt.figure() | |
| ax = fig.add_subplot(1, 1, 1) | |
| im, norm = imshow_norm(image, ax, origin='lower', | |
| interval=MinMaxInterval(), stretch=SqrtStretch()) | |
| fig.colorbar(im) | |
| While this is the simplest case, it is also possible for a completely different | |
| image to be used to establish the normalization (e.g. if one wants to display | |
| several images with exactly the same normalization and stretch). | |
| The inputs to the | |
| class can | |
| also be the vmin and vmax limits, which you can determine from the | |
| `Intervals and Normalization`_ classes, and the stretch object: | |
| .. plot:: | |
| :include-source: | |
| :align: center | |
| import numpy as np | |
| import matplotlib.pyplot as plt | |
| from astropy.visualization import (MinMaxInterval, SqrtStretch, | |
| ImageNormalize) | |
| # Generate a test image | |
| image = np.arange(65536).reshape((256, 256)) | |
| # Create interval object | |
| interval = MinMaxInterval() | |
| vmin, vmax = interval.get_limits(image) | |
| # Create an ImageNormalize object using a SqrtStretch object | |
| norm = ImageNormalize(vmin=vmin, vmax=vmax, stretch=SqrtStretch()) | |
| # Display the image | |
| fig = plt.figure() | |
| ax = fig.add_subplot(1, 1, 1) | |
| im = ax.imshow(image, origin='lower', norm=norm) | |
| fig.colorbar(im) | |
| Finally, we also provide a convenience | |
| function that | |
| can be useful for quick interactive analysis (it is also used by the | |
| ``fits2bitmap`` command-line script). However, it is not recommended | |
| to be used in scripted programs; it's better to use | |
| directly: | |
| .. plot:: | |
| :include-source: | |
| :align: center | |
| import numpy as np | |
| import matplotlib.pyplot as plt | |
| from astropy.visualization import simple_norm | |
| # Generate a test image | |
| image = np.arange(65536).reshape((256, 256)) | |
| # Create an ImageNormalize object | |
| norm = simple_norm(image, 'sqrt') | |
| # Display the image | |
| fig = plt.figure() | |
| ax = fig.add_subplot(1, 1, 1) | |
| im = ax.imshow(image, origin='lower', norm=norm) | |
| fig.colorbar(im) | |
| Combining stretches and Matplotlib normalization | |
| ================================================ | |
| Stretches can also be combined with other stretches, just like transformations. | |
| The resulting :class:`~astropy.visualization.stretch.CompositeStretch` can be | |
| used to normalize Matplotlib images like any other stretch. For example, a | |
| composite stretch can stretch residual images with negative values: | |
| .. plot:: | |
| :include-source: | |
| :align: center | |
| import numpy as np | |
| import matplotlib.pyplot as plt | |
| from astropy.visualization.stretch import SinhStretch, LinearStretch | |
| from astropy.visualization import ImageNormalize | |
| # Transforms normalized values [0,1] to [-1,1] before stretch and then back | |
| stretch = LinearStretch(slope=0.5, intercept=0.5) + SinhStretch() + \ | |
| LinearStretch(slope=2, intercept=-1) | |
| # Image of random Gaussian noise | |
| image = np.random.normal(size=(64, 64)) | |
| fig = plt.figure() | |
| ax = fig.add_subplot(1, 1, 1) | |
| # ImageNormalize normalizes values to [0,1] before applying the stretch | |
| norm = ImageNormalize(stretch=stretch) | |
| im = ax.imshow(image, origin='lower', norm=norm, cmap='gray', | |
| vmin=-5, vmax=5) | |
| fig.colorbar(im) | |