Spectral Python (SPy) is a pure Python module for processing hyperspectral image data. It has functions for reading, displaying, manipulating, and classifying hyperspectral imagery. It can be used interactively from the Python command prompt or via Python scripts. SPy is free, open source software distributed under the GNU General Public License. To see some examples of how SPy can be used, you may want to jump straight to the documentation sections on Displaying Data or Spectral Algorithms. A categorized listing of the main classes and functions are in the Class/Function Glossary. You can download SPy from GitHub, the Python Package Index (PyPI), or Sourceforge. See the Installing SPy section section of the documentation for details.
2014-10-18 : SPy 0.16.0 provides initial support for Python 3.
New features in this release include the Adaptive Coherence/Cosine Esimator (ace) target detector, Pixel Purity Index (ppi), ability to save ENVI classification files (envi.save_classification), and linear contrast enhancement (by data limits or cumulative histogram percentiles). The SPy imshow function now applies a 2% histogram color stretch by default (this can be overridden in the spectral.settings object).
Additional info is in the version 0.16.0 issues.
2014-06-04 : SPy 0.15.0 is released.
This version adds the Minimum Noise Fraction algorithm (mnf) (a.k.a., Noise-Adjusted Principal Components). The related function noise_from_diffs performs estimation of image noise from a spectrally homogeneous region of the image.
SpyFile read methods now accept an optional use_memmap argument that provides finer control over when to use (or not use) the memmap interface to read image file data.
Many thanks to Don March (http://ohspite.net) for improving ENVI header support (comment lines and blank parameters are now accepted) and providing several performance improvements.
Additional details are here.
2014-03-02 : SPy has moved!
The Spectral Python web site is now located at www.spectralpython.net. All old URLs will automatically redirect to the new site. The primary source code repository has also moved and is now hosted on GitHub at https://github.com/spectralpython/spectral. For the indefinite future, source code and release builds will continue to be mirrored on Sourceforge.net and as always, the current release can always be installed from the Python Package Index (PyPI) using pip.
2014-02-23 : SPy 0.14 is released. This is primarily a bug fix release.
2014-01-06 : Numerous new user interface features and performance improvements in SPy 0.13.
The SPy imshow wrapper around matplotlib’s imshow function provides numerous new features, including:
- Interactive image class labeling using keyboard & mouse
- Zoom windows
- Class overlays with adjustable transparency
- Dynamic view of changing pixel classes when modified in an ND Window.
Data/Statistic cacheing and more efficient use of numpy provides significant performance improvement in mutiple algorithms (GMLC 14x, Mahalanobis classifier 8x, kmeans 3x). Functions rx and matched_filter are significantly faster, particularly when using common global covariance.
The cov_avg function computes covariance averaged over a set of classes (useful when samples are limited or global covariance is desired). Christian Mielke provided code for the msam function, which computes the Modified SAM score (by Oshigami et al).
2013-09-06 : SPy 0.12 is released.
SPy 0.12 provides an improved memmap interface that enables accessing image data using arbitrary interleaves and supports editable images (see open_memmap for details). The RX anomaly detector (rx) now allows anomaly detection using local (sub-image) statistics by specifying an inner/outer window around each pixel. The ability to disable algorithm progress messages and addition of a wrapper around matplotlib’s imshow function are provided to simplify integration of SPy code with IPython Notebooks.
2013-04-03 : SPy 0.11 is released.
This release adds an RX anomaly detector, ability to save and create images in ENVI format (see save_image and create_image), and a unit-testing sub-package. The top-level namespace has been simplified and several functions have been renamed for consistency (image is now open_image and save_image is now save_rgb).
2013-02-23 : SPy 0.10.1 bug-fix release is now available.
This is a bug-fix release that corrects the spectrum displayed when double- clicking on a raster display. Version 0.10 introduced a bug that had the row/column swapped, resulting in either the wrong pixel being plotted or an exception raised.
If you have installed SPy 0.10, you should install this update as soon as possible.
2013-02-17 : SPy 0.10 is released: SPy now uses IPython for GUI display.
As of this release, SPy now uses IPython for non-blocking GUI windows. IPython should be started in pylab mode with the appropriate backend set (see Starting IPython). The standard python interpreter can still be used if GUI functions are not being called. This release also resolves a number of issues associated with different versions of wxWidgets (2.8.x vs. 2.9.x) on various operating systems.
2013-01-23 : SPy 0.9 adds a linear matched filter target detector.
2012-07-10 : SPy 0.8 adds N-Dimensional visualization of hyperspectral image data.
The ndwindow function enables viewing of high-dimensional images in a 3D display. See N-Dimensional Feature Display for details.
Hypercube display now uses mouse control for pan/zoom/rotate.
Fixed a bug in several deprecation warnings that caused infinte recursion.
2012-02-19 : SPy 0.7 Released.
The kmeans algorithm is about 10 times faster than version 0.6. Many method/function names have been renamed for consistency with external packages. A few bugs potentially affecting BIP and BSQ input have been fixed.
2011-01-17 : SPy 0.6 Released.
This release adds ASTER Spectral Library support, ability to save spectral libraries, and installation via distutils.