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Since December 2008, UCL-MSSL developed a platform independent stereo application in collaboration with JPL, NASA as a subtask of EU-FP7 PRoViSG. This work was originally proposed for two months of work, but it was rescheduled to run untill August 2011 after realising its synergetic relationship with other UCL tasks within the ProVisG project. Within this time period, UCL delivered consortium members a stereo application (called StereoWS ver. 1.0), which integrates various practical stereo tools into the JPL’s stereo rendering engine (called JADIS). ...

...More information is available at Wikipedia, the Kalmn Filter was derived to solve the Wiener filter problem. The Wiener filter problem is to reduce the amount of noise present in a signal by comparison with an estimation of the desired noiseless signal. The discrete-time equivalent of Wiener's work was derived independently by Kolmogorov and published in 1941. Hence the theory is often called the Wiener-Kolmogorov filtering theory. In these examples the signal processes is the movement of the mouse and random data. While a simple application the algorithm can have numerous applications including image smoothing, edge tracking and optical flow to name a few.