Using our current approach, we have built maps as large as 260 x 166 meters from sequences of range data. The algorithm is built upon an earlier surface matching system developed by Andrew Johnson. The input to our algorithm is a sequence of range images obtained from different viewpoints. For example, we generated several sequences while driving down a dirt road, stopping periodically to record the surroundings with a laser scanner mounted on the roof. First, we convert each range image in the sequence into a triangular surface mesh. Then, in the registration step, we determine the transformation that aligns each mesh with the next one in the sequence. Finally, we transform all the meshes into a single coordinate system and integrate them into a single 3D map.
Our map building algorithm provides three capabilities not found together in any previous terrain modeling algorithm. First, we have no requirement for an initial approximation of the transform between views or the orientation of the sensor. Second, there is no need to detect explicit features in the environment because we rely on local shape signatures over the entire sensed surface. Finally, it is unnecessary to reduce the sensed data to the more limited elevation map representation.
Our initial work demonstrated that automatically building terrain maps of this size is possible. We concentrated on the aspects specific to map building using ground-based sensors, including widely varying resolution, range shadows, absence of reliably detectable features, and very large data sets. Now, we are extending the basic algorithm and testing the limits of its performance. We are looking at ways to determine how much overlap between views is necessary to register the views, and we are trying to reduce the amount of computation in the registration process by intelligently selecting points on the terrain surface for comparison.
Details are available on the following topics:
Examples of the type of terrain for which we are building maps. The slag heap near CMU (left) and Haughten crater on Devin Island in the Canadian Arctic (right). |
The data for our experiments was gathered using laser rangefinders: the Ben Franklin 2 mounted on Navlab 5 (left) and CMU's autonomous helicopter (right). |
Last modified February 15, 1999 Daniel Huber (dhuber@cs.cmu.edu) |