DocumentCode
2338910
Title
Formation control for multiple mobile robots: a non-linear attractor dynamics approach
Author
Bicho, Estela ; Monteiro, Sergio
Author_Institution
Dept. of Industrial Electron., Minho Univ., Portugal
Volume
2
fYear
2003
fDate
27-31 Oct. 2003
Firstpage
2016
Abstract
In this paper we focus on modelling formations of non-holonomic mobile robots using non-linear attractor dynamics (see video). The benefit is that the behavior of each robot is generated by time series of asymptotically stable states, which therefore contribute to the robustness against environmental perturbations. This study extends our previous work [S Monteiro et al., 2002]. Here we develop a set of decentralized and distributed basic control architectures that allows each robot to maintain a desired pose within a formation and to enable changes in the shape of the formation which are necessary to avoid obstacles. Simulation results, for teams of four and six mobile robots driving in cluttered and unknown environments, while simultaneously trying to drive in line, column, square, diamond and hexagon are presented. We explain how this approach naturally extends to larger teams of robots.
Keywords
asymptotic stability; control system synthesis; decentralised control; distributed control; mobile robots; multi-robot systems; nonlinear control systems; nonlinear dynamical systems; robot dynamics; robust control; time series; asymptotically stable states; decentralized control; distributed basic control architectures; formation control; multiple mobile robots; nonlinear attractor dynamics approach; robustness; time series; Distributed control; Industrial electronics; Mobile robots; Robot kinematics; Robot sensing systems; Robust stability; Service robots; Shape control; Switches; Velocity control;
fLanguage
English
Publisher
ieee
Conference_Titel
Intelligent Robots and Systems, 2003. (IROS 2003). Proceedings. 2003 IEEE/RSJ International Conference on
Print_ISBN
0-7803-7860-1
Type
conf
DOI
10.1109/IROS.2003.1248953
Filename
1248953
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