Location dependent variable information gain approach to multi robot coverage problem

Author(s):  
Mert Turanli ◽  
Hakan Temeltas
2021 ◽  
pp. 349-353
Author(s):  
Thomas Green ◽  
Kevin Kamel ◽  
Siyuan Li ◽  
Christopher Shinn ◽  
Paolo Toscano ◽  
...  

Author(s):  
Mor Sinay ◽  
Noa Agmon ◽  
Oleg Maksimov ◽  
Sarit Kraus ◽  
David Peleg

Area coverage is an important task for mobile robots, mainly due to its applicability in many domains, such as search and rescue. In this paper we study the problem of multi-robot coverage, in which the robots must obey a strong communication restriction: they should maintain connectivity between teammates throughout the coverage. We formally describe the Multi-Robot Connected Tree Coverage problem, and an algorithm for covering perfect N-ary trees while adhering to the communication requirement. The algorithm is analyzed theoretically, providing guarantees for coverage time by the notion of speedup factor. We enhance the theoretically-proven solution with a dripping heuristic algorithm, and show in extensive simulations that it significantly decreases the coverage time. The algorithm is then adjusted to general (not necessarily perfect) N-ary trees and additional experiments prove its efficiency. Furthermore, we show the use of our solution in a simulated officebuilding scenario. Finally, we deploy our algorithm on real robots in a real office building setting, showing efficient coverage time in practice.


1995 ◽  
Vol 04 (01) ◽  
pp. 1-50 ◽  
Author(s):  
S. FRASCA ◽  
M.A. PAPA

There are many reasons, other than that of excluding local disturbances, for using more gravitational antennas at the same time. In fact a network of resonant antennas allows — the detection of radiation coming from any direction and in any polarization state (sky coverage problem). — the estimate of some parameters of the source (information gain). — the verification of the predictions of general relativity regarding the features of gravitational waves (e.g. their propagation velocity, their quadrupole nature etc.) and the existence of celestial objects which cannot be observed other than through the gravitational effects they produce (e.g. black holes). — the enhancement of the noise rejection capability of the instrument thus enhancing its sensitivity (network filtering). Regarding this feature, some very interesting characteristics are exhibited by local networks of equal antennas (gravitational arrays). In this paper the major issues related to these problems will be presented and discussed and the experimental and theoretical results will briefly be reviewed. Some new ideas will also be introduced.


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