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Begum Cannataro

Publications and source records attributed to Begum Cannataro.

3 recordsLinked to original sources

AC-DC: Adaptive Communication for Scalable Dynamic Average Consensus in Multi-Robot Ergodic Search

We study scalable peer-to-peer dynamic average consensus (DC) for multi-robot systems under finite-range, finite-rate, and interference-constrained communication. We introduce Adaptive Communication for Dynamic Average Consensus (AC-DC), which jointly adapts Who communicates with whom, When, and over What parts of the consensus state, using local inputs and successfully received neighbor information. Each robot's consensus state estimates the current average of the robots' local inputs. AC-DC updates these estimates as local inputs change and averages the values exchanged between robot pairs. In AC-DC, robot pairs update without waiting for every robot to complete a communication round, and the selected-state messages carry consensus state coordinates independent of team size for a fixed state representation. We apply AC-DC to dynamic-priority multi-robot ergodic search: one consensus stream estimates team visitation for motion coordination, while the other fuses regional measurement information to update uncertainty maps and search targets. Across twelve settings with up to 80 robots and 20 paired trials per setting, AC-DC has the lowest mean (i) normalized covariance-trace area under the curve (AUC) and (ii) attempted modeled communication payload among the compared decentralized methods. Averaged across settings, AC-DC achieves paired AUC reductions of 27.5% relative to state-of-the-art baselines, with 8.7x less communication traffic. As the number of robots increases, we observe that AC-DC's communication payload approaches that of the ideal centralized baseline (one ground compute-station communicating directly with all robots): with 120 robots in a fixed 600 x 600 m scaling test, AC-DC uses 19.3 MB versus 19.2 MB for the ideal centralized baseline, while remaining peer-to-peer.

cs.RO↗

Approximate Analytical Solutions for the Circular Restricted Three-Body Problem Including Non-Hamiltonian Solar Radiation Pressure

The circular restricted three-body problem (CR3BP) with solar radiation pressure (SRP) has often been analyzed with assumptions made on a spacecraft's attitude, such that the problem remains Hamiltonian. These assumptions are unsatisfactorily limiting for a starshade mission since the starshade's attitude will inherently vary from the configuration that corresponds to Hamiltonian dynamics. This paper presents the derivation of the equations of motion for CR3BP with SRP that permit the application of the Lindstedt-Poincare method, such that approximate solutions are produced, which may serve as invaluable trajectory design tools. Examples of periodic orbits and manifolds corresponding to three sets of attitude angles are shown and the accuracy of their seventh-order approximations is considered.

math.DS↗

Tracing Position in the Regime of the Restricted Three-Body Problem to a Halo Orbit

Driven by the desire to find positions that satisfy keepout constraints for a space-based telescope mission, this work develops a process for tracing a point in space in the regime of the restricted three-body problem to a halo orbit, characterized by its out-of-plane amplitude, and its position on that halo orbit, denoted by the halo orbit time. This process utilizes third-order solutions from the Lindstedt-Poincare method, which have been partially inverted to expect a point in space as an input. Three different methodologies that use these partially inverted expressions are presented. Results are produced for 1,000 randomly selected points using all three methods and are compared to truth. Ultimately, the method that employed two distinct accuracy metrics yielded the most accurate results for the dataset.

math.DS↗