In this paper, we study the communication problem from rovers on Mars’ surface to Mars-orbiting satellites. We first justify that, to a good extent, the rover-to-orbiter communication problem can be modeled as communication over a   $2 \times 2$   X-channel with the network topology  varying  over time. For such a fading X-channel where transmitters are only aware of the time-varying topology but not the time-varying channel state (i.e., no CSIT), we propose coding strategies that  code across topologies , and develop upper bounds on the sum degrees-of-freedom (DoF) that is shown to be tight under certain pattern of the topology variation. Furthermore, we demonstrate that the proposed scheme approximately achieves the ergodic sum-capacity of the network. Using the proposed coding scheme, we numerically evaluate the ergodic rate gain over a time-division-multiple-access (TDMA) scheme for Rayleigh and Rice fading channels. We also numerically demonstrate that with practical orbital parameters, a 9.6% DoF gain, as well as more than 11.6% throughput gain can be achieved for a rover-to-orbiter communication network.
['Songze Li', 'David T. H. Kao', 'A. Salman Avestimehr']
Rover-to-Orbiter Communication in Mars: Taking Advantage of the Varying Topology