In this study, we model the LEO satellite constellation with link failures as the Δ -random regular graph, where Δ : (≥q 4) is the number of antennas per satellite, i.e, each satellite can establish at most Δ inter-satellite links (ISLs). It is found that the critical temporary failure probability at which the constellation structure collapses is pc(Δ) = Δ -2Δ -1. We show that the capacity upper bound is proportional to Δ γ (p)L(α,D) when p< pc(Δ). L(α,D) is the average hop distance without link failures under traffic decay factor α in (0,1). γ (p)< is the hop stretch factor measuring the extra hops to overcome link failures. D is the diameter of constellations. When p to 0 and α to 1 , our results degenerate to the capacity upper bound under all-to-all traffic model. We also show that the capacity upper bound of one-to-many traffic is sm times that of many-to-one, where m is the number of source or destination satellites. This is because, in one-to-many traffic model, the source satellite transmits identical data packets to the destination satellites. To achieve the capacity upper bound, we propose the distributed shortest-hop routing framework based on local link states (DSR-L), which uses prior geometric knowledge of the constellation structure. These results can provide effective guidance for resilience strategies regarding redundant satellites and ISL configurations.
The Capacity of LEO Satellite Constellations With Link Failures
Pace P.;Fortino G.;
2026-01-01
Abstract
In this study, we model the LEO satellite constellation with link failures as the Δ -random regular graph, where Δ : (≥q 4) is the number of antennas per satellite, i.e, each satellite can establish at most Δ inter-satellite links (ISLs). It is found that the critical temporary failure probability at which the constellation structure collapses is pc(Δ) = Δ -2Δ -1. We show that the capacity upper bound is proportional to Δ γ (p)L(α,D) when p< pc(Δ). L(α,D) is the average hop distance without link failures under traffic decay factor α in (0,1). γ (p)< is the hop stretch factor measuring the extra hops to overcome link failures. D is the diameter of constellations. When p to 0 and α to 1 , our results degenerate to the capacity upper bound under all-to-all traffic model. We also show that the capacity upper bound of one-to-many traffic is sm times that of many-to-one, where m is the number of source or destination satellites. This is because, in one-to-many traffic model, the source satellite transmits identical data packets to the destination satellites. To achieve the capacity upper bound, we propose the distributed shortest-hop routing framework based on local link states (DSR-L), which uses prior geometric knowledge of the constellation structure. These results can provide effective guidance for resilience strategies regarding redundant satellites and ISL configurations.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


