Stochastic Channel Models for Satellite Mega-Constellations

Fuente: arXiv
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Auteurs principaux: McBain, Brendon, Hong, Yi, Viterbo, Emanuele
Format: Preprint
Publié: 2025
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author McBain, Brendon
Hong, Yi
Viterbo, Emanuele
author_facet McBain, Brendon
Hong, Yi
Viterbo, Emanuele
contents A general satellite channel model is proposed for communications between a rapidly moving low Earth orbit (LEO) satellite in a mega-constellation and a stationary user on Earth. The channel uses a non-homogeneous binomial point process (NBPP) for modelling the satellite positions, marked with an ascending/descending binary random variable for modelling the satellite directions. Using the marked NBPP, we derive the probability distributions of power gain, propagation delay, and Doppler shift, resulting in a stochastic signal propagation model for the mega-constellation geometry in isolation of other effects. This forms the basis for our proposed channel model as a randomly time-varying channel. The scattering function of this channel is derived to characterise how the received power is spread in the delay-Doppler domain. Global channel parameters such as path loss and channel spread are analysed in terms of the scattering function. The channel statistics and the global channel parameters closely match realistic orbit simulations of the Starlink constellation.
format Preprint
id arxiv_https___arxiv_org_abs_2507_20255
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Stochastic Channel Models for Satellite Mega-Constellations
McBain, Brendon
Hong, Yi
Viterbo, Emanuele
Information Theory
A general satellite channel model is proposed for communications between a rapidly moving low Earth orbit (LEO) satellite in a mega-constellation and a stationary user on Earth. The channel uses a non-homogeneous binomial point process (NBPP) for modelling the satellite positions, marked with an ascending/descending binary random variable for modelling the satellite directions. Using the marked NBPP, we derive the probability distributions of power gain, propagation delay, and Doppler shift, resulting in a stochastic signal propagation model for the mega-constellation geometry in isolation of other effects. This forms the basis for our proposed channel model as a randomly time-varying channel. The scattering function of this channel is derived to characterise how the received power is spread in the delay-Doppler domain. Global channel parameters such as path loss and channel spread are analysed in terms of the scattering function. The channel statistics and the global channel parameters closely match realistic orbit simulations of the Starlink constellation.
title Stochastic Channel Models for Satellite Mega-Constellations
topic Information Theory
url https://arxiv.org/abs/2507.20255