A Semi-2D Synthetic Storm Technique for Orbital Diversity on Earth-Space Propagation Paths

In this article, new assumptions are introduced into the well-known synthetic storm technique (SST) proposed by Drufuca and further developed by Matricciani, to address the orbital diversity in satellite links. The new approach receives as input information on collocated rain rate recordings and ins...

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Veröffentlicht in:IEEE transactions on antennas and propagation 2021-03, Vol.69 (3), p.1631-1642
Hauptverfasser: Pastoriza-Santos, Vicente, Machado, Fernando, Nandi, Dalia, Sanroman, Pablo, Perez-Fontan, Fernando
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container_title IEEE transactions on antennas and propagation
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creator Pastoriza-Santos, Vicente
Machado, Fernando
Nandi, Dalia
Sanroman, Pablo
Perez-Fontan, Fernando
description In this article, new assumptions are introduced into the well-known synthetic storm technique (SST) proposed by Drufuca and further developed by Matricciani, to address the orbital diversity in satellite links. The new approach receives as input information on collocated rain rate recordings and instantaneous estimates of the storm direction and speed; and assumes that the rain event is transversely constant to the storm movement. The achieved improvements are evaluated by analyzing two example measured rain attenuation events "seen" by two Ka -band beacon receivers looking at two different satellites spaced around in azimuth. A study is made of the cross correlation coefficient between rain attenuation series for these two links. Moreover, a methodology is sketched as to how multiple non-GEO satellite constellation availability (for global Internet access at Ka -band) could be evaluated in the frame of the SST.
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source IEEE Electronic Library (IEL)
subjects Attenuation
Correlation analysis
Correlation coefficients
Cross correlation
Evaluation
Ice
orbital diversity
Radar imaging
Rain
satellite communication
Satellite communications
Satellite constellations
Satellites
Storms
synthetic storm technique (SST)
title A Semi-2D Synthetic Storm Technique for Orbital Diversity on Earth-Space Propagation Paths
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