# Unveiling the Hyper-Rayleigh Regime of the Fluctuating Two-Ray Fading   Model

**Authors:** Celia Garcia-Corrales, Unai Fernandez-Plazaola, Francisco J. Ca\~nete,, Jos\'e F. Paris, F. Javier Lopez-Martinez

arXiv: 1905.00065 · 2020-04-02

## TL;DR

This paper investigates the hyper-Rayleigh behavior of the Fluctuating Two-Ray (FTR) fading model, revealing its full hyper-Rayleigh nature and the role of wave fluctuations, providing new insights into fading severity analysis.

## Contribution

It introduces a new scale to measure hyper-Rayleigh behavior and demonstrates that FTR exhibits full hyper-Rayleigh fading, unlike its predecessor model.

## Key findings

- FTR fading model shows full hyper-Rayleigh behavior.
- Two-Wave with Diffuse Power model has only strong hyper-Rayleigh behavior.
- Fluctuations in dominant waves cause full hyper-Rayleigh behavior.

## Abstract

The recently proposed Fluctuating Two-Ray (FTR) model is gaining momentum as a reference fading model in scenarios where two dominant specular waves are present. Despite the numerous research works devoted to the performance analysis under FTR fading, little attention has been paid to effectively understanding the interplay between the fading model parameters and the fading severity. According to a new scale defined in this work, which measures the hyper-Rayleigh character of a fading channel in terms of the Amount of Fading, the outage probability and the average capacity, we see that the FTR fading model exhibits a full hyper-Rayleigh behavior. However, the Two-Wave with Diffuse Power fading model from which the former is derived has only strong hyper-Rayleigh behavior, which constitutes an interesting new insight. We also identify that the random fluctuations in the dominant specular waves are ultimately responsible for the full hyper-Rayleigh behavior of this class of fading channels.

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1905.00065/full.md

## References

24 references — full list in the complete paper: https://tomesphere.com/paper/1905.00065/full.md

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Source: https://tomesphere.com/paper/1905.00065