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Scintillation modeling

Author(s)
Materassi, Massimo  
nstitute for Complex Systems of the National Research Council (ISC-CNR), Florence, Italy  
Alfonsi, Lucilla  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia  
Spogli, Luca  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia  
Forte, Biagio  
Department of Electronic and Electrical Engineering, University of Bath, Bath, United Kingdom  
Language
English
Obiettivo Specifico
2A. Fisica dell'alta atmosfera
Publisher
Elsevier
Status
Published
Pages Number
277-299
Refereed
Yes
Journal
The Dynamical Ionosphere : A Systems Approach to Ionospheric Irregularity  
Date Issued
January 24, 2020
Alternative Location
https://www.sciencedirect.com/science/article/pii/B9780128147825000182
ISBN
9780128147825
URI
https://www.earth-prints.org/handle/2122/14185
Subjects
01.02. Ionosphere  
Abstract
In this chapter, some scintillation models are described, taking into account of the dynamical nature of the Earth's ionosphere and its “complexity.” After a short description of the problem, a detailed explanation is provided about the propagation model named WAM, after its authors Wernik, Alfonsi, and Materassi. WAM is a propagation model based on a phase screen approach, where the statistical characteristics of the screen are constructed according to in situ data of ionospheric irregularities. Then, the Ground-Based Scintillation Climatology (GBSC) model is presented; this is a tool based on a wide statistical database from high performance receivers.
Type
book chapter
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2020_Materassi_TheDynamicalIonosphere.pdf

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