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http://hdl.handle.net/2122/14185| Authors: | Materassi, Massimo* Alfonsi, Lucilla* Spogli, Luca* Forte, Biagio* |
Title: | Scintillation modeling | Publisher: | Elsevier | Issue Date: | 24-Jan-2020 | URL: | https://www.sciencedirect.com/science/article/pii/B9780128147825000182 | ISBN: | 9780128147825 | Subject Classification: | 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. |
| Appears in Collections: | Book chapters |
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| 2020_Materassi_TheDynamicalIonosphere.pdf | 56.44 MB | Adobe PDF |
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