A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting

Abstract Equatorial plasma bubbles (EPBs) have been a longstanding and increasingly important subject because they cause severe scintillations in radio waves from Global Navigation Satellite System satellites. The phenomenon was found in the 1930s as irregular ionosonde observations and was termed e...

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Main Author: Tatsuhiro Yokoyama
Format: Article
Language:English
Published: SpringerOpen 2017-12-01
Series:Progress in Earth and Planetary Science
Subjects:
Online Access:http://link.springer.com/article/10.1186/s40645-017-0153-6
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author Tatsuhiro Yokoyama
author_facet Tatsuhiro Yokoyama
author_sort Tatsuhiro Yokoyama
collection DOAJ
description Abstract Equatorial plasma bubbles (EPBs) have been a longstanding and increasingly important subject because they cause severe scintillations in radio waves from Global Navigation Satellite System satellites. The phenomenon was found in the 1930s as irregular ionosonde observations and was termed equatorial spread F (ESF). ESF is interpreted as plasma density irregularities associated with EPBs that have nonlinearly evolved into the topside ionosphere. Numerical simulations have been powerful tools to study the fully nonlinear evolution of EPBs, which cannot be wholly understood from theoretical predictions. In this paper, historical achievements in the numerical simulation of EPBs are reviewed, and future directions toward scintillation evaluation and forecast are discussed.
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spelling doaj.art-b52476a522cf4ff3aecae332797e47e42022-12-21T23:30:10ZengSpringerOpenProgress in Earth and Planetary Science2197-42842017-12-014111310.1186/s40645-017-0153-6A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecastingTatsuhiro Yokoyama0National Institute of Information and Communications TechnologyAbstract Equatorial plasma bubbles (EPBs) have been a longstanding and increasingly important subject because they cause severe scintillations in radio waves from Global Navigation Satellite System satellites. The phenomenon was found in the 1930s as irregular ionosonde observations and was termed equatorial spread F (ESF). ESF is interpreted as plasma density irregularities associated with EPBs that have nonlinearly evolved into the topside ionosphere. Numerical simulations have been powerful tools to study the fully nonlinear evolution of EPBs, which cannot be wholly understood from theoretical predictions. In this paper, historical achievements in the numerical simulation of EPBs are reviewed, and future directions toward scintillation evaluation and forecast are discussed.http://link.springer.com/article/10.1186/s40645-017-0153-6Equatorial ionosphereEquatorial spread FEquatorial plasma bubblesNumerical simulationScintillationHigh-performance computing
spellingShingle Tatsuhiro Yokoyama
A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
Progress in Earth and Planetary Science
Equatorial ionosphere
Equatorial spread F
Equatorial plasma bubbles
Numerical simulation
Scintillation
High-performance computing
title A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
title_full A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
title_fullStr A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
title_full_unstemmed A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
title_short A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
title_sort review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting
topic Equatorial ionosphere
Equatorial spread F
Equatorial plasma bubbles
Numerical simulation
Scintillation
High-performance computing
url http://link.springer.com/article/10.1186/s40645-017-0153-6
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