Comparison of empirical models of ionospheric heating to global simulations

Intense currents produced during geomagnetic storms dissipate energy in the ionosphere through Joule heating. This dissipation has significant space weather effects, and thus it is important to determine the ability of physics-based simulations to replicate real events quantitatively. Several empiri...

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Main Authors: Fatemeh Bagheri, Ramon E. Lopez
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-06-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2023.1170390/full
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author Fatemeh Bagheri
Ramon E. Lopez
author_facet Fatemeh Bagheri
Ramon E. Lopez
author_sort Fatemeh Bagheri
collection DOAJ
description Intense currents produced during geomagnetic storms dissipate energy in the ionosphere through Joule heating. This dissipation has significant space weather effects, and thus it is important to determine the ability of physics-based simulations to replicate real events quantitatively. Several empirical models estimate Joule heating based on ionospheric currents using the AE index. In this study, we select 11 magnetic storm simulations from the CCMC database and compare the integrated Joule heating in the simulations with the results of empirical models. We also use the SWMF global magnetohydrodynamic simulations for 12 storms to reproduce the correlation between the simulated AE index and simulated Joule heating. We find that the scale factors in the empirical models are half what is predicted by the SWMF simulations.
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spelling doaj.art-f565ed8b89ab4051ac49ba29521813842023-06-08T04:56:40ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2023-06-011010.3389/fspas.2023.11703901170390Comparison of empirical models of ionospheric heating to global simulationsFatemeh BagheriRamon E. LopezIntense currents produced during geomagnetic storms dissipate energy in the ionosphere through Joule heating. This dissipation has significant space weather effects, and thus it is important to determine the ability of physics-based simulations to replicate real events quantitatively. Several empirical models estimate Joule heating based on ionospheric currents using the AE index. In this study, we select 11 magnetic storm simulations from the CCMC database and compare the integrated Joule heating in the simulations with the results of empirical models. We also use the SWMF global magnetohydrodynamic simulations for 12 storms to reproduce the correlation between the simulated AE index and simulated Joule heating. We find that the scale factors in the empirical models are half what is predicted by the SWMF simulations.https://www.frontiersin.org/articles/10.3389/fspas.2023.1170390/fullionospheric joule heatingCCMC simulationsSWMF simulationsAE indexFAC
spellingShingle Fatemeh Bagheri
Ramon E. Lopez
Comparison of empirical models of ionospheric heating to global simulations
Frontiers in Astronomy and Space Sciences
ionospheric joule heating
CCMC simulations
SWMF simulations
AE index
FAC
title Comparison of empirical models of ionospheric heating to global simulations
title_full Comparison of empirical models of ionospheric heating to global simulations
title_fullStr Comparison of empirical models of ionospheric heating to global simulations
title_full_unstemmed Comparison of empirical models of ionospheric heating to global simulations
title_short Comparison of empirical models of ionospheric heating to global simulations
title_sort comparison of empirical models of ionospheric heating to global simulations
topic ionospheric joule heating
CCMC simulations
SWMF simulations
AE index
FAC
url https://www.frontiersin.org/articles/10.3389/fspas.2023.1170390/full
work_keys_str_mv AT fatemehbagheri comparisonofempiricalmodelsofionosphericheatingtoglobalsimulations
AT ramonelopez comparisonofempiricalmodelsofionosphericheatingtoglobalsimulations