Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms

Abstract This paper presents the validation of modeled total electron content (TEC) from 14 ionospheric models, including empirical, physics‐based, and data assimilation (DA) models, hosted by the NASA/NSF Community Coordinated Modeling Center (CCMC), NOAA Space Weather Prediction Center, and NASA J...

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Main Authors: Min‐Yang Chou, Jia Yue, Jack Wang, J. D. Huba, Mostafa El Alaoui, Maria M. Kuznetsova, Lutz Rastätter, Ja Soon Shim, Tzu‐Wei Fang, Xing Meng, Dominic Fuller‐Rowell, John M. Retterer
Format: Article
Language:English
Published: Wiley 2023-06-01
Series:Space Weather
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Online Access:https://doi.org/10.1029/2023SW003480
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author Min‐Yang Chou
Jia Yue
Jack Wang
J. D. Huba
Mostafa El Alaoui
Maria M. Kuznetsova
Lutz Rastätter
Ja Soon Shim
Tzu‐Wei Fang
Xing Meng
Dominic Fuller‐Rowell
John M. Retterer
author_facet Min‐Yang Chou
Jia Yue
Jack Wang
J. D. Huba
Mostafa El Alaoui
Maria M. Kuznetsova
Lutz Rastätter
Ja Soon Shim
Tzu‐Wei Fang
Xing Meng
Dominic Fuller‐Rowell
John M. Retterer
author_sort Min‐Yang Chou
collection DOAJ
description Abstract This paper presents the validation of modeled total electron content (TEC) from 14 ionospheric models, including empirical, physics‐based, and data assimilation (DA) models, hosted by the NASA/NSF Community Coordinated Modeling Center (CCMC), NOAA Space Weather Prediction Center, and NASA Jet Propulsion Laboratory (JPL). This study aims to assess the current progress and capability of the CCMC‐hosted ionospheric models in capturing the storm time ionosphere during the low and moderate solar flux years. We focus on the low‐latitude ionosphere (i.e., ±40° in magnetic latitude) and compare the modeled TEC with the Madrigal TEC during the 2013 March and 2021 November storms. Multiple metrics are used to quantitatively assess the models' accuracy, precision, association, bias, and capability in capturing the TEC changes in response to the storms. The skill score based on the metric scores is further proposed to evaluate the overall performance of ionospheric models against the reference model (International Reference Ionosphere 2016; IRI‐2016). The results indicate that the DA model GLObal Total Electron Content and JPL Global Ionospheric Map models show good performance in modeling the TEC and reasonably reflect the storm time TEC changes spatially and temporally. The empirical models IRI‐2016 and 2020 show relatively good performance compared with the physics‐based models regarding the model‐data comparison; however, it is difficult to characterize the TEC changes caused by storms. The physics‐based models can simulate the storm effect in spatial and temporal TEC variations better than the empirical model. The performance of ionospheric models in capturing the storm time TEC anomaly is presented and discussed.
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issn 1542-7390
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spelling doaj-art-19769f65f48a4e328d3dd403f66c75232025-01-14T16:27:02ZengWileySpace Weather1542-73902023-06-01216n/an/a10.1029/2023SW003480Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic StormsMin‐Yang Chou0Jia Yue1Jack Wang2J. D. Huba3Mostafa El Alaoui4Maria M. Kuznetsova5Lutz Rastätter6Ja Soon Shim7Tzu‐Wei Fang8Xing Meng9Dominic Fuller‐Rowell10John M. Retterer11NASA Goddard Space Flight Center Community Coordinated Modeling Center Greenbelt MD USANASA Goddard Space Flight Center Community Coordinated Modeling Center Greenbelt MD USANASA Goddard Space Flight Center Community Coordinated Modeling Center Greenbelt MD USASyntek Technologies Fairfax VA USANASA Goddard Space Flight Center Community Coordinated Modeling Center Greenbelt MD USANASA Goddard Space Flight Center Community Coordinated Modeling Center Greenbelt MD USANASA Goddard Space Flight Center Community Coordinated Modeling Center Greenbelt MD USADepartment of Atmospheric Sciences Yonsei University Seoul South KoreaNOAA Space Weather Prediction Center Boulder CO USAJet Propulsion Laboratory California Institute of Technology Pasadena CA USANOAA Space Weather Prediction Center Boulder CO USAInstitute for Scientific Research Boston College Chestnut Hill MA USAAbstract This paper presents the validation of modeled total electron content (TEC) from 14 ionospheric models, including empirical, physics‐based, and data assimilation (DA) models, hosted by the NASA/NSF Community Coordinated Modeling Center (CCMC), NOAA Space Weather Prediction Center, and NASA Jet Propulsion Laboratory (JPL). This study aims to assess the current progress and capability of the CCMC‐hosted ionospheric models in capturing the storm time ionosphere during the low and moderate solar flux years. We focus on the low‐latitude ionosphere (i.e., ±40° in magnetic latitude) and compare the modeled TEC with the Madrigal TEC during the 2013 March and 2021 November storms. Multiple metrics are used to quantitatively assess the models' accuracy, precision, association, bias, and capability in capturing the TEC changes in response to the storms. The skill score based on the metric scores is further proposed to evaluate the overall performance of ionospheric models against the reference model (International Reference Ionosphere 2016; IRI‐2016). The results indicate that the DA model GLObal Total Electron Content and JPL Global Ionospheric Map models show good performance in modeling the TEC and reasonably reflect the storm time TEC changes spatially and temporally. The empirical models IRI‐2016 and 2020 show relatively good performance compared with the physics‐based models regarding the model‐data comparison; however, it is difficult to characterize the TEC changes caused by storms. The physics‐based models can simulate the storm effect in spatial and temporal TEC variations better than the empirical model. The performance of ionospheric models in capturing the storm time TEC anomaly is presented and discussed.https://doi.org/10.1029/2023SW003480ionospherenumerical modelsTECgeomagnetic stormvalidation
spellingShingle Min‐Yang Chou
Jia Yue
Jack Wang
J. D. Huba
Mostafa El Alaoui
Maria M. Kuznetsova
Lutz Rastätter
Ja Soon Shim
Tzu‐Wei Fang
Xing Meng
Dominic Fuller‐Rowell
John M. Retterer
Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms
Space Weather
ionosphere
numerical models
TEC
geomagnetic storm
validation
title Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms
title_full Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms
title_fullStr Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms
title_full_unstemmed Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms
title_short Validation of Ionospheric Modeled TEC in the Equatorial Ionosphere During the 2013 March and 2021 November Geomagnetic Storms
title_sort validation of ionospheric modeled tec in the equatorial ionosphere during the 2013 march and 2021 november geomagnetic storms
topic ionosphere
numerical models
TEC
geomagnetic storm
validation
url https://doi.org/10.1029/2023SW003480
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