Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation

<p>We present a new semi-analytical magnetopause location model specifically designed for 4D drift-resolved radiation belt modeling codes. We specifically designed this magnetopause location model for the 4D version of Salammbô, but it can be adaptable to similar codes. The model combines para...

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Main Authors: R. Kiraz, N. Dahmen, V. Maget, B. Lavraud
Format: Article
Language:English
Published: Copernicus Publications 2025-07-01
Series:Annales Geophysicae
Online Access:https://angeo.copernicus.org/articles/43/369/2025/angeo-43-369-2025.pdf
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author R. Kiraz
N. Dahmen
V. Maget
B. Lavraud
author_facet R. Kiraz
N. Dahmen
V. Maget
B. Lavraud
author_sort R. Kiraz
collection DOAJ
description <p>We present a new semi-analytical magnetopause location model specifically designed for 4D drift-resolved radiation belt modeling codes. We specifically designed this magnetopause location model for the 4D version of Salammbô, but it can be adaptable to similar codes. The model combines parameterization by the Kp index with a representation of the magnetopause in <span class="inline-formula"><i>L</i><sup>∗</sup></span> geomagnetic coordinates and magnetic local time (MLT). It is based on a 20-year dataset relying on computed magnetopause stand-off distances using a solar wind database and a relevant magnetopause model, then converted into <span class="inline-formula"><i>L</i><sup>∗</sup></span> geomagnetic coordinates for all dayside MLT. Through the statistical analysis of this dataset, the model was formulated and validated against a magnetopause crossing catalog. Its performance was benchmarked against the magnetopause location model previously developed for the 3D version of the Salammbô code. The results demonstrate an improvement in predicting the magnetopause position in <span class="inline-formula"><i>L</i><sup>∗</sup></span> across dayside MLT sectors, with enhanced accuracy in the dawn sector. These results highlight the model's ability to model the magnetopause location in <span class="inline-formula"><i>L</i><sup>∗</sup></span> across dayside MLT sectors. This advancement may be specifically useful for simulating magnetopause shadowing in ring current and radiation belt modeling codes.</p>
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spelling doaj-art-ea8a5301707b4e9ebfd084797cae42bd2025-08-20T03:30:44ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762025-07-014336938210.5194/angeo-43-369-2025Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementationR. Kiraz0N. Dahmen1V. Maget2B. Lavraud3ONERA/DPHY, Université de Toulouse, Toulouse, 31055, FranceONERA/DPHY, Université de Toulouse, Toulouse, 31055, FranceONERA/DPHY, Université de Toulouse, Toulouse, 31055, FranceLaboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, Bordeaux, 33615 Pessac, France<p>We present a new semi-analytical magnetopause location model specifically designed for 4D drift-resolved radiation belt modeling codes. We specifically designed this magnetopause location model for the 4D version of Salammbô, but it can be adaptable to similar codes. The model combines parameterization by the Kp index with a representation of the magnetopause in <span class="inline-formula"><i>L</i><sup>∗</sup></span> geomagnetic coordinates and magnetic local time (MLT). It is based on a 20-year dataset relying on computed magnetopause stand-off distances using a solar wind database and a relevant magnetopause model, then converted into <span class="inline-formula"><i>L</i><sup>∗</sup></span> geomagnetic coordinates for all dayside MLT. Through the statistical analysis of this dataset, the model was formulated and validated against a magnetopause crossing catalog. Its performance was benchmarked against the magnetopause location model previously developed for the 3D version of the Salammbô code. The results demonstrate an improvement in predicting the magnetopause position in <span class="inline-formula"><i>L</i><sup>∗</sup></span> across dayside MLT sectors, with enhanced accuracy in the dawn sector. These results highlight the model's ability to model the magnetopause location in <span class="inline-formula"><i>L</i><sup>∗</sup></span> across dayside MLT sectors. This advancement may be specifically useful for simulating magnetopause shadowing in ring current and radiation belt modeling codes.</p>https://angeo.copernicus.org/articles/43/369/2025/angeo-43-369-2025.pdf
spellingShingle R. Kiraz
N. Dahmen
V. Maget
B. Lavraud
Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation
Annales Geophysicae
title Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation
title_full Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation
title_fullStr Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation
title_full_unstemmed Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation
title_short Modeling magnetopause location for 4D drift-resolved radiation belt codes: Salammbô model implementation
title_sort modeling magnetopause location for 4d drift resolved radiation belt codes salammbo model implementation
url https://angeo.copernicus.org/articles/43/369/2025/angeo-43-369-2025.pdf
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AT vmaget modelingmagnetopauselocationfor4ddriftresolvedradiationbeltcodessalammbomodelimplementation
AT blavraud modelingmagnetopauselocationfor4ddriftresolvedradiationbeltcodessalammbomodelimplementation