Energy Flux Through the Magnetopause During Flux Transfer Events in Hybrid-Vlasov 2D Simulations

© 2022. The Authors.

Détails bibliographiques
Publié dans:Geophysical research letters. - 1984. - 49(2022), 19 vom: 16. Okt., Seite e2022GL100079
Auteur principal: Ala-Lahti, Matti (Auteur)
Autres auteurs: Pulkkinen, Tuija I, Pfau-Kempf, Yann, Grandin, Maxime, Palmroth, Minna
Format: Article en ligne
Langue:English
Publié: 2022
Accès à la collection:Geophysical research letters
Sujets:Journal Article Vlasiator flux transfer events hybrid‐Vlasov magnetopause reconnection solar wind—magnetosphere coupling
Description
Résumé:© 2022. The Authors.
Solar wind-magnetosphere coupling drives magnetospheric dynamic phenomena by enabling energy exchange between magnetospheric and solar wind plasmas. In this study, we examine two-dimensional noon-midnight meridional plane simulation runs of the global hybrid-Vlasov code Vlasiator with southward interplanetary magnetic field driving. We compute the energy flux, which consists of the Poynting flux and hydrodynamic energy flux components, through the Earth's magnetopause during flux transfer events (FTEs). The results demonstrate the spatiotemporal variations of the energy flux along the magnetopause during an FTE, associating the FTE leading (trailing) edge with an energy injection into (escape from) the magnetosphere on the dayside. Furthermore, FTEs traveling along the magnetopause transport energy to the nightside magnetosphere. We identify the tail lobes as a primary entry region for solar wind energy into the magnetosphere, consistent with results from global magnetohydrodynamic simulations and observations
Description:Date Revised 09.09.2024
published: Print-Electronic
Citation Status PubMed-not-MEDLINE
ISSN:0094-8276
DOI:10.1029/2022GL100079