Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations

A coronal mass ejection (CME) and post-CME blob phenomena in the solar atmosphere, associated with shear flow and convergent flow perturbations in the photosphere, are investigated using a resistive two-fluid (electron–ion) code. It is found that there are notable deviations between the two-fluid an...

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Main Authors: J. C. Du, Z. W. Ma
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ada951
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author J. C. Du
Z. W. Ma
author_facet J. C. Du
Z. W. Ma
author_sort J. C. Du
collection DOAJ
description A coronal mass ejection (CME) and post-CME blob phenomena in the solar atmosphere, associated with shear flow and convergent flow perturbations in the photosphere, are investigated using a resistive two-fluid (electron–ion) code. It is found that there are notable deviations between the two-fluid and previous magnetohydrodynamic simulations. In this two-fluid approach, the decoupling motions of ions and electrons leads to the emergence of an additional electric field. With expansion of a magnetic arcade associated with the footpoint shear flows, a thin current sheet is formed and a series of magnetic reconnections occurs in the lower region of the central magnetic arcade. The initial reconnection gives rise to a rising magnetic island, displaying typical CME characteristics. Subsequent reconnections produce smaller, more rapidly ascending blobs. These smaller blobs ultimately merge with the primary CME core, thereby accelerating its ascent.
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spelling doaj-art-fec9654aa311477dbd3ea6c7368d72c82025-02-07T06:32:03ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01980112010.3847/1538-4357/ada951Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid SimulationsJ. C. Du0Z. W. Ma1https://orcid.org/0000-0001-6199-9389Institute for Fusion Theory and Simulation, Department of Physics, Zhejiang University , Hangzhou 310027, People's Republic of China ; [email protected] for Fusion Theory and Simulation, Department of Physics, Zhejiang University , Hangzhou 310027, People's Republic of China ; [email protected] coronal mass ejection (CME) and post-CME blob phenomena in the solar atmosphere, associated with shear flow and convergent flow perturbations in the photosphere, are investigated using a resistive two-fluid (electron–ion) code. It is found that there are notable deviations between the two-fluid and previous magnetohydrodynamic simulations. In this two-fluid approach, the decoupling motions of ions and electrons leads to the emergence of an additional electric field. With expansion of a magnetic arcade associated with the footpoint shear flows, a thin current sheet is formed and a series of magnetic reconnections occurs in the lower region of the central magnetic arcade. The initial reconnection gives rise to a rising magnetic island, displaying typical CME characteristics. Subsequent reconnections produce smaller, more rapidly ascending blobs. These smaller blobs ultimately merge with the primary CME core, thereby accelerating its ascent.https://doi.org/10.3847/1538-4357/ada951Solar coronal mass ejectionsSolar coronaSolar magnetic reconnection
spellingShingle J. C. Du
Z. W. Ma
Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations
The Astrophysical Journal
Solar coronal mass ejections
Solar corona
Solar magnetic reconnection
title Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations
title_full Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations
title_fullStr Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations
title_full_unstemmed Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations
title_short Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations
title_sort solar coronal mass ejection and post coronal mass ejection blob formation in two fluid simulations
topic Solar coronal mass ejections
Solar corona
Solar magnetic reconnection
url https://doi.org/10.3847/1538-4357/ada951
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AT zwma solarcoronalmassejectionandpostcoronalmassejectionblobformationintwofluidsimulations