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Synthetic Remote-sensing and In Situ Observations of Fine-scale Structure in a Pseudostreamer Coronal Mass Ejection through the Solar Corona

Lynch, B. J.; Wyper, P. F.; Palmerio, E.; Casillas, L.; Dahlin, J. T.; Daldorff, L. K. S.; Guidoni, S. E.; Higginson, A. K.; Kumar, P.; Liberatore, A.; Liewer, P. C.; Panasenco, O.; Penteado, P.; Velli, M.

Synthetic Remote-sensing and In Situ Observations of Fine-scale Structure in a Pseudostreamer Coronal Mass Ejection through the Solar Corona Thumbnail


Authors

B. J. Lynch

E. Palmerio

L. Casillas

J. T. Dahlin

L. K. S. Daldorff

S. E. Guidoni

A. K. Higginson

P. Kumar

A. Liberatore

P. C. Liewer

O. Panasenco

P. Penteado

M. Velli



Abstract

Coronal pseudostreamer flux systems have a specific magnetic configuration that influences the morphology and evolution of coronal mass ejections (CMEs) from these regions. Here we continue the analysis of the Wyper et al. magnetohydrodynamic simulation of a CME eruption from an idealized pseudostreamer configuration through the construction of synthetic remote-sensing and in situ observational signatures. We examine the pre-eruption and eruption signatures in extreme ultraviolet and white light from the low corona through the extended solar atmosphere. We calculate synthetic observations corresponding to several Parker Solar Probe–like trajectories at ∼10R⊙ to highlight the fine-scale structure of the CME eruption in synthetic WISPR imagery and the differences between the in situ plasma and field signatures of flank and central CME-encounter trajectories. Finally, we conclude with a discussion of several aspects of our simulation results in the context of interpretation and analysis of current and future Parker Solar Probe data.

Citation

Lynch, B. J., Wyper, P. F., Palmerio, E., Casillas, L., Dahlin, J. T., Daldorff, L. K. S., Guidoni, S. E., Higginson, A. K., Kumar, P., Liberatore, A., Liewer, P. C., Panasenco, O., Penteado, P., & Velli, M. (2025). Synthetic Remote-sensing and In Situ Observations of Fine-scale Structure in a Pseudostreamer Coronal Mass Ejection through the Solar Corona. Astrophysical Journal, 277(2), Article 40. https://doi.org/10.3847/1538-4365/adb14e

Journal Article Type Article
Acceptance Date Jan 27, 2025
Online Publication Date Mar 19, 2025
Publication Date Apr 1, 2025
Deposit Date Apr 14, 2025
Publicly Available Date Apr 14, 2025
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 277
Issue 2
Article Number 40
DOI https://doi.org/10.3847/1538-4365/adb14e
Keywords Active solar corona, Solar filament eruptions, Solar flares, Solar coronal mass ejections, Solar coronal streamers, Interplanetary magnetic fields, Solar magnetic reconnection
Public URL https://durham-repository.worktribe.com/output/3738637

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