Source Region and Launch Characteristics of Magnetic-arch-blowout Solar Coronal Mass Ejections Driven by Homologous Compact-flare Blowout Jets

Source Region and Launch Characteristics of Magnetic-arch-blowout Solar Coronal Mass Ejections Driven by Homologous Compact-flare Blowout Jets

We study the formation of four coronal mass ejections (CMEs) originating from homologous blowout jets. All of the blowout jets originated from NOAA Active Region (AR) 11515 on 2012 July 2, within a time interval of ≈14 hr. All of the CMEs were wide (angular widths ≈ 95°–150°), and propagated with sp...

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Bibliographic Details
Main Authors: Binal D. Patel, Bhuwan Joshi, Alphonse C. Sterling, Ronald L. Moore
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar coronal mass ejections
Solar active regions
Solar active region filaments
Solar flares
Solar coronal transients
Solar magnetic fields
Online Access:https://doi.org/10.3847/1538-4357/ad4995

Internet

https://doi.org/10.3847/1538-4357/ad4995

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