Lauren Doyle
Observations and 3D Magnetohydrodynamic Modeling of a Confined Helical Jet Launched by a Filament Eruption
Doyle, Lauren; Wyper, Peter F.; Scullion, Eamon; McLaughlin, James A.; Ramsay, Gavin; Doyle, J. Gerard
Authors
Dr Peter Wyper peter.f.wyper@durham.ac.uk
Associate Professor
Eamon Scullion
James A. McLaughlin
Gavin Ramsay
J. Gerard Doyle
Abstract
We present a detailed analysis of a confined filament eruption and jet associated with a C1.5 class solar flare. Multiwavelength observations from the Global Oscillations Network Group and Solar Dynamics Observatory reveal the filament forming over several days following the emergence and then partial cancellation of a minority polarity spot within a decaying bipolar active region. The emergence is also associated with the formation of a 3D null point separatrix that surrounds the minority polarity. The filament eruption occurs concurrently with brightenings adjacent to and below the filament, suggestive of breakout and flare reconnection, respectively. The erupting filament material becomes partially transferred into a strong outflow jet (∼60 km s−1 ) along coronal loops, becoming guided back toward the surface. Utilizing high-resolution Hα observations from the Swedish Solar Telescope/CRisp Imaging SpectroPolarimeter, we construct velocity maps of the outflows, demonstrating their highly structured but broadly helical nature. We contrast the observations with a 3D magnetohydrodynamic simulation of a breakout jet in a closed-field background and find close qualitative agreement. We conclude that the suggested model provides an intuitive mechanism for transferring twist/helicity in confined filament eruptions, thus validating the applicability of the breakout model not only to jets and coronal mass ejections but also to confined eruptions and flares.
Citation
Doyle, L., Wyper, P. F., Scullion, E., McLaughlin, J. A., Ramsay, G., & Doyle, J. G. (2019). Observations and 3D Magnetohydrodynamic Modeling of a Confined Helical Jet Launched by a Filament Eruption. Astrophysical Journal, 887(2), Article 246. https://doi.org/10.3847/1538-4357/ab5d39
Journal Article Type | Article |
---|---|
Acceptance Date | Nov 26, 2019 |
Online Publication Date | Dec 26, 2019 |
Publication Date | Dec 20, 2019 |
Deposit Date | Jan 15, 2020 |
Publicly Available Date | Jan 15, 2020 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 887 |
Issue | 2 |
Article Number | 246 |
DOI | https://doi.org/10.3847/1538-4357/ab5d39 |
Public URL | https://durham-repository.worktribe.com/output/1278888 |
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