Formation of a rotating jet during the filament eruption on 10-11 April 2013
arXiv:1505.01615 · doi:10.1093/mnras/stv1039
Abstract
We analyze multi-wavelength and multi-viewpoint observations of a helically twisted plasma jet formed during a confined filament eruption on 10-11 April 2013. Given a rather large scale event with its high spatial and temporal resolution observations, it allows us to clearly understand some new physical details about the formation and triggering mechanism of twisting jet. We identify a pre-existing flux rope associated with a sinistral filament, which was observed several days before the event. The confined eruption of the filament within a null point topology, also known as an Eiffel tower (or inverted-Y) magnetic field configuration results in the formation of a twisted jet after the magnetic reconnection near a null point. The sign of helicity in the jet is found to be the same as that of the sign of helicity in the filament. Untwisting motion of the reconnected magnetic field lines gives rise to the accelerating plasma along the jet axis. The event clearly shows the twist injection from the pre-eruptive magnetic field to the jet.
14 pages, 12 figures, to appear in MNRAS
References in corpus (4)
Cited by in corpus (14)
- On a solar blowout jet: driven mechanism and the formation of cool and hot components
- Three-Dimensional Simulations of Tearing and Intermittency in Coronal Jets
- 3He-Rich Solar Energetic Particles in Helical Jets on the Sun
- First direct observation of a torsional Alfvén oscillation at coronal heights
- Triggering mechanism and material transfer of a failed solar filament eruption
- Is flux rope a necessary condition for the progenitor of coronal mass ejections?
- Flux Rope Breaking and Formation of a Rotating Blowout Jet
- A Model for the Coupled Eruption of a Pseudostreamer and Helmet Streamer
- Kelvin--Helmholtz instability in a twisting solar polar coronal hole jet observed by \emph{SDO}/AIA
- Origin of Quasi-Periodic Pulsation at the Base of Kink Unstable Jet
- High mode magnetohydrodynamic waves propagation in a twisted rotating jet emerging from a filament eruption
- Formation and Thermodynamic Evolution of plasmoids in active region jets
- Covert connection of filaments
- How Rotating Solar Atmospheric Jets Become Kelvin--Helmholtz Unstable