Insights into the Kinematic Evolution of Filament-Induced Jets: Coupling of Interchange and Flare Reconnection
arXiv:2610.39253 · doi:10.3847/1538-4357/aeab9b
Abstract
Jets are ubiquitous eruptive activities in the solar atmosphere, playing an important role in mass transport, atmospheric heating, and energy supply. However, the triggering mechanism remains elusive. To reveal the fine process of jet evolution, we study a jet associated with a B-class flare that involves in two distinct stages. Analyzing the complete evolution of a solar jet captured by the Solar Dynamics Observatory (SDO), we clearly identify its dual-stage kinematics, evolving from interchange to flare reconnection. This dual-stage jet is characterized by distinct dual-stage signatures in magnetic morphology, H profile, jet speed, jet height, X-ray flux, loop-top source, and temperature. These differences are naturally unified by a physical picture coupling interchange and flare reconnection, offering new insights into understanding of the physical process of filament-induced jets.
arXiv comment10 pages, 5 figures
References in corpus (49)
- Fast Reconnection in High-Lundquist-Number Plasmas Due to Secondary Tearing Instabilities
- Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
- Plasmoid-Induced-Reconnection and Fractal Reconnection
- Fast magnetic reconnection in the plasmoid-dominated regime
- Differential Emission Measures from the Regularized Inversion of Hinode and SDO data
- Small-scale filament eruptions as the driver of solar coronal hole X-ray jets
- Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere
- Differential Emission Measure Analysis of Multiple Structural Components of Coronal Mass Ejections in the Inner Corona
- Plasmoid Ejections and Loop Contractions in an Eruptive M7.7 Solar Flare: Evidence of Particle Acceleration and Heating in Magnetic Reconnection Outflows
- Giant Chromospheric Anemone Jet Observed with Hinode and Comparison with Magnetohydrodynamic Simulations: Evidence of Propagating Alfven Waves and Magnetic Reconnection
- Plasma Jets and Eruptions in Solar Coronal Holes: a 3D flux emergence experiment
- Fan-spine topology formation through two-step reconnection driven by twisted flux emergence
- A fundamental mechanism of solar eruption initiation
- A Breakout Model for Solar Coronal Jets with Filaments
- Magnetic reconnection between a solar filament and nearby coronal loops
- Simultaneous observation of a flux rope eruption and magnetic reconnection during an X-class solar flare
- Interchange reconnection as the source of the fast solar wind within coronal holes
- A Cancellation Nanoflare Model for Solar Chromospheric and Coronal Heating
- Blobs in recurring EUV jets
- Frequently Occurring Reconnection Jets from Sunspot Light Bridges
- A standard-to-blowout jet
- Picoflare jets power the solar wind emerging from a coronal hole on the Sun
- A model for straight and helical solar jets: II. Parametric study of the plasma beta
- Rotating Solar Jets in Simulations of Flux Emergence with Thermal Conduction
- Evidence For The Magnetic Breakout Model in an Equatorial Coronal-Hole Jet
- Particle Acceleration at a Flare Termination Shock: Effect of Large-scale Magnetic Turbulence
- Triggering mechanism and material transfer of a failed solar filament eruption
- From Pseudostreamer Jets to CMEs: Observations of the Breakout Continuum
- Physical properties of solar polar jets: A statistical study with Hinode XRT data
- Blowout Jets and Impulsive Eruptive Flare in a Bald-Patch Topology
- A Magnetic Reconnection model for Hot Explosions in the Cool Atmosphere of the Sun
- Flux Rope Breaking and Formation of a Rotating Blowout Jet
- A solar blowout jet caused by the eruption of a magnetic flux rope
- A highly dynamic small-scale jet in a polar coronal hole
- Another Look at Erupting Minifilaments at the Base of Solar X-Ray Polar Coronal "Standard" and "Blowout" Jets
- The role of small-scale surface motions in the transfer of twist to a solar jet from a remote stable flux rope
- Resolving the Fan-Spine Reconnection Geometry of a Small-Scale Chromospheric Jet Event with the New Solar Telescope
- Dynamics evolution of a solar active-region filament from quasi-static state to eruption: rolling motion, untwisting motion, material transfer, and chirality
- Multi-stage reconnection powering a solar coronal jet
- Hi-C 2.1 Observations of Small-Scale Miniature-Filament-Eruption-Like Cool Ejections in Active Region Plage
- Power-law Distribution of Solar-Cycle Modulated Coronal Jets
- Thin coronal jets and plasmoid-mediated reconnection: Insights from Solar Orbiter observations and Bifrost simulations
- High-Resolution Observations of a Small-Scale Cancellation Nanoflare: Supporting Evidence for the Cancellation Nanoflare Model
- Theoretical Studies on the Evolution of Solar Filaments in Response to New Emerging Flux
- Magnetic flux cancellation in the solar atmosphere through 3D realistic numerical modeling
- Resolving Interchange Reconnection Dynamics in a Fan-Spine-like Topology Observed by Solar Orbiter
- A self-consistent 3D MHD model producing a solar blowout jet
- Bidirectional Plasma Jets Driven by Magnetic Reconnection: Observations by GST and SDO
- Repeated Sunspot Light Bridge Jets Associated with Slipping Base Brightenings