Determining the 3D Dynamics of Solar Flare Magnetic Reconnection
Top Cited Papers
Open Access
- 22 October 2025
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 993 (1) , 31
Abstract
Solar flares are major space weather events that result from the explosive conversion of stored magnetic energy into bulk motion, plasma heating, and particle acceleration. While the standard flare model has proven highly successful in explaining key morphological features of flare observations, many aspects of the energy release are not yet understood. In particular, the turbulent three-dimensional structure of the flare current sheet is thought to play an important role in fast reconnection, particle acceleration, and bursty dynamics. Although direct diagnosis of the magnetic field dynamics in the corona remains highly challenging, rich information may be gleaned from flare ribbons, which represent the chromospheric imprints of reconnection in the corona. Intriguingly, recent solar imaging observations have revealed a diversity of fine structure in flare ribbons that hints at corresponding complexity in the reconnection region. We present high-resolution three-dimensional magnetohydrodynamics simulations of an eruptive flare and describe our efforts to interpret fine-scale ribbon features in terms of the current sheet dynamics. In our model, the current sheet is characterized by many coherent magnetic structures known as plasmoids. We derive a model analog for ribbons by generating a time series of field-line length maps ( L -maps) and identifying abrupt shortenings as flare reconnection events. We thereby demonstrate that plasmoids imprint transient “spirals” along the analog of the ribbon front, with a morphology consistent with observed fine structure. We discuss the implications of these results for interpreting SolO, Interface Region Imaging Spectrograph, and Daniel K. Inouye Solar Telescope observations of explosive flare energy release.Keywords
All Related Versions
Funding Information
- NASA ∣ Science Mission Directorate (80NSSC21K1313)
- NASA ∣ Science Mission Directorate (80NSSC23K1065)
- NASA ∣ Science Mission Directorate (80NSSC23K0414)
- National Science Foundation (AST-2407849)
- National Science Foundation (AGS-2401228)
- UKRI ∣ Science and Technology Facilities Council (ST/W00108X/1)
- NASA ∣ Science Mission Directorate (80NSSC24K0608)
This publication has 111 references indexed in Scilit:
- A model for stealth coronal mass ejectionsJournal of Geophysical Research: Space Physics, 2016
- The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)Solar Physics, 2011
- The Solar Dynamics Observatory (SDO)2011
- An Instrument to Measure Coronal Emission Line PolarizationSolar Physics, 2008
- Slip-Running Reconnection in Quasi-Separatrix LayersSolar Physics, 2006
- Analysis of Magnetic Shear in An X17 Solar Flare on October 28, 2003Solar Physics, 2006
- Theory of radio pulsations in coronal loopsSolar Physics, 1987
- Non-thermal processes in large solar flaresSolar Physics, 1976
- Magnetic reconnection in the corona and the loop prominence phenomenonSolar Physics, 1976
- Theoretical model of flares and prominencesSolar Physics, 1974