High-resolution SST continuum observations of two white-light flares across the Paschen jump show >40% enhancements co-temporal with HXR, yet a blue/red ratio below one that conflicts with accepted WL formation mechanisms.
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3 Pith papers cite this work, alongside 308 external citations. Polarity classification is still indexing.
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Data-constrained 3D modeling of the 2011 August 4 flare reveals strong polarity asymmetry in electron precipitation driven by magnetic mirror ratios, with turbulent scattering and Coulomb collisions modulating the energy-dependent flux.
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.
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Investigating white-light flare mechanisms via the Paschen jump using high-resolution continuum observations from the Swedish 1-m Solar Telescope
High-resolution SST continuum observations of two white-light flares across the Paschen jump show >40% enhancements co-temporal with HXR, yet a blue/red ratio below one that conflicts with accepted WL formation mechanisms.
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Data-Constrained Modeling of Electron Transport and Asymmetric Precipitation in the 2011 August 4 Solar Flare
Data-constrained 3D modeling of the 2011 August 4 flare reveals strong polarity asymmetry in electron precipitation driven by magnetic mirror ratios, with turbulent scattering and Coulomb collisions modulating the energy-dependent flux.
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Transport of electrons in tangled magnetic fields
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.