DKIST VBI observations identify 30 spicule events triggered by microfilaments as small as 0.17 Mm, revealing two morphological classes and occasional twisting motions.
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A 2D AMR solar atmosphere model with 1.25 km cells in the transition region yields a converged 1.2x O VI non-equilibrium intensity enhancement over equilibrium, while Doppler and nonthermal widths still miss observed values.
A synthesis of large-scale coronal dynamics and small-scale solar transients as potential precursors to magnetic switchbacks, with pros/cons evaluation and terminology clarification.
Derives polarization-dependent damping and heating rates for Alfvénic waves in two-fluid weakly ionized plasmas and simulates nonlinear ponderomotive effects and collisional dissipation.
citing papers explorer
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Observational Evidence of Solar Spicules Associated with Microfilament Eruptions Using DKIST
DKIST VBI observations identify 30 spicule events triggered by microfilaments as small as 0.17 Mm, revealing two morphological classes and occasional twisting motions.
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Potential Solar Precursors to Magnetic Switchbacks
A synthesis of large-scale coronal dynamics and small-scale solar transients as potential precursors to magnetic switchbacks, with pros/cons evaluation and terminology clarification.
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Propagation of waves in weakly ionized two-fluid plasmas. II. Nonlinear Alfv\'enic waves
Derives polarization-dependent damping and heating rates for Alfvénic waves in two-fluid weakly ionized plasmas and simulates nonlinear ponderomotive effects and collisional dissipation.