High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.
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Prominence emission in the G-band originates from Ti II and Ca I lines, not CH, and shows no clear ionization memory effect.
A weak global coronal shock accelerated 75-122 keV electrons locally where it hit quasi-perpendicular open fields in a dimming region, shown by EUV wavefront imaging and radio herringbone drift rates.
Multi-spacecraft study of the 2021 October 28 X1.0 flare and fast CME finds total energy release consistent with pre-event stored magnetic energy, with CME kinetic and potential energy dominating the budget.
A zero-beta MHD simulation of the 2024 May 6 event shows X-point reconnection above two current channels of opposite helicity deflects the erupting filament and forms the observed three-ribbon structure via QSLs in a sandwich magnetic configuration.
citing papers explorer
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A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.
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Prominence signatures in the Fraunhofer G-band; Testing ionization memory with multi-line prominence diagnostics
Prominence emission in the G-band originates from Ti II and Ca I lines, not CH, and shows no clear ionization memory effect.
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Signatures of localised particle acceleration at a global coronal shock wave
A weak global coronal shock accelerated 75-122 keV electrons locally where it hit quasi-perpendicular open fields in a dimming region, shown by EUV wavefront imaging and radio herringbone drift rates.
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Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption
Multi-spacecraft study of the 2021 October 28 X1.0 flare and fast CME finds total energy release consistent with pre-event stored magnetic energy, with CME kinetic and potential energy dominating the budget.
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Deflection of a Filament Eruption with Three Parallel Flare Ribbons via Reconnection at an X-Point
A zero-beta MHD simulation of the 2024 May 6 event shows X-point reconnection above two current channels of opposite helicity deflects the erupting filament and forms the observed three-ribbon structure via QSLs in a sandwich magnetic configuration.