activity
20162026
most citedUnderstanding the Physical Nature of Coronal "EIT Waves"

92 citations · 232 across the 37 of their papers we have counts for

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Showing 2026Show all

7 papers · 1 filter

astro-ph.SR2026

DEM analysis of the 6 September 2011 large-scale coronal wave

Amaia Razquin, Astrid M. Veronig, Karin Dissauer

Large-scale coronal waves are globally propagating intensity enhancements in extreme-ultraviolet (EUV) and soft X-ray (SXR) observations, associated with solar flares and coronal m…

astro-ph.SR2026

Chromospheric magnetic field extrapolations reveal the flux-rope configuration of a solar filament

Robert Jarolim, João M. da Silva Santos, Matthias Rempel +5

Solar eruptions are powered by the release of magnetic energy stored in the lower solar atmosphere, but the pre-eruptive magnetic configuration of filament channels remains difficu…

astro-ph.SR2026

Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool

Markus Baumgartner-Steinleitner, Astrid M. Veronig, Karin Dissauer +1

We investigate the two-dimensional velocity field of the fast and complex large-scale coronal wave observed on September 6, 2011. We use both a classical perturbation profile appro…

astro-ph.SR2026

A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy

Valeriy Vasilyev, Alexander I. Shapiro, Nadiia Kostogryz +10

TRAPPIST-1 is an ultra-cool dwarf that flares frequently. These flares shape the surrounding planets' high-energy irradiation environments, with consequences for atmospheric chemis…

astro-ph.SR2026★ 1 cited

Multi-Viewpoint Observation of a Failed Prominence Eruption on the Sun

Tingyu Gou, Katharine K. Reeves, Peter R. Young +5

Solar eruptions are sudden ejections of coronal mass and magnetic fields accompanied by intense energy release. The eruptive structure does not always erupt successfully, but somet…

astro-ph.SR2026★ 1 cited

Magnetic flux systems involved in the May 2024 solar energetic events from AR 13664 inferred through coronal dimmings

Amaia Razquin, Karin Dissauer, Astrid M. Veronig +1

Coronal dimmings are transient depletions of coronal plasma observed in extreme ultraviolet and soft X-rays, interpreted as low-corona signatures of coronal mass ejections (CMEs).…

astro-ph.SR2026

Neural blind deconvolution to reconstruct high-resolution ground-based solar observations

Christoph Schirninger, Robert Jarolim, Astrid M. Veronig +2

Ground-based solar observations enable unprecedented spatial, spectral, and temporal resolution of the lower solar atmosphere, yet Earths turbulent atmosphere imposes significant l…