collaborators

14 papers

astro-ph.SR2026

The DIRECD coronal mass ejection direction catalog: three-dimensional propagation inferred from coronal dimmings

Shantanu Jain, Tatiana Podladchikova, Karin Dissauer +2

Coronal mass ejections (CMEs) are among the primary drivers of space weather disturbances at Earth, yet their early propagation in the low corona remains poorly constrained owing t…

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

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.IM2026

Stellar Coronal Mass Ejections with HWO: A Science Case Concept

R. O. Parke Loyd, James Paul Mason, Ivey Davis +3

The primary mission of the Habitable World Observatory (HWO) will be to constrain the prevalence of life on Earth-like planets. These planets will be subject to impacts by energeti…

astro-ph.SR2026

The Role of Reconnection at Magnetic Separators in Complex Solar Flare Ribbons

Graham Barnes, Karin Dissauer

Solar flare ribbons, manifesting as transient brightenings in the chromosphere, are believed to trace out the footpoints of magnetic field lines that are reconnecting higher in the…

astro-ph.SR2026

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).…