› Magnetic Reconnection in 3D vs. 2D and Dependency on Magnetic Shear - Lars K. S. Daldorff, CUA/NASA
09:00-09:15 (15min)
› (When) Can wave heating balance optically thin radiative losses in the corona? - Ineke De Moortel, Rosseland Centre for Solar Physics, University of Oslo, University of St. Andrews
09:15-09:30 (15min)
› Transverse MHD waves as signatures of braiding-induced magnetic reconnection in coronal loops - Ayu Ramada Sukarmadji, Northumbria University
09:30-09:45 (15min)
› Coronal heating studies with the Multi-slit Solar Explorer (MUSE) - Bart De Pontieu, Lockheed Martin Solar & Astrophysics Laboratory
10:00-10:15 (15min)
› Preliminary Results from the Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) - Amy Winebarger, NASA MSFC
10:15-10:30 (15min)
› Thermal properties of the smallest EUV brightenings observed with SolO/HRI-EUV and SDO/AIA. - Antoine Dolliou, Institut d'astrophysique spatiale
11:30-11:45 (15min)
› Narrowing down causality between coronal heating mechanisms and observations (invited) - Patrick Antolin, Northumbria University
11:45-12:15 (30min)
› Doppler Shifts and their Centre to Limb Variation in Transition Region - Durgesh Tripathi, IUCAA
14:00-14:15 (15min)
› Inferring quiet Sun heating using machine learning - Vishal Upendran, IUCAA
14:15-14:30 (15min)
› The 'coronal veil' hypothesis: evidence, implications, and future studies (invited) - Anna Malanushenko, National Center for Atmospheric Research [Boulder]
14:30-15:00 (30min)
› Cross Sections of Coronal Loop Flux Tubes - James Klimchuk, NASA Goddard Space Flight Center
15:00-15:15 (15min)
› Understanding the cross-field thermal structure of a coronal loop using slow magnetoacoustic waves - S. Krishna Prasad, Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven
16:30-16:45 (15min)
› Accelerated particle beams in a 3D simulation of the quiet Sun - Lars Frogner, Institute of Theoretical Astrophysics [Oslo], Rosseland Centre for Solar Physics
16:45-17:00 (15min)