Advances in the modelling and observation of the photosphere-corona interaction
chair: Paolo Pagano
› Plasma properties in the Quiet-sun of the Transition Region - Yamini Rao, DAMTP, Cambridge University
14:00-14:15 (15min)
› Diffuse solar coronal features originating from highly structured spicular footpoints - Nikolina Milanovic, Max Planck Institute for Solar System Research
14:15-14:30 (15min)
› Measuring the Photospheric Driving of Magnetic Footpointswith Quantifiable Uncertainties (invited) - Raphael Attie, NASA/GSFC
14:30-15:00 (30min)
› Undetected Minority-polarity Flux as the Missing Link in Coronal Heating - Yi-Ming Wang, National Research Laboratory
15:00-15:15 (15min)
Advances in the modelling and observation of the photosphere-corona interaction
chair: Paolo Pagano
› A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method - Craig Johnston, George Mason University [Fairfax], GSFC Heliophysics Science Division
16:30-16:45 (15min)
› Flows in Enthalpy Based Thermal Evolution of Loops - Abhishek Rajhans, Inter University Centre for Astronomy and Astrophysics, Pune
16:45-17:00 (15min)
› On the assessment of the damping mechanism for transverse coronal loop oscillations - Inigo Arregui, Instituto de Astrofisica de Canarias
09:00-09:15 (15min)
› Decayless kink oscillations detected with AIA and EUI - Valery Nakariakov, University of Warwick
09:15-09:30 (15min)
› Decay-less loop oscillations generated by steady-flow drivers - Konstantinos Karampelas, CmPA, KU Leuven, University of Northumbria
09:30-09:45 (15min)
› On the decayless transverse oscillations in active region coronal loops: Observations from Solar Orbiter/ EUI - Sudip Mandal, Max Planck Institute for Solar System Research
09:45-10:00 (15min)
› Simulating the FIP effect in coronal loops using a multi-species kinetic-fluid model - Nicolas Poirier, Institut de recherche en astrophysique et planétologie
11:30-11:45 (15min)
› Coronal abundance diagnostics with EIS and SPICE - Eric Buchlin, Institut d'astrophysique spatiale
11:45-12:00 (15min)
› Electron densities from Fe XIII EUV and IR lines - Jaroslav Dudik, Astronomical Institute of the Czech Academy of Sciences
12:00-12:15 (15min)
› Non-equilibrium processes and opacity in solar active region cores - Giulio Del Zanna, University of Cambridge
14:00-14:15 (15min)
› Physical properties of active region upflows - Pascal Démoulin, Laboratoire Cogitamus, Laboratoire d\'études spatiales et dínstrumentation en astrophysique
14:15-14:30 (15min)
› Single and Multiple Vantage Point 3D Coronal Reconstruction with the CROBAR Method - Joseph Plowman, Southwest Research Institute [Boulder]
14:30-14:45 (15min)
› A review of small scale current sheets and coronal heating (invited) - Thomas Howson, University of St. Andrews
16:30-17:00 (30min)
› EUV MUSE diagnostics of heating release from MHD loop modeling - Fabio Reale, INAF - Osservatorio Astronomico di Palermo, Università degli studi di Palermo - University of Palermo
17:00-17:15 (15min)
› Observational and numerical characterization of a wave-like front propagating along a coronal fan - Valeria Sieyra, Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven
17:15-17:30 (15min)
› Loop heating by non-linear damping of transverse waves - Tom Van Doorsselaere, KULeuven
17:30-17:45 (15min)
› 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)
› Multi-scale manifestations of thermal non-equilibrium in coronal loops (invited) - Clara Froment, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E)
09:00-09:30 (30min)
› The role of thermal instability in thermal non-equilibrium - Ramon Oliver, University of the Balearic Islands
09:30-09:45 (15min)
› Prevalence of Thermal Non-Equilibrium over an Active Region - Seray Sahin, University of Northumbria
09:45-10:00 (15min)
› Simulations of Thermal Non-Equilibrium Caused by Nanoflares - Therese Kucera, NASA Goddard Space Flight Center
10:00-10:15 (15min)