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Damien Przybylski (Max Planck Institute for Solar System Research)16/03/2026, 14:10Review talk
First Name: Damien
Last Name: Przybylski
Email Address: przybylski@mps.mpg.de
Affiliation: Max Planck Institute for Solar System ResearchAll Authors: D. Przybylski
Abstract: The solar chromosphere presents a formidable modelling challenge. The coupling of the turbulent convection zone to the underlying magnetic field leads to it's highly dynamic nature, displaying spicules,...
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João da Silva Santos (National Solar Observatory (USA))16/03/2026, 14:40Contributed talk
First Name: João M.
Last Name: da Silva Santos
Email Address: jdasilvasantos@nso.edu
Affiliation: National Solar Observatory (USA)All Authors: Joshua Bentley, Serena Criscuoli, Tom Schad, Momchil Molnar, Alex Pietrow, Bart De Pontieu, Juan Martinez-Sykora
Abstract: Single-peak Mg II h&k profiles are commonly observed in solar plage regions, and they are known to indicate hot,...
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Patrick Ondratschek (Max Planck Institute for Solar System Research)16/03/2026, 14:55Poster
First Name: Patrick
Last Name: Ondratschek
Affiliation: Max Planck Institute for Solar System ResearchAll Authors: P. Ondratschek, D. Przybylski, H.N. Smitha, R. Cameron, S. K. Solanki
Abstract: The Mg II h&k lines are well-suited to study the solar chromosphere. Forming under non-local thermodynamic equilibrium conditions, the line formation of these lines is complicated and not...
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Jayant Joshi (Indian Institute of Astrophysics, Bengaluru)16/03/2026, 15:40Invited talk
First Name: Jayant
Last Name: Joshi
Email Address: jayant.joshi@iiap.res.in
Affiliation: Indian Institute of Astrophysics, BengaluruAll Authors: Jayant Joshi
Abstract: Recent high-resolution observations reveal that small-scale magnetic reconnection in the solar lower atmosphere, manifested as quiet-Sun Ellerman bombs (QSEBs), is far more ubiquitous than previously recognised,...
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Sanghita Chandra (Max Planck Institute for Solar System Research)16/03/2026, 16:00Contributed talk
First Name: Sanghita
Last Name: Chandra
Email Address: chandra@mps.mpg.de
Affiliation: Max Planck Institute for Solar System ResearchAll Authors: Sanghita Chandra, Robert Cameron, Damien Przybylski, Sami K. Solanki
Abstract: It has been suggested that spicules play a role in coronal heating, with reports of an association with transition region (e.g. Si IV emission) and coronal...
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Janmejoy Sarkar (Max Planck Institute for Solar System Research and IUCAA)16/03/2026, 16:15Contributed talk
First Name: Janmejoy
Last Name: Sarkar
Email Address: sarkarjj@mps.mpg.de
Affiliation: Max Planck Institute for Solar System Research and IUCAAAll Authors: Janmejoy Sarkar, VN Nived, Soumya Roy, Rahul Gopalakrishnan, Rushikesh Deogaonkar, Sreejith Padinhatteeri, Durgesh Tripathi, A.N. Ramaprakash, Achim Gandorfer, Sami Solanki.
Abstract: The Solar Ultraviolet Imaging Telescope...
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Kyuhyoun Cho (LMSAL / SETI)16/03/2026, 16:30Invited talk
First Name: Kyuhyoun
Last Name: Cho
Email Address: kcho@seti.org
Affiliation: LMSAL / SETIAll Authors: Bart De Pontieu, Paola Testa
Abstract: Nonthermal broadening in spectral lines formed in the solar transition region has been a subject of interest for several decades, as its underlying mechanisms remain unclear and it may provide key insights into the heating of the upper...
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Daye Lim (Royal Observatory of Belgium and KU Leuven)16/03/2026, 16:50Contributed talk
First Name: Daye
Last Name: Lim
Email Address: daye.lim@oma.be
Affiliation: Royal Observatory of Belgium and KU LeuvenAll Authors: Daye Lim, Tom Van Doorsselaere, Nancy Narang, Laura A. Hayes, Emil Kraaikamp, Aadish Joshi, Konstantina Loumou, Cis Verbeeck, David Berghmans, and Krzysztof Barczynski
Abstract: Small-scale extreme-ultraviolet (EUV) transient brightenings are...
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Tania Varesano (SWRI / CU Boulder)16/03/2026, 17:05Metcalf Award
First Name: Tania
Last Name: Varesano
Email Address: tania.varesano@colorado.edu
Affiliation: SWRI / CU BoulderAll Authors: Tania Varesano, Don Hassler, Yeimy Rivera, Joe Plowman
Abstract: The SPICE (Spectral Imaging of the Coronal Environment) and HIS (Heavy Ion Sensor) instruments on Solar Orbiter were designed to enable us to trace the source regions of elemental enrichment...
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