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Matthias Rempel (High Altitude Observatory, NSF National Center for Atmospheric Research)16/03/2026, 09:15Invited talk
First Name: Matthias
Last Name: Rempel
Email Address: rempel@ucar.edu
Affiliation: High Altitude Observatory, NSF National Center for Atmospheric ResearchAll Authors: Matthias Rempel
Abstract: The Sun is a unique star in the sense that we can observe it at high resolution and study phenomena at a detail that is hidden in stellar observations. This applies specifically to...
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Adam Finley (ESA/ESTEC)16/03/2026, 09:35Contributed talk
First Name: Adam
Last Name: Finley
Email Address: adam.finley.astro@gmail.com
Affiliation: ESA/ESTECAll Authors: Adam J. Finley
Abstract: The repeated emergence of active regions in close proximity to one another creates long-lived sources of solar activity called active nests. These nests are thought to form due to non-axisymmetries in the generation and storage of the Sun's...
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Hanna Strecker (Instituto de Astrofísica de Andalucía (IAA-CSIC))16/03/2026, 09:50Contributed talk
First Name: Hanna
Last Name: Strecker
Email Address: streckerh@iaa.es
Affiliation: Instituto de Astrofísica de Andalucía (IAA-CSIC) and Spanish Space Solar Physics Consortium, Granada, SpainAll Authors: David Orozco Suárez; Instituto de Astrofísica de Andalucía (IAA-CSIC) and Spanish Space Solar Physics Consortium, Granada, Spain; Gherardo Valori; MPS Göttingen, Germany; Artem...
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Jie Jiang (Beihang University, China)16/03/2026, 10:05Review talk
First Name: Jie
Last Name: Jiang
Email Address: jiejiang@buaa.edu.cn
Affiliation: Beihang University, ChinaAll Authors: Jie Jiang
Abstract: Over 40 years of detailed solar magnetic field observations have shown that the original Babcock–Leighton (BL) dynamo scenario proposed in the 1960s could capture the essential physics of the global solar dynamo. That is the surface...
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