15–20 Mar 2026
Berlin
Europe/Berlin timezone
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Session

Dynamos, production and the evolution of the magnetic field

1
16 Mar 2026, 09:15
Harnack Haus (Berlin)

Harnack Haus

Berlin

Presentation materials

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  1. Matthias Rempel (High Altitude Observatory, NSF National Center for Atmospheric Research)
    16/03/2026, 09:15
    Invited talk

    First Name: Matthias
    Last Name: Rempel
    Email Address: rempel@ucar.edu
    Affiliation: High Altitude Observatory, NSF National Center for Atmospheric Research

    All 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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  2. Adam Finley (ESA/ESTEC)
    16/03/2026, 09:35
    Contributed talk

    First Name: Adam
    Last Name: Finley
    Email Address: adam.finley.astro@gmail.com
    Affiliation: ESA/ESTEC

    All 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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  3. Hanna Strecker (Instituto de Astrofísica de Andalucía (IAA-CSIC))
    16/03/2026, 09:50
    Contributed 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, Spain

    All 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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  4. Jie Jiang (Beihang University, China)
    16/03/2026, 10:05
    Review talk

    First Name: Jie
    Last Name: Jiang
    Email Address: jiejiang@buaa.edu.cn
    Affiliation: Beihang University, China

    All 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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