15–20 Mar 2026
Berlin
Europe/Berlin timezone
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Session

Magnetic field & impact on irradiance, atmosphere, etc.

2
16 Mar 2026, 11:20
Harnack Haus (Berlin)

Harnack Haus

Berlin

Presentation materials

There are no materials yet.

  1. Theodosios Chatzistergos (Max Planck Institute for Solar System Research)
    16/03/2026, 11:20
    Review talk

    First Name: Theodosios
    Last Name: Chatzistergos
    Email Address: chatzistergos@mps.mpg.de
    Affiliation: Max Planck Institute for Solar System Research, Göttingen, Germany

    All Authors: Theodosios Chatzistergos

    Abstract: Because direct measurements of solar irradiance exist only from the late 1970s onward, models are required to reconstruct earlier irradiance variations. On...

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  2. Xiang Li (Max Planck Institute for Solar System Research)
    16/03/2026, 11:50
    Contributed talk

    First Name: Xiang
    Last Name: Li
    Email Address: lixiang@mps.mpg.de
    Affiliation: Max Planck Institute for Solar System Research

    All Authors: Xiang Li, Gherardo Valori, Daniele Calchetti, Sami K. Solanki, Johann Hirzberger, Jonas Sinjan

    Abstract: The solar vector magnetic field is inferred from spectropolarimetric observations of the polarization in magnetically sensitive spectral...

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  3. Nancy Narang (Royal Observatory of Belgium)
    16/03/2026, 12:05
    Contributed talk

    First Name: Nancy
    Last Name: Narang
    Email Address: nancy.narang@oma.be
    Affiliation: Royal Observatory of Belgium

    All Authors: Nancy Narang, Cis Verbeeck, David Berghmans, Marilena Mierla, Susanna Parenti, Pradeep Chitta, Daniele Calchetti, Frederic Auchere

    Abstract: The extreme-ultraviolet (EUV) brightenings identified by Solar Orbiter, commonly known as “campfires”, are one of...

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  4. Milan Gosic (LMSAL/SETI)
    16/03/2026, 13:35
    Invited talk

    First Name: Milan
    Last Name: Gosic
    Email Address: mgosic.solar@gmail.com
    Affiliation: LMSAL/SETI

    All Authors: Milan Gosic

    Abstract: The quiet regions of the solar surface are densely populated with small and weak magnetic flux patches. These patches contain an amount of magnetic flux comparable to what is found in active regions during the peak of the solar cycle. This suggests...

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  5. Jonas Sinjan (Max Planck Institute for Solar System Research)
    16/03/2026, 13:55
    Contributed talk

    First Name: Jonas
    Last Name: Sinjan
    Affiliation: Max Planck Institute for Solar System Research

    All Authors: Jonas Sinjan, Johann Hirzberger, Daniele Calchetti, Gherardo Valori, Xiaohong Li, Sami K. Solanki and the PHI team

    Abstract: Active regions are the source region for the most energetic phenomena on the Sun. Maps of active regions’ photospheric magnetic fields, and derived...

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