15–20 Mar 2026
Berlin
Europe/Berlin timezone
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Session

Coronal structure and dynamics

5
17 Mar 2026, 11:35
Harnack Haus (Berlin)

Harnack Haus

Berlin

Presentation materials

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  1. Lakshmi Pradeep Chitta (Max Planck Institute for Solar System Research)
    17/03/2026, 11:35
    Review talk

    First Name: Lakshmi Pradeep
    Last Name: Chitta
    Email Address: chitta@mps.mpg.de
    Affiliation: Max Planck Institute for Solar System Research

    All Authors: Lakshmi Pradeep Chitta

    Abstract: The outer solar atmosphere, the million-Kelvin degree hot corona, is intricately governed by the magnetic field. The diverse magnetic landscape in the solar surface results in an equally diverse...

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  2. Phillip Hess (US Naval Research Laboratory)
    17/03/2026, 12:05
    Contributed talk

    First Name: Phillip
    Last Name: Hess
    Email Address: phillip.n.hess2.civ@us.navy.mil
    Affiliation: US Naval Research Laboratory

    All Authors: Phillip Hess, Robin Colaninno, Angelos Vourlidas, Guillermo Stenborg, Evangelos Paouris, Erika Palmerio, Russell Howard, Eleni Nikou

    Abstract: As the Solar Orbiter spacecraft moves out of the ecliptic plane, remote sensing observations are...

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  3. Clara Froment (LPC2E/CNRS)
    17/03/2026, 12:20
    Contributed talk

    First Name: Clara
    Last Name: Froment
    Email Address: clara.froment@cnrs-orleans.fr
    Affiliation: LPC2E/CNRS

    All Authors: Clara Froment and Sophie Masson

    Abstract: We report the detection of thermal non-equilibrium (TNE) cycles in a pseudo-streamer observed with SDO/AIA. TNE is an ubiquitous mechanism in the solar atmosphere, especially in coronal loops. These evaporation and...

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  4. Cosima Breu (University of Graz)
    17/03/2026, 13:50
    Invited talk

    First Name: Cosima
    Last Name: Breu
    Email Address: brecosima.breu@uni-graz.at
    Affiliation: University of Graz

    All Authors: Cosima Breu

    Abstract: A large part of the solar -and possibly stellar- corona is made up of closed magnetic loops containing hot and bright plasma. The exact physical mechanism leading to the heating of the plasma is still unclear. Numerous scaling laws have...

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  5. Sudip Mandal (Max Planck Institute for Solar System Research)
    17/03/2026, 14:10
    Contributed talk

    First Name: Sudip
    Last Name: Mandal
    Email Address: mandals@mps.mpg.de
    Affiliation: Max Planck Institute for Solar System Research, Germany

    All Authors: Sudip Mandal, Hardi Peter, Cosima Breu, Lakshmi Pradeep Chitta, Patrick Antolin, Sami K Solanki, and the EUI team

    Abstract: Decayless kink oscillations are ubiquitous in solar loops. Since these oscillations do not exhibit the...

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  6. Adriana De-Sassi (ETH Zürich)
    17/03/2026, 14:25
    Poster

    "Coronal dimmings, also called transient coronal holes, are well documented following eruptions (e.g. Veronig et al. 2025). Between 17 and 18 March 2022, a coordinated Solar Orbiter–Hinode–IRIS campaign monitored the formation of a coronal dimming following a filament eruption (Ngampoopun et al. 2023).
    We investigate whether the eruption produced a coronal-hole-like behaviour in the initially...

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  7. Antoine Dolliou (Max Planck Institute for Solar System Research)
    17/03/2026, 14:40
    Contributed talk

    First Name: Antoine
    Last Name: Dolliou
    Email Address: dolliou@mps.mpg.de
    Affiliation: MPS

    All Authors: H. Peter, S. Mandal, P. Chitta, L. Teriaca, Y. Chen, D. Calchetti

    Abstract: Network loops are a common feature in the quiet Sun, and the processes sustaining their energy budget are still not fully understood. In this work, our aim is to find signatures of the heating...

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  8. Tanmoy Samanta (Indian Institute of Astrophysics)
    17/03/2026, 14:55
    Invited talk

    First Name: Tanmoy
    Last Name: Samanta
    Email Address: tanmoy.samanta@iiap.res.in
    Affiliation: Indian Institute of Astrophysics, Bangalore, India

    All Authors: Tanmoy Samanta

    Abstract: Small-scale transients, including spicules, jets, and localized brightenings, are increasingly recognized as important contributors to mass and energy transport between the chromosphere and corona....

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  9. Vincenzo Andretta (INAF - Capodimonte Astronomical Observatory)
    17/03/2026, 15:15
    Contributed talk

    First Name: Vincenzo
    Last Name: Andretta
    Email Address: vincenzo.andretta@inaf.it
    Affiliation: INAF - Capodimonte Astronomical Observatory, Naples

    All Authors: Marco Romoli and the Metis Team

    Abstract: The Metis coronagraph on board Solar Orbiter is providing a new window into coronal dynamics through observations with exceptional temporal and spatial resolution. Its high...

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  10. Lucia Abbo (INAF - Astrophysical Observatory of Turin)
    17/03/2026, 16:00
    Contributed talk

    First Name: Lucia
    Last Name: Abbo
    Email Address: lucia.abbo@inaf.it
    Affiliation: INAF - Astrophysical Observatory of Turin

    All Authors: Lucia Abbo, Emanuele Amato, Vincenzo Andretta, David Berghmans, Riccardo Chiartano, Laurent Dolla, Silvano Fineschi, Alessandro Liberatore, Marilena Mierla, Marco Romoli, Daniele Spadaro, Roberto Susino, Luca Zangrilli, Joe Zender, Andrei...

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  11. Samantha Wallace (Embry-Riddle Aeronautical University)
    17/03/2026, 16:15
    Contributed talk

    First Name: Samantha
    Last Name: Wallace
    Email Address: samantha.wallace@erau.edu
    Affiliation: Embry-Riddle Aeronautical University

    All Authors: Samantha Wallace, Natalia Zambrana Prado, Nicholeen M. Viall, Peter Young, Therese A. Kucera, Susan T. Lepri, Stephanie L. Yardley, Vincenzo Andretta, David Lario, Spiro Antiochos, Charles N. Arge, Samuel J. Schonfeld, Carl J....

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  12. Bart De Pontieu (LMSAL)
    17/03/2026, 16:30
    Contributed talk

    First Name: Bart
    Last Name: De Pontieu
    Email Address: bdp@lmsal.com
    Affiliation: LMSAL

    All Authors: Bart De Pontieu, Mark Cheung, Juan Martinez-Sykora, Paola Testa, Amy Winebarger and the MUSE team

    Abstract: In this talk I will discuss the upcoming Multi-slit Solar Explorer (MUSE) mission, which is scheduled for launch in 2027. MUSE is a NASA MIDEX mission, composed of a...

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