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16th European Solar Physics Meeting

6–10 Sept 2021
Online
Europe/Rome timezone

Session

Poster Session 10.4

9 Sept 2021, 11:00
Online

Online

Conveners

Poster Session 10.4

  • Francesca Zuccarello (Istituto Nazionale di Astrofisica (INAF))

Presentation materials

Zoom link
  1. 164. Magnetoseismology for the solar corona: from ~10 Gauss to coronal magnetograms
    Zihao Yang (Peking University)
    09/09/2021, 11:00
    Session 3 - Fundamental Plasma Processes in the Solar Atmosphere: Magnetic Reconnection, Waves, Emission, Particle Acceleration
    Poster

    Magnetoseismology, a technique of magnetic field diagnostics based on observations of magnetohydrodynamic (MHD) waves, has been widely used to estimate the field strengths of oscillating structures in the solar corona. However, previously magnetoseismology was mostly applied to occasionally occurring oscillation events, providing an estimate of only the average field strength of an oscillating...

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  2. 202. MHD waves in chromospheric fibrillar structures as observed with ALMA
    Maryam Saberi (University of Oslo)
    09/09/2021, 11:13
    Session 3 - Fundamental Plasma Processes in the Solar Atmosphere: Magnetic Reconnection, Waves, Emission, Particle Acceleration
    Poster

    Waves and oscillations have been shown as a prime means of transporting energy through the solar atmosphere, thus, contributing to the high temperature of the upper layers. In particular, magnetohydrodynamic (MHD) waves are observed in a number of structures in the solar chromosphere, often with observations in the near-ultraviolet (UV) to infrared wavelength range. In this poster, we present...

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  3. 120. Polarity relevance in flux rope deflections triggered by coronal holes
    Abril Sahade (Instituto de Astronomía Teórica y Experimental)
    09/09/2021, 11:26
    Session 4 - From Radio to Gamma Rays: Near-Sun Manifestations and Triggering of Solar Flares and Coronal Mass Ejections
    Poster

    Usually coronal holes (CHs) deviate coronal mass ejections (CMEs) away from them. However, there are some peculiar events reported where the eruption travels towards the CH. To contribute to a space weather forecast efforts, in relation to the prediction of CME trajectories, we study the interaction between flux ropes (FRs) and CHs through numerical simulations. We perform 2.5D numerical...

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  4. 214. Flares Associated with Slowly Positively Drifting Bursts Observed in 800-2000 MHz
    Dr Alena Zemanova (Astronomical Institute, Czech Academy of Sciences)
    09/09/2021, 11:39
    Session 4 - From Radio to Gamma Rays: Near-Sun Manifestations and Triggering of Solar Flares and Coronal Mass Ejections
    Poster

    The slowly positively drifting bursts (SPDBs) can occur as a single burst or as a group and its frequency drift is usually less than 300 MHz s^-1. The origin of these burst is unknown and they are observed quite rarely. In our Ondrejov radiospectrograph archive we found up to 10 events during the period 2012-2015 and they are connected with flares. We picked 3 flares for the study. As the...

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