European Solar Physics Online Seminar Archive

Following an initiative by the University of Oslo the MPS will participate in the "European Solar Physics Online Seminar" series (ESPOS). Details can be found here: https://folk.uio.no/tiago/espos/
The aim of this video conference series is to promote ideas more widely with a specialized audience, and give some exposure to cutting-edge research for students and other young researchers that do not regularly travel to conferences. The ESPOS series is planned to take place every second Thursday at 11am.
Solar observations offer both a rich interdisciplinary laboratory on fundamental astrophysics and precious tools for Space Weather applications. The involved plasma processes determine a complex radio ... [more]
We present high spatial resolution narrow-band images in three different chromospheric spectral lines, including Ca II K with the new CHROMospheric Imaging Spectrometer installed at the Swedish 1-m ... [more]
The ubiquitous presence of small magnetic elements in the Quiet Sun represents a prominent coupling between the photosphere and the upper layers of the Sun’s atmosphere. Small magnetic element ... [more]

ESP Online Seminar: 3D Whole-Prominence Fine Structure models: the current state of the affairs (Stanislav Gunár )

ESPOS
To understand the links between the distribution of the prominence plasma, the configuration of its magnetic field and the observations of prominence/filament fine structures obtained in UV/EUV ... [more]

ESP Online Seminar: The Sun from Coimbra: history, recent results and perspectives (João Fernandes)

ESPOS
The Astronomical Observatory of the Coimbra University has a collection of solar observations on a daily basis, since 1926. We obtain regular observations of the full solar disk using a classical ... [more]

ESP Online Seminar: 2D and 3D Kinematic Analysis of an Ideal-MHD Prominence Eruption (Thomas Rees-Crockford)

ESPOS
We carry out multi-dimensional kinematic analysis of a prominence eruption in order to characterise the role of eruptive ideal-MHD instabilities. Using SDO/AIA and STEREO/EUVI-A we reconstruct the ... [more]
Since the work of Carlin et al. (2012), more studies have investigated, with the help of MHD models of the solar chromosphere, the behavior of scattering linear polarization (LP) in presence of ... [more]

ESP Online Seminar: Swirls and Alfvén pulses in the Solar Atmosphere (JiaJia Liu)

ESPOS

ESP Online Seminar: The largest flares of solar cycle 24 as potential clues for stellar superflares (Paolo Romano)

ESPOS

ESP Online Seminar: Eruptions and flaring activity in emerging quadrupolar regions (Petros Syntelis)

ESPOS

ESP Online Seminar: MHD wave modes in the solar magnetic flux tubes with elliptical cross-section (Anwar Ali Aldhafeeri)

ESPOS

ESP Online Seminar: Spectral diagnostics of cool flare loops observed by SST (Julius Koza)

ESPOS

ESP Online Seminar: Penumbral brightening events (Mariarita Murabito)

ESPOS

ESP Online Seminar: Solar irradiance variability and surface magnetism (Kok Leng Yeo)

ESPOS
The variation in solar irradiance is commonly assumed to be driven by its surface magnetism. Until recently, this assumption could not be verified conclusively as models of solar irradiance ... [more]
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