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.

ESP Online Seminar: Magnetic Rayleigh–Taylor Unstable Plumes and Hybrid KH-RT Instability into a Loop-like Eruptive Prominence (Sudheer K. Mishra)

ESPOS
The magnetic Rayleigh–Taylor instability is a fundamental MHD instability and recent observations show that this instability develops in the solar prominences. We analyze the observations from Solar ... [more]

ESP Online Seminar: Learning to Invert Solar Flares with RADYN Physics

ESPOS
During a solar flare, it is believed that reconnection takes place in the corona followed by fast energy transport to the chromosphere. The resulting intense heating strongly disturbs the ... [more]

ESP Online Seminar: Learning to Invert Solar Flares with RADYN Physics

ESPOS
During a solar flare, it is believed that reconnection takes place in the corona followed by fast energy transport to the chromosphere. The resulting intense heating strongly disturbs the ... [more]

ESP Online Seminar: Magnetic properties of short-lived penumbral microjets (Azaymi Litzi Siu Tapi)

ESPOS
Studying the polarization properties of penumbral microjets that have the shortest durations requires spectropolarimetric observations with the fastest temporal cadence possible and is currently a ... [more]

ESP Online Seminar: Solar Flare Prediction Using Magnetic Field Diagnostics Above the Photosphere (Marianna Korsos)

ESPOS
We present the application of the weighted horizontal gradient of magnetic field (WGM) flare prediction method to 3D extrapolated magnetic configurations of flaring solar ARs. The main aim is to ... [more]

ESP Online Seminar: Understanding hooks of solar flare ribbons and the evolution of coronal mass ejections (Juraj Lorinčík)

ESPOS
Solar flares and eruptions are one of the most energetic phenomena occuring in the solar system. They are typically described by the cartoon-like 2D Standard model of solar flares. This model is ... [more]

ESP Online Seminar: Study of damping of propagating kink waves in the solar corona (Ajay Tiwari)

ESPOS
Propagating kink waves have been reported recently and have been found to be ubiquitous in the solar corona including in the quiet Sun. It is imperative to understand the mechanisms that enable their ... [more]
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