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.

ESPOS: European Solar Physics Online Seminar (Clara Froment)

ESPOS: ESPOS
[more]

ESPOS - European Solar Physics Online Seminar: Theoretical Foundation of 3D Alfven Resonances: Time Dependent Solutions (T. Elsden)

ESPOS
The coupling of fast and Alfven magnetohydrodynamic (MHD) waves is of fundamental interest in astrophysical plasmas. Under certain conditions, Alfven waves can be resonantly excited by fast mode ... [more]

ESP Online Seminar: Magnetic field variations associated with umbral flashes and penumbral waves (J. Joshi)

ESPOS
Oscillations in sunspots have been extensively studied for several decades. Most of the research conducted about sunspot oscillations has focussed around variations in Doppler velocities and ... [more]

ESP Online Seminar: Formation of the penumbra and start of the Evershed Flow (M. Murabito)

ESPOS
Penumbral formation is a significant part of the flux emergence process. Despite the new advanced techniques in observations and simulations, there are still processes that need to be clarified. In ... [more]

ESP Online Seminar: Deep Learning in Solar Physics (A. Asensio Ramos)

ESPOS
Deep learning has emerged as a very powerful set of techniques to extract relevant information from observations, sometimes showing much better results that other set of finely tuned algorithms. In ... [more]

ESP Online Seminar: Spectropolarimetric diagnostics using Sodium D lines (I.Milic)

ESPOS
In this talk we will focus on diagnostic potential of the spectral region around D lines of Sodium. We will first outline our approach to non-lte inversions, and present a method for computation of ... [more]

ESP Online Seminar: Interface Region Imaging Spectrograph views of how the solar (B. de Pontieu) atmosphere is energized

ESPOS
At the interface between the Sun's surface and million-degree outer atmosphere or corona lies the chromosphere. At 10,000K it is much cooler than the corona, but also many orders of magnitude denser ... [more]

ESP Online Seminar: Ca II 8542 Å Brightenings Induced by a Solar Microflare (C. Kuckein)

ESPOS
We study small-scale brightenings in Ca II 8542 Å line-core images to determine their nature and effect on localized heating and mass transfer in active regions. To that end, we analyzed ... [more]
Web-View
Print Page
Open in new window
Estimated DIN-A4 page-width
Go to Editor View