ESPOS

European Solar Physics Online Seminars

Ca II K brightness as a function of magnetic field strength and characteristics of the observations

Mariarita Murabito

Hosted by INAF-OAR - Rome Astrophysical Observatory, Italy on September 19, 2024

Quantifying when and where strong magnetic skew forms in a data-driven global model of the solar corona when limited observational data exist

Jack Reid

Hosted by University of St. Andrews, United Kingdom on September 5, 2024

Modeling of non-radially propagating halo CMEs and forecasting their arrival time at Earth

Angelos Valentino

Hosted by Centre for Mathematical Plasma Astrophysics, KU Leuven, Belgium on June 27, 2024

Automatic Identification and Tracking of Sunspots

Charlotte Proverbs

Hosted by University of Central Lancashire, United Kingdom on June 13, 2024

Detection and in-depth analyses of quiet-Sun IRIS Bright Points

Llŷr Dafydd Humphries

Hosted by Aberystwyth University, United Kingdom on May 30, 2024