Dr Marianna B. Korsós
Solar physicist • Space Weather
I am a solar physicist whose research focuses on understanding the pre-eruptive evolution of the source regions of the largest solar eruptions in the Solar System—solar flares and coronal mass ejections (CMEs). These source regions, known as solar active regions, host the complex magnetic structures that give rise to major eruptive activity. My work centres on the magnetic field evolution of active regions prior to eruption, with the aim of identifying characteristic signatures that indicate when an active region is becoming ready to erupt. I am particularly interested in the role of so-called active longitudes, where solar eruptions preferentially occur. These long-lived longitudinal zones are characterised by enhanced magnetic flux emergence, making the active regions that form there more magnetically complex and therefore more prone to producing hazardous flares and CMEs. I combine observational solar physics with advanced data analysis and machine-learning techniques to improve short- and medium-term space-weather prediction. In addition to my research, I serve as Deputy Chair of the UK Solar Physics community, contributing to community building, mentoring, and outreach.