Connection of photospheric magnetic fields to coronal phenomena: Within the framework of my PhD thesis, I am combining high-resolution observations from the SO/PHI and EUI instruments onboard Solar Orbiter in an effort to understand the magnetic nature of extended regions in the corona characterised by low EUV emissions.



Since 2021: PhD student at the Max Planck Institute for Solar System Research
2020: MSc in Physics at Bielefeld University
2013: BSc in Physics at Paderborn University


J. D. Nölke, S. K. Solanki, J. Hirzberger, et al. (2023). Coronal voids and their magnetic nature.  A&A 678, A196. DOI: 10.1051/0004-6361/202346040.

Conference contributions

SOLARNET Conference: The Many Scales of the Magnetic Sun (Potsdam, May 2023), talk
8th Solar Orbiter Workshop (Belfast, September 2022), talk

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