Max-Planck-Institut für Sonnensystemforschung (MPS), Göttingen, Germany) and School of Space Research, Kyung Hee University, Yongin, Republic of Korea
Author in the following contributions
- Comparison of the photospheric line-of-sight velocity measured by SO/PHI-HRT and SDO/HMI
- The Fast Imaging Solar Scanning Spectro-Polarimeter (FISS-SP): First observations and early results
- Unveiling the dynamics and thermal structures of the jet base from SO high-resolution observation
- Direct Estimates of the Wilson Depression with Stereoscopic Observations of SO/PHI and SDO/HMI
- The highest resolution full-disk magnetic field maps, obtained with SO/PHI
- Simulation of a solar prominence with MURaM
- Ca II 8542 spectra of an enhanced network region simulated with the MURaM chromospheric extension
- High-resolution observations of small-scale activity in coronal hole plumes
- Magnetic structure of coronal dark halos
- Combining the point of view of SO/PHI-HRT and SDO/HMI to characterise facular and solar network brightness at the limb
- Coalignment for a quiet region from two vantage points of SO/PHI and Hinode/SP
- Coronal Loops are not one-dimensional
- Changes in chromospheric structure with magnetic field strength
- The Open Flux Problem: First steps with Solar Orbiter to investigate the underestimation of magnetic flux
- The never-ending attraction of the Sun’s magnetic personality
- Chromospheric Fe I lines in the NUV solar spectrum
- On the common appearance of superstrong magnetic fields in bipolar light bridges
