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Susanne Höfner is a Professor in the Department of Physics and Astronomy at Uppsala University, specializing in the study of the physical properties of evolved stars. Her research focuses particularly on the dynamical processes involving stellar pulsation and winds, as well as the formation of stardust. She works on developing advanced radiation-hydrodynamical models to compare observations and enhance our understanding of these phenomena. Currently, she leads the EXWINGS project, funded by an ERC Advanced Grant, which aims to explain the winds of cool giant and supergiant stars through global 3D models. Her expertise encompasses Astronomy and Space Physics, particularly in the area of Stellar Winds.
General Master's requirements applying across Science, Technology, and Humanities departments.