Fan Zhang

Fan Zhang is a Postdoctoral Fellow at the Rosseland Center for Solar Physics, University of Oslo, specializing in computational fluid dynamics and solar plasma modeling. His research bridges high-order numerical methods with astrophysical applications, particularly in magnetohydrodynamics (MHD) for solar corona and wave propagation studies.

• University of Oslo
• Rosseland Center for Solar Physics

Research Interests

Zhang's work focuses on advancing numerical techniques for shock-capturing and MHD simulations, enabling precise modeling of solar phenomena like coronal mass ejections (CMEs), Alfvén waves, and plasma dynamics. He develops finite-volume and compact nonlinear schemes tailored for unstructured grids, addressing challenges in numerical stability and accuracy.

Recent Publications

His 15 most recent articles (2025–2021) highlight innovations in time-accurate MHD models (e.g., SIP-IFVM, COCONUT), mesh topology effects on solar simulations, and algorithms for overshooting oscillation suppression. Key themes include computational efficiency, high-order numerical schemes, and two-fluid modeling of solar plasmas.

Collaborative Work

Zhang frequently collaborates with international researchers on projects like COCONUT, which optimizes preprocessing of magnetic maps for space-weather forecasting and solar cycle modeling. His contributions span algorithm design, model validation, and cross-disciplinary computational frameworks.