Sudip Mandal
Astrophysicist | Solar physics
The Sun’s atmosphere is structured and energized by magnetic fields, from plasma waves and coronal-loop dynamics to reconnection-driven activity. My research uses high-resolution space observations and historical solar archives to understand how magnetic fields and plasma flows shape the coupled solar atmosphere, tracking wave propagation, loop evolution, and long-term magnetic variability across solar-cycle timescales.
Waves, Coronal Dynamics & Solar Variability · EUI/Solar Orbiter Co-Investigator · Solar Orbiter RSWG Co-Chair · 45+ Peer-Reviewed Publications
SoMAD — Solar Magnetism and Atmospheric Dynamics
Studying magnetic variability and atmospheric dynamics across solar timescales.
Conceptual schematic illustrating the broad SoMAD research themes. This stylized illustration is included for visual context only — it is not to scale, not data-derived, and should not be interpreted as a scientifically complete or self-consistent representation of solar atmospheric structure and dynamics.