معرفی
Sergey Belov is a Research Fellow in the Department of Physics at the University of Warwick, specializing in solar plasma physics. His work combines theoretical modeling and observational data analysis to study energy transport in the solar corona.
Research focuses on magnetohydrodynamic wave propagation, thermal regulation mechanisms, and nanoflare detection using AIA/SDO ultraviolet data. He develops machine learning methods for identifying quasi-periodic pulsations in solar flare emissions.
Collaborative projects include developing the SITES algorithm for differential emission measure analysis and wave diagnostic tools for solar observations. His work contributes to understanding coronal heating through wave energy dissipation.
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