Feng Chen

Feng Chen joined HAO in 2016 as a post doctoral fellow supported by the Advanced Study Program of NCAR. His research focuses on the emergence of magnetic field from the interior of the Sun to its surface and further to the solar corona, and how the magnetic field gives rise to the brillant structures and dynamic of the corona observed in the Extreme Ultraviolet wavelength. He uses super computers to carry out magnetohydrodynamic simulations that can produce images looking like the real Sun.

Feng Chen image
Feng Chen

Feng Chen got his B.S. in astronomy and M.S. in astrophysics in Nanjing Univeristy. He received his PhD in physics in 2015 from University of Göttingen. The thesis work was done at the Max Planck Institute for Solar System Research.

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