50 citations · 58 across the 5 of their papers we have counts for
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astro-ph.SR2023
Data-driven simulations of magnetic field evolution in Active Region 11429: Magneto-friction method using PENCIL code
P. Vemareddy, Jörn Warnecke, Ph. A. Bourdin
Coronal magnetic fields evolve quasi statically over long time scales and dynamically over short time scales. As of now there exists no regular measurements of coronal magnetic fie…
astro-ph.SR2023★ 3 cited
Coronal bright point statistics I. Lifetime, shape, and coronal co-rotation
I. Kraus, Ph. -A. Bourdin, J. Zender +2
Context. The corona of the Sun is the part of the solar atmosphere with temperatures of over one million Kelvin, which needs to be heated internally in order to exist. This heating…