no code implementations • 28 Jan 2021 • Haisheng Ji, Parida Hashim, Zhenxiang Hong, Zhe Xu, Jinhua Shen, Kaifan Ji, Wenda Cao
All findings show that the magnetic perturbations are actually magneto-acoustic oscillations on the solar surface, the photosphere, powered by p-mode oscillations.
Solar and Stellar Astrophysics