Transverse oscillations in 3D along Ca II K bright fibrils in the solar chromosphere
Context. Fibrils in the solar chromosphere carry transverse oscillations as determined from non-spectroscopic imaging data. They are estimated to carry an energy flux of several kW m ‑2, which is a significant fraction of the average chromospheric radiative energy losses. Aims. We aim to determine the oscillation properties of fibrils not only in
Kianfar, Sepideh et al.
Fecha de publicación:
6
2025