Magnetoacoustic wave energy dissipation in the atmosphere of solar pores
The suitability of solar pores as magnetic wave guides has been a key topic of discussion in recent years. Here, we present observational evidence of propagating magnetohydrodynamic wave activity in a group of five photospheric solar pores. Employing data obtained by the Facility Infrared Spectropolarimeter at the Dunn Solar Telescope, oscillations
Gilchrist-Millar, Caitlin A. et al.
Fecha de publicación:
2
2021