Modeling the effects of a lightbridge on oscillations in a solar pore
Modeling the effects of a lightbridge on oscillations in a solar pore
Solar pores are ideal magnetic structures for wave propagation and transport of energy radially-outwards across the upper layers of the solar atmosphere. We aim to model the excitation and propagation of magnetohydrodynamic waves in a pore with a lightbridge modelled as two interacting magnetic flux tubes separated by a thin, …