Multiple Scattering of Seismic Waves from Ensembles of Upwardly Lossy Thin Flux Tubes
arXiv:1506.07638 · doi:10.1007/s11207-015-0732-x
Abstract
Our previous semi-analytic treatment of f- and p-mode multiple scattering from ensembles of thin flux tubes (Hanson and Cally, Astrophys. J. 781, 125; 791, 129, 2014) is extended by allowing both sausage and kink waves to freely escape at the top of the model using a radiative boundary condition there. As expected, this additional avenue of escape, supplementing downward loss into the deep solar interior, results in substantially greater absorption of incident f- and p-modes. However, less intuitively, it also yields mildly to substantially smaller phase shifts in waves emerging from the ensemble. This may have implications for the interpretation of seismic data for solar plage regions, and in particular their small measured phase shifts.
9 Pages, 5 Figures. Accepted by Solar Physics
References in corpus (6)
- {\it f}-mode interactions with thin flux tubes: the scattering matrix
- Numerical simulations of multiple scattering of the mode by flux tubes
- The scattering of - and -modes from ensembles of thin magnetic flux tubes - An analytical approach
- Energy Loss of Solar Modes due to the excitation of Magnetic Sausage Tube Waves: Importance of Coupling the Upper Atmosphere
- Simulation of f-Mode Propagation Through a Cluster of Small Identical Magnetic Flux Tubes
- An Analytical Approach to Scattering Between Two Thin Magnetic Flux Tubes in a Stratified Atmosphere