Theoretical free-oscillation spectra: the importance of wide band coupling

Illustrative calculations are presented of the effect of the coupling of la rge groups of Earth's normal modes in a realistic 3-D earth model. In previ ous work the effect of modal splitting and coupling has been treated either in the self-coupling approximation (SC) or in the group-coupling approxima tion (GC), also known as quasi-degenerate perturbation theory. In SC a mode is treated as isolated in the spectrum and the theory of degenerate splitt ing is used to calculate the effect of lateral heterogeneity, rotation and ellipticity on each individual modal multiplet. In GC a small number of mod es close together in frequency are treated as a group and the effect of cou pling within the group is included. Of course, SC can be considered as a sp ecial case of GC in which there is only a single modal multiplet in the gro up. In principle, modal spectra are affected by coupling among all modes. G iven that explicit calculations can be performed only for a finite collecti on of modes, we are led to consider the question of how large the group of modes considered must be in order to obtain theoretical spectra of sufficie nt accuracy for a given purpose. The particular purpose that we have in min d is the use of modal spectra to refine 3-D models of earth structure. To d o this we carry out calculations in which the results of SC and GC are comp ared with those of full coupling (FC), by which we mean coupling calculatio ns including large collections of multiplets, for example all modes having frequencies less than a certain upper bound or cut-off frequency. The resul ts indicate that SC and GC often represent a poor approximation to FC. The differences in modal spectra calculated using SC/GC and those obtained usin g FC are, in many cases, comparable to the differences between observed and theoretical spectra. We compare FC for all 140 spheroidal and toroidal mod es up to 3 mHz with GC using the 25 pairs of modes defined by Resovsky & Ri tzwoller (1998) and with GC in 33 subgroups of spheroidal and toroidal mode s. We find that full coupling is needed to obtain the best synthetic spectr a. The matrices for full coupling of 140 modes become large (approximately 2500 x 2500), but are still tractable.