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- ItemMeridional circulation and global solar oscillations(Dordrecht [u.a.] : Springer Science + Business Media, 2008) Roth, M.; Stix, M.We investigate the influence of large-scale meridional circulation on solar p modes by quasi-degenerate perturbation theory, as proposed by Lavely and Ritzwoller (Roy. Soc. Lond. Phil. Trans. Ser. A 339, 431, 1992). As an input flow we use various models of stationary meridional circulation obeying the continuity equation. This flow perturbs the eigenmodes of an equilibrium model of the Sun. We derive the signatures of the meridional circulation in the frequency multiplets of solar p modes. In most cases the meridional circulation leads to negative average frequency shifts of the multiplets. Further possibly observable effects are briefly discussed. © 2008 The Author(s).
- ItemGONG p-Mode Parameters Through Two Solar Cycles(Dordrecht [u.a.] : Springer Science + Business Media B.V, 2018) Kiefer, René; Komm, Rudi; Hill, Frank; Broomhall, Anne-Marie; Roth, MarkusWe investigate the parameters of global solar p-mode oscillations, namely damping width Γ, amplitude A, mean squared velocity ⟨v2⟩, energy E, and energy supply rate dE/dt, derived from two solar cycles’ worth (1996 – 2018) of Global Oscillation Network Group (GONG) time series for harmonic degrees l=0--150. We correct for the effect of fill factor, apparent solar radius, and spurious jumps in the mode amplitudes. We find that the amplitude of the activity-related changes of Γ and A depends on both frequency and harmonic degree of the modes, with the largest variations of Γ for modes with 2400 μHz≤ν≤3300 μHz and 31≤l≤60 with a minimum-to-maximum variation of 26.6±0.3% and of A for modes with 2400 μHz≤ν≤3300 μHz and 61≤l≤100 with a minimum-to-maximum variation of 27.4±0.4%. The level of correlation between the solar radio flux F10.7 and mode parameters also depends on mode frequency and harmonic degree. As a function of mode frequency, the mode amplitudes are found to follow an asymmetric Voigt profile with νmax=3073.59±0.18 μHz. From the mode parameters, we calculate physical mode quantities and average them over specific mode frequency ranges. In this way, we find that the mean squared velocities ⟨v2⟩ and energies E of p modes are anticorrelated with the level of activity, varying by 14.7±0.3% and 18.4±0.3%, respectively, and that the mode energy supply rates show no significant correlation with activity. With this study we expand previously published results on the temporal variation of solar p-mode parameters. Our results will be helpful to future studies of the excitation and damping of p modes, i.e., the interplay between convection, magnetic field, and resonant acoustic oscillations.