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Scattering of the f-mode by Small Magnetic Flux Elements from Observations and Numerical Simulations

  • Authors: T. Felipe, D. Braun, A. Crouch, and A. Birch

Felipe et al. 2012 The Astrophysical Journal 757 148.

  • Provider: AAS Journals

Caption: Figure 8.

Top panel: variation of the absorption coefficient with L for the azimuthal orders m = 0 (dashed line) and m = 1 (solid line). Bottom panel: variation of the absorption coefficient with m at L = 2364. In both panels, asterisks correspond to the simulation with a flux tube with a 170 km radius, diamonds to the flux tube with a 370 km radius, and crosses to the flux tube with a 560 km radius.

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