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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 2.

Top panel: variation of the observational phase shift with L for the azimuthal order m = 0 (solid line), m = 1 (dashed line), and m = 2 (dashed-dotted line). Bottom panel: variation of the observational phase shift with m at L = 1412. The error estimates are obtained from an average over m of the absolute value of the phase-shift difference between + m and − m, divided by . This estimation assumes that the error does not depend on m.

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