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Measurement of Low Signal-To-Noise Ratio Solar p-Modes in Spatially Resolved Helioseismic Data

  • Authors: D. Salabert, J. Leibacher, T. Appourchaux, and F. Hill

SALABERT et al. 2009 The Astrophysical Journal 696 653.

  • Provider: AAS Journals

Caption: Figure 17.

Effect of asymmetry and spatial leaks on the fits. Left panel: differences (in nHz) in the 2088 day GONG frequencies estimated using different models to describe the m-averaged spectrum: symmetric Lorentzian profile minus asymmetric Lorentzian profile (Equation (2)) both models including the first δ m ± 2 spatial leaks, i.e., S2 minus A2 (red dots); both asymmetric Lorentzian profiles (Equation (2)) but ignoring the closest δ m ± 2 spatial leaks for one of them, i.e., A minus A2 (black plus signs). The differences in the extracted frequencies using different fitting profiles are represented as a function of frequency. Right panel: same as the left panel, but for the differences (in μHz) in the fitted mode linewidths.

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