Figure 5 from Measurement of Low Signal-To-Noise Ratio Solar p-Modes in Spatially Resolved Helioseismic Data

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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 5.

Examples of m-averaged power spectra in the case of the l = 17 multiplet for four different radial-orders n = 2, 4, 6, and 8. The red lines represent the best MLE fits (Equation (2)), including the closest δ m = ±2 spatial leaks, whose positions are illustrated by the dotted lines.

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