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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 16.

Left column: l–ν diagram, and a 1, a 3, and a 5 splitting coefficients for the common, low-frequency p-modes measured in the 3960 day GONG data set obtained by using the maximum likelihood (circles) and the narrowest peak (dots) of the m-averaged spectrum as FOM to determine the best estimates of the a-coefficients (see Section 3.1 and Figure 1). Right column: associated 1σ formal uncertainties (nHz) of the mode central frequencies, and of the a 1, a 3, and a 5 splitting coefficients.

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