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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 9.

Formal uncertainties (1σ) in nHz of the central frequencies (left panel) and of the a 1-coefficients (right panel) as a function of frequency of the common modes measured in the 2088 day GONG data set by Korzennik (2005) fitting the individual- m spectra (red dots) and by using the m-averaged spectrum technique (black plus signs).

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