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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 3.

Examples of m-averaged power spectra (left panels) before (top) and after (bottom) correcting for the shift coefficients in the case of the oscillation multiplet l = 16, n = 4 observed in 2088 days of GONG data. The corresponding m–ν diagrams are also shown (right panels). The crosses indicate the position of the corresponding theoretical central frequency calculated from Christensen-Dalsgaard's model S (Christensen-Dalsgaard et al. 1996). The dot-dashed lines on the left-hand side panels give the 10% probability limit that a peak is due to noise in the 238 windows, 1.5 μHz wide. The illustrated spectral window contains the 2 l + 1 components of the represented multiplet.

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