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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 7.

l–ν diagrams of the low-frequency modes with 1 ⩽ l ⩽ 25 measured in 2088 days of GONG (left panel) and MDI data (right panel). The open circles represent the modes measured by Korzennik (2005) using a classic peak-fitting method of the individual- m spectra, while the red dots correspond to the additional modes measured using the m-averaged spectrum technique that were not observed by Korzennik (2005). The ridges of same radial order are also indicated from n = 2 to n = 12.

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