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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 14.

Differences between the low-frequency central frequencies observed in 3960 days of GONG data (1 ⩽ l ⩽ 35) using the m-averaged spectrum technique and the associated theoretical values, taken from Christensen-Dalsgaard's model S (Christensen-Dalsgaard et al. 1996), as a function of the angular degree (left panel), of the frequency (middle panel), and of the inner turning point (right panel). The uncertainties multiplied by a factor of 20 are also presented. Ridges of same radial orders are connected, and for guidance some of the corresponding radial orders are indicated in the middle panel.

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