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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 11.

l–ν diagram of the low-frequency, low-degree (1 ⩽ l ⩽ 3) modes measured with the integrated-light instruments GOLF and BiSON (open circles) by R. A. García, P. Boumier, and W. J. Chaplin (2007, private communications) and with the spatially resolved instruments GONG and MDI using the m-averaged spectrum technique (red dots), over comparable periods of time.

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