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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 8.

Left panel: histogram of the differences (in nHz) in the estimated central frequencies between the 2088 day GONG data set using the m-averaged spectrum technique and the coeval 2088 day GONG Korzennik (2005)'s estimates. Right panel: histogram of the differences (in nHz) in the estimated frequencies between the 2088 day GONG and MDI data sets using the m-averaged spectrum technique in the sense GONG minus MDI. The corresponding Gaussian function fits and their associated mean values and standard deviations are also indicated.

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