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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 1.

(left panel), natural logarithm of the mode linewidth (middle panel), and entropy (right panel) of the m-averaged spectrum as a function of the shift coefficient a 1 obtained from 10 simulated l = 15 spectra. The vertical dashed lines represent the introduced value of a 1 (400 nHz) in the simulations. The horizontal dotted-dashed line in the center panel represents the mode linewidth of the simulated spectra, 0.4 μHz.

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