Fig. 2 from On the Spatial Dependence of Low‐Degree Solar p‐Mode Frequency Shifts from Full‐Disk and Resolved‐Sun Observations

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On the Spatial Dependence of Low‐Degree Solar p‐Mode Frequency Shifts from Full‐Disk and Resolved‐Sun Observations

Authors: S. J. Jiménez-Reyes, R. A. García, W. J. Chaplin, and S. G. Korzennik

Jiménez‐Reyes et al. 2004 The Astrophysical Journal Letters 610 L65.

Provider: AAS Journals

Caption: Fig. 2.

Frequency shift, in units of μHz, averaged for modes over ﹩2400\,\mu \mathrm{Hz}\,\leq \nu \leq 3400\,\mu \mathrm{Hz}\,﹩, from GOLF (abscissa, with label ﹩\ell ﹩) and MDI (ordinate, with labels ﹩\ell ﹩, ﹩\vert m\vert ﹩). The dashed line in each panel gives the 1:1 correlation, while the solid line is a linear fit between the data.

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