Fig. 1 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. 1.

Frequency shift per unit change in the 10.7 cm radio flux for individual (ℓ, m) p‐mode components (as extracted from resolved‐Sun MDI data) against the corresponding normalized Legendre components of the Kitt Peak magnetic field (the latter averaged over the full time period of the observations).

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