Fig. 12 from Activity‐related Changes in Local Solar Acoustic Mode Parameters from Michelson Doppler Imager and Global Oscillations Network Group

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Activity‐related Changes in Local Solar Acoustic Mode Parameters from Michelson Doppler Imager and Global Oscillations Network Group

Authors: R. Howe, R. W. Komm, F. Hill, D. A. Haber, and B. W. Hindman

Howe et al. 2004 The Astrophysical Journal 608 562.

Provider: AAS Journals

Caption: Fig. 12.

Mode frequency plotted against the magnetic flux value corresponding to the maximum amplitude change, as derived from the quadratic functions whose coefficients are shown in Fig. 11, for ﹩n=3﹩ (plus signs), ﹩n=4﹩ (triangles), ﹩n=5﹩ (diamonds), and ﹩n=6﹩ (circles).

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