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A Floor in the Sun's Photospheric Magnetic Field: Implications for an Independent Small-scale Dynamo

  • Authors: E. W. Cliver, S. M. White, I. G. Richardson

E. W. Cliver et al 2024 The Astrophysical Journal Letters 961 .

  • Provider: AAS Journals

Caption: Figure 1.

Upper curve: MDI line of sight (LOS) magnetic flux (MF; black) scaled to match the HMI LOS MF (light blue) based on their overlap. Lower curves: observed F 10.7 flux reduced to 1 au (red) and F 10.7* (dark blue), computed from the magnetic flux of the composite record. All curves have a 1 month resolution. (Adapted from Svalgaard & Sun 2016.)

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