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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 6.

Decomposition of annually averaged solar wind B from 1965 to 2021 into its three components: (a) CME-related flows, (b) high-speed streams (HSSs), and (c) slow solar wind (SSW; with the ∼2.8 nT floor level indicated), for comparison with the sunspot number in panel (d), with cycle numbers indicated. The data behind this figure are available in machine-readable format.

(The data used to create this figure are available.)

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