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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 5.

Example of the decomposition of the solar wind for the 60 days interval from 2009 April 30 to June 28 into its three principal components: coronal mass ejections (CME), high-speed streams (HSS), and slow solar wind (SSW). After Richardson et al. (2000) and Richardson & Cane (2012). Data sources: http://omniweb.gsfc.nasa.gov/; Richardson (2023).

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