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Implications of the Recent Low Solar Minimum for the Solar Wind during the Maunder Minimum

  • Authors: M. Lockwood and M. J. Owens

Lockwood & Owens 2014 The Astrophysical Journal Letters 781 L7.

  • Provider: AAS Journals

Caption: Figure 2.

(a): 12-point running means of monthly international sunspot numbers, lang R rang 1yr. (c) and (e): Reconstructed annual near-Earth SW speed lang V SW rang 1yr (panel (c)) and IMF lang B rang 1yr (panel (e)) from the various pairings of geomagnetic indices. The blue filled and black open dots give annual mean and median values, respectively, of satellite observations and the cyan line in panel (e) is the modeled field B m shown in Figure 1. (d) and (f): normalized distributions of hourly (in gray) and annual (in blue) means of V SW (panel (d)) and B (panel (f)), observed during the space age (note that the pdf scale has been halved for annual values for clarity). Panel (d) also shows the distribution of hourly V SW means for the calendar year 2009. (b): lang V SW rang 1yr as a function of lang B rang 1yr. In panels (b), (c), and (e), black, red, orange, and green are for reconstructed values from the pairings of, respectively, IDV(1d)aa C, IDVaa C, IDV(1d)IHV, and IDVIHV.

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