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SUN-LIKE MAGNETIC CYCLES IN THE RAPIDLY ROTATING YOUNG SOLAR ANALOG HD 30495

  • Authors: Ricky Egeland, Travis S. Metcalfe, Jeffrey C. Hall, and Gregory W. Henry

2015 The Astrophysical Journal 812 12.

  • Provider: AAS Journals

Caption: Figure 3.

Lomb–Scargle periodograms from the time series of Figure 1. Panel (a) contains the result from single-instrument S-index surveys and panel (b) the combined S-index time series, as well as the APT photometry of Figure 1(c). Note the division in the period scale. The hatched region near ﹩P\approx 1\;\mathrm{year}﹩ contains artifacts of the seasonal sampling. The green and red horizontal dashed lines are the “excellent” and “poor” significance thresholds for the S-index periodograms, as defined in Baliunas et al. (1995). Note that the APT periodogram is scaled down by a factor of five for easy comparison and the magenta horizontal line is the “excellent” threshold for that series.

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