Image Details

Choose export citation format:

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 5.

Short-time Lomb–Scargle analysis. A Lomb–Scargle periodogram is computed for 5 year moving windows in 1 year increments of the composite S-index time series for HD 30495. The contour plot gives the periodogram power normalized by the number of data points as a function of time and period, with the 99.9% significance contour highlighted as a dotted white line. The indicated time is for the center of the 5-year window. In each window, the highest peak above the 99.9% threshold is found and plotted as a large open circle, while a secondary significant peak, if present, is plotted as a small open circle. Vertical blue and red dashed lines indicate the minima and maxima in the long-term cycle model.The top panel indicates the number of data points in each 5-year window. The right panel gives the integrated normalized power for all windows. The bottom panel plots the amplitude ﹩{\rm{\Delta }}S﹩ of sine fits of the significant peak periods in the windowed data as open circles, with the amplitude of the three-component cycle model in red.

Other Images in This Article
Copyright and Terms & Conditions