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Lifetimes and Emergence/Decay Rates of Star Spots on Solar-type Stars Estimated by Kepler Data in Comparison with Those of Sunspots

  • Authors: Kosuke Namekata, Hiroyuki Maehara, Yuta Notsu, Shin Toriumi, Hisashi Hayakawa, Kai Ikuta, Shota Notsu, Satoshi Honda, Daisaku Nogami, and Kazunari Shibata

2019 The Astrophysical Journal 871 187.

  • Provider: AAS Journals

Caption: Figure 2.

Schematic pictures to explain the method ([A]–[E]) of tracing the local minima described in Section 2.2. All panels correspond to the phase-time diagram of the local minima, which is similar to Figure 1(c). The panels are described as follows: [A] explains how to start the tracing and identification of spots, [B] explains how to continue the tracing after the identifications, [C] explains how to avoid the observational data gaps, and [D, E] explains how to remove the spot candidates that can merge with other spots in longitudes that are originally located at the separated longitudes. If there are other local minima in the gray region, the spot candidates are removed in our algorithm.

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