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ACTIVE LONGITUDE AND SOLAR FLARE OCCURRENCES

  • Authors: N. Gyenge, A. Ludmány, and T. Baranyi

2016 The Astrophysical Journal 818 127.

  • Provider: AAS Journals

Caption: Figure 1.

Example for the spatial distribution of the quantity W in the CR 1718. The black line represents the 3σ significance limit. The largest peak represents the AL. In this CR, at the other side (roughly 180° phase shift), the weaker and more disperse peaks correspond to the co-dominant AL.

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