Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares
Authors: Kosuke Namekata, Vladimir S. Airapetian, Pascal Petit, Hiroyuki Maehara, Kai Ikuta, Shun Inoue, Yuta Notsu, Rishi R. Paudel, Zaven Arzoumanian, Antoaneta A. Avramova-Boncheva, Keith Gendreau, Sandra V. Jeffers, Stephen Marsden, Julien Morin, Coralie Neiner, Aline A. Vidotto, Kazunari Shibata
Kosuke Namekata et al
2024 The Astrophysical Journal961.
Provider: AAS Journals
Caption: Figure 5.
The same as Figures 3 and 4, but for the superflare observed on 2022 April 17 (E3). The basal level of Hα EW is a median value of −25 to −5 minutes, while the basal level of soft X-ray is a mean value of block 1.
