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Abstract: Origin of the Fe Kα line from solar and stellar flares: Statistical and Multiwavelength approaches (AGU25)

Origin of the Fe Kα line from solar and stellar flares: Statistical and Multiwavelength approaches

Shun Inoue1, Teruaki Enoto1, Dr. Yuta Notsu2, Wataru B. Iwakiri3, Tomoki Kimura4, Hiroyuki Uchida1, Kenji Hamaguchi5, Kosuke Namekata6, Zaven Arzoumanian7, Keith Gendreau7, Shin Toriumi8, Atsushi Yamazaki9, Go Murakami10, Fuminori Tsuchiya11 and Kazuo Yoshioka12, (1)Kyoto University, Kyoto, Japan, (2)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)Chiba University, Chiba, Japan, (4)Tokyo University of Science, Faculty of Science Division I, Department of Physics, Tokyo, Japan, (5)NASA/GSFC, Grrenbelt, United States, (6)Kyoto University & NASA Goddard Space Flight Center, Kyoto, Japan, (7)NASA Goddard Space Flight Center, Greenbelt, United States, (8)JAXA Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan, (9)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (10)ISAS-JAXA, Sagamihara, Japan, (11)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (12)The University of Tokyo, Tokyo, Japan