H beta line spectrum (486.1 nm) from proton aurora observed by the Hyper-Spectral Camera for Aurora Imaging (HySCAI)

Katsumi Ida

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM18] Dynamics of Magnetosphere and Ionosphere

Thu. May 28, 2026 10:45 AM - 12:15 PM 304 (International Conference Hall, Makuhari Messe)

Chairperson:Hasegawa Hiroshi, Obana Yuki(International Research Center for Space and Planetary Environmental Science, Kyushu University), Yamamoto Kazuhiro(Institute for Space-Earth Environmental Research)

10:45 AM - 11:00 AM

[PEM18-06] H beta line spectrum (486.1 nm) from proton aurora observed by the Hyper-Spectral Camera for Aurora Imaging (HySCAI)

*Katsumi Ida¹, Mikirou Yoshinuma¹, Yusuke Ebihara² (1. National Institute for Fusion Science, 2. Research Institute for Sustainable Humanosphere, Kyoto University)

Keywords:proton aurora, H-beta line spectrum, HyperSpectral Camera, Kiruna

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