Transient ionization of the mesosphere during auroral breakup: Arase satellite and ground-based conjugate observations at Syowa Station

• Published in: Earth, planets, and space planets, and space, 2019-01, Vol.71 (1), p.1-10, Article 9
• Main Authors: Kataoka, Ryuho, Nishiyama, Takanori, Tanaka, Yoshimasa, Kadokura, Akira, Uchida, Herbert Akihito, Ebihara, Yusuke, Ejiri, Mitsumu K., Tomikawa, Yoshihiro, Tsutsumi, Masaki, Sato, Kaoru, Miyoshi, Yoshizumi, Shiokawa, Kazuo, Kurita, Satoshi, Kasahara, Yoshiya, Ozaki, Mitsunori, Hosokawa, Keisuke, Matsuda, Shoya, Shinohara, Iku, Takashima, Takeshi, Sato, Tatsuhiko, Mitani, Takefumi, Hori, Tomoaki, Higashio, Nana
• Format: Article
• Language: English
• Subjects: 3. Space science; Aurora; Auroral breakup; Auroral electrons; Auroral observations; Auroras; Broadband; Chorus waves; Computer simulation; Cosmic noise; Cyclotrons; Earth and Environmental Science; Earth Sciences; Electron precipitation; Electrons; Energetic electrons; Environmental aspects; Express Letter; Field of view; Geology; Geophysics/Geodesy; Ground-based observation; Ion cyclotron waves; Ionization; Mesosphere; Middle atmosphere; Noise; Observations; Particle transport; Rainfall; Satellite observation; Satellites; Sky; Very high frequencies; X-rays
• ISSN: 1880-5981; 1343-8832; 1880-5981
• DOI: 10.1186/s40623-019-0989-7

Transient mesospheric echo in the VHF range was detected at an altitude of 65–70 km during the auroral breakup that occurred from 2220 to 2226 UT on June 30, 2017. During this event, the footprint of the Arase satellite was located within the field of view of the all-sky imagers at Syowa Station in the Antarctic. Auroral observations at Syowa Station revealed the dominant precipitation of relatively soft electrons during the auroral breakup. A corresponding spike in cosmic noise absorption was also observed at Syowa Station, while the Arase satellite observed a flux enhancement of > 100 keV electrons and a broadband noise without detecting chorus waves or electromagnetic ion cyclotron waves. A general-purpose Monte Carlo particle transport simulation code was used to quantitatively evaluate the ionization in the middle atmosphere. Results of this study indicate that the precipitation of energetic electrons of > 100 keV, rather than X-rays from the auroral electrons, played a dominant role in the transient and deep (65–70 km) mesospheric ionization during the observed auroral breakup.