Helium distribution in interplanetary space by Hisaki satellite

Atsushi YAMAZAKI; Kazuo YOSHIOKA; Go MURAKAMI; Tomoki KIMURA; Fuminori TSUCHIYA; Masato KAGITANI; Takeshi SAKANOI; Naoki TERADA; Yasumasa KASABA; Ichiro YOSHIKAWA

Presentation information

Poster

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

[P-EM25] Heliosphere and Interplanetary Space

Mon. May 25, 2015 6:15 PM - 7:30 PM Convention Hall (2F)

Convener:*Munetoshi Tokumaru(Solar-Terrestrial Environment Laboratory, Nagoya University), Tomoko Nakagawa(Information and Communication Engineering, Tohoku Institute of Technology)

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6:15 PM - 7:30 PM

[PEM25-P05] Helium distribution in interplanetary space by Hisaki satellite

*Atsushi YAMAZAKI¹, Kazuo YOSHIOKA¹, Go MURAKAMI¹, Tomoki KIMURA¹, Fuminori TSUCHIYA², Masato KAGITANI², Takeshi SAKANOI², Naoki TERADA², Yasumasa KASABA², Ichiro YOSHIKAWA³ (1.ISAS/JAXA, 2.Tohoku Univ., 3.Univ. Tokyo)

Keywords:Interplanetry helium, EUV observation

The HISAKI (SPRINT-A) satellite has a unique characteristics of the long term planet observation, such as Venus and Jupiter. The interval of planet observational terms, HISAKI has detected the emission from interplanetary space. In this presentation the HISAKI observation of interplanetary emission is shown and its potential on the interplanetary issue is argued.