日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM09] Space Weather and Space Climate

2023年5月26日(金) 10:45 〜 12:15 オンラインポスターZoom会場 (2) (オンラインポスター)

コンビーナ:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)、Mary Aronne中村 紗都子(名古屋大学宇宙地球環境研究所)

現地ポスター発表開催日時 (2023/5/25 17:15-18:45)

10:45 〜 12:15

[PEM09-P14] Annual total ionizing dose on the geostationary meteorological satellite Himawari8 estimated from the SEDA observation

*坂口 歌織1齊藤 慎司1長妻 努1 (1.情報通信研究機構)

キーワード:トータルドーズ、高エネルギー粒子観測、静止軌道

Total ionizing dose (TID) effects are common problem in space. Major sources of TID at geostationary orbit are energetic electrons in the outer Van Allen radiation belt and solar energetic particles (SEPs) accompanied by solar flares. Space environment data acquisition monitor (SEDA) onboard Japanese geostationary meteorological satellite Himawari8 have been observing energetic electrons and protons since November 2014. Yearly changes in TID are estimated from the SEDA observation in 2015–2022 by inputting data to SHIELDOSE-2 model assuming 1-mm Aluminum sphere shield. It is found that annual electron dose is highest in 2017 and lowest in 2020, it is less than half of 2017. Also, annual proton dose is found highest in 2017, followed by 2015, 2021, and 2022, but in any year other than these no major SEPs have occurred. TID is commonly estimated from the AE8 trapped electron model and JPL-1991 SEPs models. By comparison, the estimated TID from SEDA is several times lower than the TID estimated based on the AE8 and JPL1991 models.