日本地球惑星科学連合2019年大会

講演情報

[J] 口頭発表

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-EM16] 大気圏・電離圏

2019年5月29日(水) 10:45 〜 12:15 A03 (東京ベイ幕張ホール)

コンビーナ:大塚 雄一(名古屋大学宇宙地球環境研究所)、津川 卓也(情報通信研究機構)、川村 誠治(国立研究開発法人 情報通信研究機構)、座長:大塚 雄一江尻 省(国立極地研究所)

10:45 〜 11:00

[PEM16-07] ALOS2 ScanSAR InSARによるSporadic-Eイベントの検出へ向けて

*古屋 正人1前田 隼2日置 幸介1 (1.北海道大学大学院理学研究院地球惑星科学部門、2.北海道大学附属図書館)

キーワード:電離層、スポラディックE、干渉合成開口レーダー、だいち2号

Maeda et al. (2016) and Furuya et al. (2017) reported their detections of sporadic-E (Es) episodes in Japan, using L-band interferometric synthetic aperture radar (InSAR). The SAR data images are acquired by Advanced Land Observation Satellite (ALOS) 1/2 launched by JAXA in 2006 and 2014, respectively. The high spatial resolution of InSAR data allow us to examine the detailed structure of Es episode, which will complement the high temporal resolution of GNSS TEC data. The previous two studies are based on stripmap-mode SAR images, which have higher spatial resolution but are limitted in terms of the observation swath-width (Maeda et al., 2016; Furuya et al., 2017). Although the stripmap-mode is the most standard SAR imaging mode, ScanSAR mode is also nearly operational nowadays, and can image the Earth with much wider swath-width by as much as 350 km; the standard stripmap-mode of SM1 for ALOS2 covers only 50 km. Although the ScanSAR mode is a bit worse in terms of the spatial resolution along radar range direction than the stripmap mode image, ScanSAR InSAR image can dramatically improve the observation coverage, and thus help detect both small-scale and large-scale structure of Es.
We first check the data availability of ScanSAR images in Japan at any specific areas, and then check if any significant anomalies in either TEC or ROTI are observed via the database provided by NICT. We will report our preliminary results of ScanSAR InSAR imaging of Es in Japan.