日本地球惑星科学連合2025年大会

講演情報

[E] 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-EM14] 太陽地球系結合過程の研究基盤形成

2025年5月28日(水) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

17:15 〜 19:15

[PEM14-P17] Recalibration of ionogram virtual height and scaled parameters obtained by NICT's ionosonde observation

*西岡 未知1津川 卓也1 (1.(独)情報通信研究機構)

キーワード:イオノゾンデ、再校正、見かけ高度

Ionosonde observation system operated by National Institute of Information and Communications technology (NICT) was replaced to Vertical Incidence Pulsed Ionospheric Radar 2 (VIPIR2) in 2016 and 2017. At the beginning of the replacement, a calibration was done for the ionograms and range bias of 300 μsec has been removed. NICT has been sharing the range adjusted ionograms since then. On the other hand, Teraoka et al (2022 JpGU, 2023 SGEPSS) pointed out that virtual heights of sporadic E-lay (h’Es) decreased around 2017 when the new ionosonde was installed based on an analysis of the manual scaled parameters. The initial range calibration may not be sufficient. Therefore, adjustment was performed again, and the result will be reported in this presentation. We conducted an analysis of the calibration signal and typical ionospheric echo. The result shows that the virtual height was lower by about 24 km. It is also necessary to recalibrate manually and automatically scaled parameters. The recalibration is conducted for all ionograms and scaled parameters. The revised products are open through web page (https://wdc.nict.go.jp/Ionosphere/) since March 2025.