日本地球惑星科学連合2024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-EM15] 太陽地球系結合過程の研究基盤形成

2024年5月29日(水) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6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 〜 18:45

[PEM15-P03] Horizontal structures of F layer and sporadic E-layer observed by the sounding rocket S-520-32

*高橋 透1斎藤 享1山本 衛2熊本 篤志3、芦原 佑樹4、篠原 学5 (1.国立研究開発法人 海上・港湾・航空技術研究所 電子航法研究所、2.京都大学生存圏研究所、3.東北大学大学院理学研究科、4.奈良工業高等専門学校電気工学科、5.鹿児島工業高等専門学校一般教育科)

キーワード:スポラディックE、トモグラフィ、Dual-Band Beacon

Sporadic-E (Es) layers are thin and dense layers appearing from 90 to 120 km and have been studied over six decades. Previous studies presented that the horizontal structure of the Es layer is likely to play an essential role in the generation of medium-scale traveling ionospheric disturbances (MSTIDs) due to E-F coupling via the Earth’s magnetic field lines.
The sounding rocket S-520-32, which aimed to observe irregularities associated with the Es layer and MSTIDs, was launched from Uchinoura Space Center (USC), JAXA (31.25 deg. N, 131.08 deg. E) at 23:20:00 JST (UT+9) on 11 August 2022. It transmitted the dual-band beacon signals (150 and 400 MHz) and received GNSS signals to separately observe the total electron content (TEC) in the E and F regions during the flight. The rocket flew between the E and F-layers and reached an altitude of 270 km. It splashed into the sea around 23:28:43. During the rocket flight, the MSTIDs were seen in the TEC map derived from the GNSS receiver network around the rocket trajectory. The ionosonde in Yamagawa, Kagoshima, 44 km away from USC, detected the Es layer, and the foEs and altitude of the Es layer were approximately 4.2 MHz and 116 km.
We installed the beacon receivers at USC, Tarumizu (TRM) (31.49 deg. N, 130.70 deg. E), Kirishima (KRS) (31.73 deg. N 130.73 deg. E), and Satsumasendai (SND) (31.83 deg. N, 130.34 deg. E). These four sites almost aligned with the backward extension of the line of rocket trajectory. We calculated the Total Electron Content (TEC) by the phase doppler of dual-band beacon signals and performed the tomography analysis with the TEC values observed at four sites. The Es layer was distributed around 100 km distance from the USC, but from 100 to 220 km, there was no single peak of electron density. The Es layer was found again around 220 to 300 km from the USC, but the altitude was lower by about 4 km, and the peak density was smaller by 1-4x1010 m-3 than the Es layer around 100 km from the USC.
The GNSS receiver received GPS, QZSS, Galileo, and BeiDou satellite signals. The deviation components of TEC (dTEC) was derived from the time series of phase doppler of the GNSS signals and compared with the horizontal structure of the Es layer which is connected by the Earth’s magnetic field line. The increase in dTEC can be seen above the Es layer, while dTEC decreased in the F region, corresponding to areas where the Es layer was not observed. Those characteristics suggested that the horizontal structure between F and Es layer seemed to show good agreement. In this presentation, we will show the observation results as well as the comparison of it with ionosonde and onboard instruments. Furthermore, we will compare the horizontal structure of the Es layer and the F-region structure to discuss the E-F coupling process.