日本地球惑星科学連合2024年大会

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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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2024年5月30日(木) 15:30 〜 16:45 展示場特設会場 (2) (幕張メッセ国際展示場 6ホール)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、Chairperson:Paul Prikryl(ニューブランズウィック大学物理学部,カナダ天然資源地磁気研究所)、西谷 望(名古屋大学宇宙地球環境研究所)

16:00 〜 16:15

[PEM12-18] Acoustic resonance in the D-region ionosphere due to Pekeris wave after the Hunga Tonga-Hunga Ha'apai volcanic eruption using AVON VLF/LF transmitter signals

*大矢 浩代1土屋 史紀2、高村 民雄3品川 裕之4高橋 幸弘5、Alfred Chen6 (1.千葉大学大学院工学研究院、2.東北大学大学院理学研究科、3.千葉大学環境リモートセンシング研究センター、4.九州大学、5.北海道大学、6.国立成功大学)

The Hunga Tonga-Hunga Ha'apai volcano in Tonga (in southern Pacific, 20.54S, 175.38W) explosively erupted around 04:10 UT on 15 January, 2022, and large pressure variations occurred from the volcano. Large and medium scale traveling ionospheric disturbances (LSTID and MSTID) due the eruptions were observed (Themens, 2022), which were caused by Lamb wave excited by the eruptions. In addition to the Lamb wave, Pekeris waves were generated by the eruption (Watanabe et al., 2022). The Lamb waves are a kind of acoustic one, and propagate horizontally with phase velocity of ~310 m/s. On the other hand, Pekeris waves are internal resonance mode that propagate horizontally with phase velocity of ~240 m/s. The Pekeris waves have anti-phase between upper and lower stratopause, while the Lamb waves are in-phase vertically. The energy of Pekeris waves is enclosed between the stratopause and mesopause, within two atmospheric temperature minima, and the amplitudes of Pekeris waves are higher at the upper stratopause (>45 km). However, variations in the D-region ionosphere due to the Lamb and Pekeris waves associated with the eruptions have not been revealed at all. In this study, we investigate variations in VLF/LF transmitter signals and atmospheric electric field (or potential gradient) to understand coupling between the D-region ionosphere and atmosphere associated with Tonga volcanic eruptions of 15 January, 2022. The VLF/LF transmitters used in this study were JJY(60 kHz, Japan), JJI(22.2 kHz, Japan), and BPC(68.5 kHz, China). The receivers were Tainan (TNN, 23.07N, 120.12E) in Taiwan, where is one of Asia VLF observation network (AVON). We used 0.1-s sampling amplitude data. Unfortunately, there were no phase data for all paths on that day. The minimum distances of the JJI-TNN, JJY60kHz-TNN, and BPC-TNN propagation paths from the Tonga volcano were 8167.7 km, 8311.6 km, and 8499.9 km, respectively. The atmospheric electric field has been observed in Chiba University (CHB), (35.63N, 140.10E), Japan. The distances of CHB from the Tonga volcano were 7789.5 km. At arrival times of Lamb (~307 m/s) and Pekeris waves (~235 m/s), both variations in VLF/LF amplitudes were observed. Here we show observed oscillations of 100–200 s in VLF/LF transmitter signals and the magnetic and atmospheric electric fields, which were caused by Pekeris wave. The period of the variations in the D-region ionosphere due to Pekeris wave was similar to that due to Lamb wave, although the amplitudes of the variations for Pekeris wave were larger than those for Lamb wave. On the other hand, no corresponding changes with the period of 100–200 s in atmospheric pressure due to Pekeris waves were observed on the ground. A simulation of neutral wind revealed Pekeris waves oscillating near the mesopause, suggesting resonance. Therefore, the oscillation in atmospheric electric field is interpreted that the resonance in the lower ionosphere was projected onto the Earth's surface via a global electric circuit. In this presentation, we will discuss the mechanism of the phenomena in detail.