日本地球惑星科学連合2025年大会

講演情報

[E] 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-EM14] 太陽地球系結合過程の研究基盤形成

2025年5月28日(水) 13:45 〜 15:15 303 (幕張メッセ国際会議場)

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)、座長:野澤 悟徳(名古屋大学宇宙地球環境研究所)、山本 衛(京都大学生存圏研究所)

14:00 〜 14:15

[PEM14-14] Equatorial Plasma Bubble detected by L-Band Synthetic Aperture Radar and GNSS-TEC Observations in Indonesian Region

*Ihsan Naufal Muafiry1Masato Furuya2Prayitno Abadi1、Teguh N. Pratama1 (1.BRIN、2.Hokkaido Univ.)

キーワード:EPB, ROTI map, L-Band SAR, ALOS-2/PALSAR-2

Equatorial Plasma Bubbles (EPBs) are disturbances in the ionosphere occurring close to the magnetic equator. These bubbles typically form after sunset during equinox months, though they can also be observed in other seasons. This phenomenon causes significant interference with radio wave signals, which are crucial for communication and navigation systems. We first search for plasma bubble occurrences in Indonesia, South-East Asian Sectors, by scanning through ROTI map available from https://gatotkaca.brin.go.id/petaionosfer/ionosphericmap/. ROTI map on May 9th, 2024 shows massive EPB clusters in Indonesia, one day prior to severe geomagnetic storm on May 10th, 2024. We further studied the small-scale structure of this EPB occurrence in Kalimantan (Indonesia) on May 9th, when ALOS-2/PALSAR-2 acquisition track overlaps the high-index of ROTI map at 23:39 local time (LT). ALOS-2/PALSAR-2 is L-band Synthetic Aperture Radar (SAR) sensor, whose images allowed us to perform azimuth offset tracking method; we concatenated two consecutive frames of ascending SAR images to expand the spatial coverage. It is notable that typical NE-SW azimuth streaking offset, exceeding 20 meters, has been observed, whose orientations are likely due to the ambient of geomagnetic field-line. The Total Electron Content (TEC) depletion associated with plasma bubble from SAR images are also measured in a range of 5-10 TECU. This amplitude is consistent with TEC depletion observed in GNSS-TEC.