Japan Geoscience Union Meeting 2022

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM13] Coupling Processes in the Atmosphere-Ionosphere System

Tue. May 24, 2022 1:45 PM - 3:15 PM 302 (International Conference Hall, Makuhari Messe)

convener:Huixin Liu(Earth and Planetary Science Division, Kyushu University SERC, Kyushu University), convener:Yuichi Otsuka(Institute for Space-Earth Environmental Research, Nagoya University), Loren Chang(Institute of Space Science, National Central University), convener:Yue Deng(University of Texas at Arlington), Chairperson:Yuichi Otsuka(Institute for Space-Earth Environmental Research, Nagoya University), Atsuki Shinbori(Institute for Space-Earth Environment Research (ISEE), Nagoya University), Mitsumu K. Ejiri(National Institute of Polar Research)


3:00 PM - 3:15 PM

[PEM13-06] Ionospheric irregularities and scintillations during the geomagnetic storm on 15 January 2022

*Susumu Saito1, Takayuki Yoshihara1, Toru Takahashi1 (1.Electronic Navigation Research Institute, National Institute of Maritime, Port, and Aviation Technology)

Keywords:Ionospheric irregularities,, Ionospheric scintillation, Geomagnetic storm

On 15 January 2022, various ionospheric disturbances were observed over Japan. Some of them appeared to be associated with the volcanic eruption of Hunga Tonga-Hunga Ha'apai. On the other hand, since a moderate geomagnetic storm commenced on 14 January 2022 was going on at the same time, it is important to distinguish the effects of the volcanic eruption and the geomagnetic storm.
We used GNSS total electron contents (TECs) and its temporal fluctuation represented by rate of TEC index (ROTI) derived from GNSS data from GEONET (GNSS Earth Observation Network). Besides the traveling ionospheric disturbances (TIDs) seen in high-pass filtered (detrended) TEC (dTEC) coinciding with atmospheric waves believed to be emitted from the volcanic eruption, multiple band-like regions with ROTI enhancement was started to be observed from 10 UT on 15 January 2022. They extended in the NW-SW direction and apparently moved westward. The structures were not aligned with the TIDs seen in dTEC. In the region of ROTI enhancement, enhancement in TEC was also observed. Stripes of sharp TEC depletions were embedded in the region. This looks similar to the storm-enhanced density (SED) or storm-induced plasma stream (SIPS) observed in the geomagnetic storms.
At the same time, strong scintillation in GNSS signals were observed over Ishigaki Island (24.4N, 124.1E), Japan. A number of TEC depletions embedded in TEC enhancements were observed. Scintillations were observed for almost all the GNSS satellite in view which indicates that the irregularities were distributed over a wide area.
Although it is still unknown that these ionospheric irregularities were due to the geomagnetic storm or combined effects with other sources, this event is important both for understanding the mechanisms of the ionospheric irregularities and for evaluating their effects on GNSS applications.