Japan Geoscience Union Meeting 2025

Presentation information

[J] Oral

M (Multidisciplinary and Interdisciplinary) » M-TT Technology & Techniques

[M-TT37] New Developments in Earth Science Explored by Dense GNSS Observation Networks

Mon. May 26, 2025 3:30 PM - 5:00 PM 104 (International Conference Hall, Makuhari Messe)

convener:Yusaku Ohta(Research Center for Prediction of Earthquakes and Volcanic Eruptions, Graduate School of Science, Tohoku University), Mikiko Fujita(Japan Agency for Marine-Earth Science and Technology), Yuichi Otsuka(Institute for Space-Earth Environmental Research, Nagoya University), Takuya NISHIMURA(Disaster Prevention Research Institute, Kyoto University), Chairperson:Mikiko Fujita(Japan Agency for Marine-Earth Science and Technology)

4:15 PM - 4:30 PM

[MTT37-10] High-Resolution 3-D GNSS Tomography of Medium-Scale Traveling Ionospheric Disturbances Driven by Atmospheric Gravity Waves Over Japan

*Weizheng Fu1, Yuichi Otsuka1, Klemens Hocke2, Guanyi Ma3, Michi Nishioka4, Hidekatsu Jin4 (1.Institute for Space-Earth Environmental Research, Nagoya University , 2.Institute of Applied Physics, University of Bern, Bern, Switzerland , 3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China, 4.National Institute of Information and Communications Technology, Tokyo, Japan)

Medium-scale traveling ionospheric disturbances (MSTIDs) are a common type of ionospheric perturbations frequently observed at mid-latitudes. Atmospheric gravity waves (AGWs) serve as an important source for their generation. This study reconstructs the three-dimensional (3-D) structures of medium-scale traveling ionospheric disturbances (MSTIDs) driven by AGWs at summer sunrise and sunset terminators, using a computerized ionospheric tomography (CIT) technique based on ultra-dense Global Navigation Satellite System (GNSS) observations over Japan. Two representative events were analyzed in detail. The reconstruction results reveal that MSTID-induced electron density perturbations predominantly occur at altitudes of 200–400 km, with vertical wavelengths of approximately 250 km. Notably, the MSTID bands are vertically tilted and exhibit a downward phase progression along their propagation direction. Calculations based on AGW dispersion relations show strong agreement between the theoretical predictions and the reconstructed vertical wavelengths. For the first time, the detailed 3-D structures of MSTIDs driven by AGWs are reconstructed by GNSS measurements. These findings highlight the effectiveness of the 3-D CIT technique in resolving ionospheric disturbances with high spatial and temporal resolution, offering a robust tool for identifying disturbances from different sources and advancing our understanding of ionospheric dynamics.


Acknowledgements
The GNSS observation data from SoftBank used in this study were provided by SoftBank Corp. and ALES Corp. through the Consortium to utilize the SoftBank original reference sites for Earth and Space Science.