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dc.contributor.author | Ssessanga, Nicholas | en |
dc.contributor.author | Yamamoto, Mamoru | en |
dc.contributor.author | Saito, Susumu | en |
dc.contributor.alternative | 山本, 衛 | ja |
dc.date.accessioned | 2022-03-31T06:29:28Z | - |
dc.date.available | 2022-03-31T06:29:28Z | - |
dc.date.issued | 2021 | - |
dc.identifier.uri | http://hdl.handle.net/2433/269106 | - |
dc.description.abstract | This paper demonstrates and assesses the capability of the advanced three-dimensional (3-D) ionosphere tomography technique, during severe conditions. The study area is northeast Asia and quasi-Japan-centred. Reconstructions are based on total electron content data from a dense ground-based global navigation satellite system receiver network and parameters from operational ionosondes. We used observations from ionosondes, Swarm satellites and radio occultation (RO) to assess the 3-D picture. Specifically, we focus on St. Patrick’s day geomagnetic storm (17–19 March 2015), the most intense in solar cycle 24. During this event, the energy ingested into the ionosphere resulted in Dst and Kp and reaching values ~ − 223 nT and 8, respectively, and the region of interest, the East Asian sector, was characterized by a ~ 60% reduction in electron densities. Results show that the reconstructed densities follow the physical dynamics previously discussed in earlier publications about storm events. Moreover, even when ionosonde data were not available, the technique could still provide a consistent picture of the ionosphere vertical structure. Furthermore, analyses show that there is a profound agreement between the RO profiles/in-situ densities and the reconstructions. Therefore, the technique is a potential candidate for applications that are sensitive to ionospheric corrections. | en |
dc.language.iso | eng | - |
dc.publisher | Springer Nature | en |
dc.rights | © The Author(s) 2021. | en |
dc.rights | This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. | en |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | - |
dc.subject | Ground-GNSS-STEC tomography | en |
dc.subject | Ionosonde data assimilation | en |
dc.subject | Geomagnetic storm | en |
dc.title | Assessing the performance of a Northeast Asia Japan-centered 3-D ionosphere specification technique during the 2015 St. Patrick’s day geomagnetic storm | en |
dc.type | journal article | - |
dc.type.niitype | Journal Article | - |
dc.identifier.jtitle | Earth, Planets and Space | en |
dc.identifier.volume | 73 | - |
dc.relation.doi | 10.1186/s40623-021-01447-8 | - |
dc.textversion | publisher | - |
dc.identifier.artnum | 124 | - |
dcterms.accessRights | open access | - |
datacite.awardNumber | 19F19031 | - |
datacite.awardNumber | 20H00197 | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19F19031/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-20H00197/ | - |
dc.identifier.eissn | 1880-5981 | - |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.awardTitle | 4次元トモグラフィーによる低・中緯度電離圏イレギュラリティの解明 | ja |
jpcoar.awardTitle | レーダー観測網・複数衛星・モデル計算を総合した赤道域電離圏変動特性の国際共同研究 | ja |
出現コレクション: | 学術雑誌掲載論文等 |

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