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dc.contributor.authorIyemori, Toshihikoen
dc.contributor.authorYamada, Akiyasuen
dc.contributor.authorAoyama, Tadashien
dc.contributor.authorHozumi, Kornyanaten
dc.contributor.authorYokoyama, Yoshihiroen
dc.contributor.authorOdagi, Yokoen
dc.contributor.authorSano, Yasuharuen
dc.contributor.authorPangsapa, Vijaken
dc.contributor.authorJarupongsakul, Thanawaten
dc.contributor.authorSaito, Akinorien
dc.contributor.authorIguchi, Masatoen
dc.contributor.alternative家森, 俊彦ja
dc.contributor.alternative山田, 彬泰ja
dc.contributor.alternative小田木, 洋子ja
dc.contributor.alternative齊藤, 昭則ja
dc.contributor.alternative井口, 正人ja
dc.date.accessioned2023-05-12T00:58:13Z-
dc.date.available2023-05-12T00:58:13Z-
dc.date.issued2022-
dc.identifier.urihttp://hdl.handle.net/2433/282051-
dc.description.abstractCorrelation between rainfall and short period GPS-TEC (total electron content) variations are investigated by using the precipitation data obtained on the ground and estimated from satellite observations (JAXA/GSMaP) as a proxy of lower atmospheric wave activity. The GPS-TEC data obtained at a tropical station, PHIM, in Phimai, Thailand, for 2014–2020, and the data obtained at a mid-latitude station, NAKG, in Tokara Nakanoshima Island, Japan, for 2017–2019, are examined. A statistical analysis of MEM (maximum entropy method) power spectral density (PSD) in the period range from 50 to 1200 s over PHIM clearly shows an enhancement in the cases of rainfall from that in no-rainfall cases, in particular, on the dusk side. The enhancement is observed both acoustic wave periods less than 5–6 min and internal gravity wave periods more than 10 min. The enhancement after sunset could be an effect of strong rainfall more frequent on the dusk side than that in other local time, or it could suggest the importance of ionospheric electron density profile change for the TEC variation. On the other hand, the PSD does not show such clear enhancement over NAKG on the dusk side, although it shows a small enhancement on both dayside and night-side. A clear PSD bulge near the main vertical acoustic resonance periods, i.e., around 275 s, appears in the average PSD profile of the TEC at PHIM, which suggests that the resonance effect contribute to some extent the PSD enhancement under rainy condition. An event analysis also suggests the contribution of acoustic resonance to the enhancement of the short period TEC variation. A complicated spatial distribution of TEC oscillation over a rainfall area around PHIM, where the TEC oscillations with various periods co-exist, is presented.en
dc.language.isoeng-
dc.publisherSpringer Natureen
dc.rights© The Author(s) 2022.en
dc.rightsThis 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.urihttp://creativecommons.org/licenses/by/4.0/-
dc.subjectGPS-TEC variationen
dc.subjectAcoustic wavesen
dc.subjectRainfallen
dc.subjectGSMaPen
dc.subjectVertical acoustic resonanceen
dc.subjectVertical couplingen
dc.subjectTropical squallen
dc.titleAmplitude enhancement of short period GPS-TEC oscillations over rainfall areaen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleEarth, Planets and Spaceen
dc.identifier.volume74-
dc.relation.doi10.1186/s40623-022-01604-7-
dc.textversionpublisher-
dc.identifier.artnum45-
dcterms.accessRightsopen access-
datacite.awardNumber15H05815-
datacite.awardNumber17K05669-
datacite.awardNumber20H00099-
datacite.awardNumber21K03643-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-15H05815/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17K05669/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-20H00099/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-21K03643/-
dc.identifier.eissn1880-5981-
jpcoar.funderName日本学術振興会ja
jpcoar.funderName日本学術振興会ja
jpcoar.funderName日本学術振興会ja
jpcoar.funderName日本学術振興会ja
jpcoar.awardTitle地球電磁気圏擾乱現象の発生機構の解明と予測ja
jpcoar.awardTitle磁気リップル現象の生成機構解明と短周期大気波動の全球的モニタリングへの応用ja
jpcoar.awardTitle多様な学術研究活動を育むアカデミックデータ・イノベーション成熟度モデルの開発ja
jpcoar.awardTitle電離圏磁場と電子密度の波状構造を生成する下層大気擾乱の特定と生成過程の解明ja
出現コレクション:学術雑誌掲載論文等

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