Chanjinda Taesuwan, Sakkrapop Khuangsatung, N. Wichaipanich, K. Hozumi
{"title":"Vertical plasma drift velocity of F2 layer inferred from ionosonde compared with IRI-2016 Model Over Chumphon, Thailand","authors":"Chanjinda Taesuwan, Sakkrapop Khuangsatung, N. Wichaipanich, K. Hozumi","doi":"10.1109/ECTI-CON58255.2023.10153281","DOIUrl":null,"url":null,"abstract":"This paper presents the vertical plasma drifts velocity of the F2-layer (Vz-hmF2) compared with the IRI-2016 model. The Vz-hmF2 data was obtained from the equatorial ionosonde station at Chumphon (Lat. 10.72°N, Long. 99.37°E, Dip 3.0°N), Thailand. The Vz-hmF2 during low solar activity in 2010 was analyzed the daily and monthly variations between both the observed and the modelled. The results show the IRI-2016 model overestimates the observed Vz during noontime to midnight while it underestimates from pre-sunrise to noontime hours. The observed Vz changes from -60 to 110 m/s and the model varies between $\\pm 20m/s$. This paper will be helpful the improvement of the IRI model in the future.","PeriodicalId":340768,"journal":{"name":"2023 20th International Conference on Electrical Engineering/Electronics, Computer, Telecommunications and Information Technology (ECTI-CON)","volume":"20 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-05-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"2023 20th International Conference on Electrical Engineering/Electronics, Computer, Telecommunications and Information Technology (ECTI-CON)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/ECTI-CON58255.2023.10153281","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
This paper presents the vertical plasma drifts velocity of the F2-layer (Vz-hmF2) compared with the IRI-2016 model. The Vz-hmF2 data was obtained from the equatorial ionosonde station at Chumphon (Lat. 10.72°N, Long. 99.37°E, Dip 3.0°N), Thailand. The Vz-hmF2 during low solar activity in 2010 was analyzed the daily and monthly variations between both the observed and the modelled. The results show the IRI-2016 model overestimates the observed Vz during noontime to midnight while it underestimates from pre-sunrise to noontime hours. The observed Vz changes from -60 to 110 m/s and the model varies between $\pm 20m/s$. This paper will be helpful the improvement of the IRI model in the future.