{"title":"日食时中频广播波强度的观测","authors":"Tetsuo Fukami, R. Higashi, I. Nagano","doi":"10.23919/URSIGASS51995.2021.9560335","DOIUrl":null,"url":null,"abstract":"The ionospheric D region generated by sunlight has great influence on the MF wave propagation. To investigate the response on the D region during the solar eclipse, we observed the MF broadcast wave intensities for two similar periods, the annular and the partial solar eclipse in Japan. As a result, more MF broadcasts were observed during the partial solar eclipse although the partial solar eclipse had more sunlight than the annular solar eclipse.","PeriodicalId":152047,"journal":{"name":"2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS)","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Observation of the MF Broadcasting Wave Intensities on the Solar Eclipse\",\"authors\":\"Tetsuo Fukami, R. Higashi, I. Nagano\",\"doi\":\"10.23919/URSIGASS51995.2021.9560335\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The ionospheric D region generated by sunlight has great influence on the MF wave propagation. To investigate the response on the D region during the solar eclipse, we observed the MF broadcast wave intensities for two similar periods, the annular and the partial solar eclipse in Japan. As a result, more MF broadcasts were observed during the partial solar eclipse although the partial solar eclipse had more sunlight than the annular solar eclipse.\",\"PeriodicalId\":152047,\"journal\":{\"name\":\"2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS)\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2021-08-28\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.23919/URSIGASS51995.2021.9560335\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.23919/URSIGASS51995.2021.9560335","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Observation of the MF Broadcasting Wave Intensities on the Solar Eclipse
The ionospheric D region generated by sunlight has great influence on the MF wave propagation. To investigate the response on the D region during the solar eclipse, we observed the MF broadcast wave intensities for two similar periods, the annular and the partial solar eclipse in Japan. As a result, more MF broadcasts were observed during the partial solar eclipse although the partial solar eclipse had more sunlight than the annular solar eclipse.