V. Melnik, A. Brazhenko, A. V. Frantsuzenko, V. Dorovskyy, M. Shevchuk
{"title":"DECAMETER TYPE IV BURST WITH UNUSUAL HIGH POLARIZATION","authors":"V. Melnik, A. Brazhenko, A. V. Frantsuzenko, V. Dorovskyy, M. Shevchuk","doi":"10.18524/1810-4215.2023.36.290136","DOIUrl":null,"url":null,"abstract":"We present results of observations of Type IV burst with unusual high polarization equalled in maximum phase about 100%. This burst was registered both by URAN-2 and NDA radio telescopes on 13 July 2022. It continued for about 5 hours and consisted of sub-bursts with high frequency drift rates and had short durations. We associate it with the weak CME, which propagated in the East direction in the form of thread-like structure. Theoretical description of sub-burst in the plasma mechanism of radio emission allow explaining their high polarization, high drift rates and short durations.","PeriodicalId":34039,"journal":{"name":"Odessa Astronomical Publications","volume":"122 ","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2023-12-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Odessa Astronomical Publications","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18524/1810-4215.2023.36.290136","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
We present results of observations of Type IV burst with unusual high polarization equalled in maximum phase about 100%. This burst was registered both by URAN-2 and NDA radio telescopes on 13 July 2022. It continued for about 5 hours and consisted of sub-bursts with high frequency drift rates and had short durations. We associate it with the weak CME, which propagated in the East direction in the form of thread-like structure. Theoretical description of sub-burst in the plasma mechanism of radio emission allow explaining their high polarization, high drift rates and short durations.