{"title":"An evolutionary feature of solar active regions","authors":"Yin Qi-feng, Luo Shao-guang, Wang Shu-lan","doi":"10.1016/0146-6364(80)90066-3","DOIUrl":null,"url":null,"abstract":"<div><p>The result that there is a time-lag between Type-I radio bursts and associated flares given in a previous paper [1] is confirmed by new statistical material.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 1","pages":"Pages 93-96"},"PeriodicalIF":0.0000,"publicationDate":"1980-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90066-3","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0146636480900663","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
The result that there is a time-lag between Type-I radio bursts and associated flares given in a previous paper [1] is confirmed by new statistical material.