{"title":"太阳活动区的演化特征","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":"{\"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}","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}
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.
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