{"title":"太阳高潮上升阶段的动力学","authors":"Cao Tian-jun, Xu Ao-ao, Tang Yu-hua","doi":"10.1016/0146-6364(80)90045-6","DOIUrl":null,"url":null,"abstract":"<div><p>We propose that the ascending front of a solar surge results from the ejection of plasmoid caused by the Maxwellian stresses of the reconnected field lines in the neutral current sheet above a satellite spot plus the explosive expansion of the matter inside. This model can effectively explain the main dynamical features in both the accelerating and decelerating phases during the rise of the surge.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"1980-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90045-6","citationCount":"8","resultStr":"{\"title\":\"Dynamics of solar surge during its ascending stage\",\"authors\":\"Cao Tian-jun, Xu Ao-ao, Tang Yu-hua\",\"doi\":\"10.1016/0146-6364(80)90045-6\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We propose that the ascending front of a solar surge results from the ejection of plasmoid caused by the Maxwellian stresses of the reconnected field lines in the neutral current sheet above a satellite spot plus the explosive expansion of the matter inside. This model can effectively explain the main dynamical features in both the accelerating and decelerating phases during the rise of the surge.</p></div>\",\"PeriodicalId\":100241,\"journal\":{\"name\":\"Chinese Astronomy\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1980-06-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0146-6364(80)90045-6\",\"citationCount\":\"8\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chinese Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/0146636480900456\",\"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/0146636480900456","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Dynamics of solar surge during its ascending stage
We propose that the ascending front of a solar surge results from the ejection of plasmoid caused by the Maxwellian stresses of the reconnected field lines in the neutral current sheet above a satellite spot plus the explosive expansion of the matter inside. This model can effectively explain the main dynamical features in both the accelerating and decelerating phases during the rise of the surge.
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