{"title":"一种计算太阳磁场和磁场的新方法","authors":"Song Mu-tao, Yin Chun-lin","doi":"10.1016/0146-6364(80)90047-X","DOIUrl":null,"url":null,"abstract":"<div><p>In this paper, an attempt is made to combine the use of the anti-rotational operator and the non-linear operator of the MHD to find a self-consistent solution for the flow and the magnetic fields. The method is illustrated by an example, which shows how the magnetic field above the solar surface changes following a motion of the feet of the field lines.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 2","pages":"Pages 163-173"},"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)90047-X","citationCount":"1","resultStr":"{\"title\":\"A new method of calculating the flow and magnetic fields of the sun\",\"authors\":\"Song Mu-tao, Yin Chun-lin\",\"doi\":\"10.1016/0146-6364(80)90047-X\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>In this paper, an attempt is made to combine the use of the anti-rotational operator and the non-linear operator of the MHD to find a self-consistent solution for the flow and the magnetic fields. The method is illustrated by an example, which shows how the magnetic field above the solar surface changes following a motion of the feet of the field lines.</p></div>\",\"PeriodicalId\":100241,\"journal\":{\"name\":\"Chinese Astronomy\",\"volume\":\"4 2\",\"pages\":\"Pages 163-173\"},\"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)90047-X\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chinese Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/014663648090047X\",\"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/014663648090047X","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A new method of calculating the flow and magnetic fields of the sun
In this paper, an attempt is made to combine the use of the anti-rotational operator and the non-linear operator of the MHD to find a self-consistent solution for the flow and the magnetic fields. The method is illustrated by an example, which shows how the magnetic field above the solar surface changes following a motion of the feet of the field lines.