{"title":"辐射传递:迭代方法","authors":"Frédéric Paletou","doi":"10.1016/S1296-2147(01)01223-9","DOIUrl":null,"url":null,"abstract":"<div><p>We review several numerical approaches which have been developed during the last 10 years in order to perform more realistic radiative modelling of solar and stellar atmospheres. However, we shall restrict ourselves to the same ‘family’ of method, the ones which are derived from the so-called Accelerated Lambda-Iteration technique.</p></div>","PeriodicalId":100307,"journal":{"name":"Comptes Rendus de l'Académie des Sciences - Series IV - Physics-Astrophysics","volume":"2 6","pages":"Pages 885-898"},"PeriodicalIF":0.0000,"publicationDate":"2001-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1296-2147(01)01223-9","citationCount":"4","resultStr":"{\"title\":\"Transfert de rayonnement : méthodes itératives\",\"authors\":\"Frédéric Paletou\",\"doi\":\"10.1016/S1296-2147(01)01223-9\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We review several numerical approaches which have been developed during the last 10 years in order to perform more realistic radiative modelling of solar and stellar atmospheres. However, we shall restrict ourselves to the same ‘family’ of method, the ones which are derived from the so-called Accelerated Lambda-Iteration technique.</p></div>\",\"PeriodicalId\":100307,\"journal\":{\"name\":\"Comptes Rendus de l'Académie des Sciences - Series IV - Physics-Astrophysics\",\"volume\":\"2 6\",\"pages\":\"Pages 885-898\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2001-08-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/S1296-2147(01)01223-9\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Comptes Rendus de l'Académie des Sciences - Series IV - Physics-Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S1296214701012239\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Comptes Rendus de l'Académie des Sciences - Series IV - Physics-Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1296214701012239","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We review several numerical approaches which have been developed during the last 10 years in order to perform more realistic radiative modelling of solar and stellar atmospheres. However, we shall restrict ourselves to the same ‘family’ of method, the ones which are derived from the so-called Accelerated Lambda-Iteration technique.
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