M. Roger, Yassine Maanane, M. Galtier, F. André, A. Delmas
{"title":"SYMBOLIC MONTE CARLO METHOD BASED ON ORTHOGONAL POLYNOMIALS SERIES: APPLICATION TO PHASE FUNCTION","authors":"M. Roger, Yassine Maanane, M. Galtier, F. André, A. Delmas","doi":"10.1615/RAD-19.360","DOIUrl":null,"url":null,"abstract":"A new Symbolic Monte Carlo (SMC) method based on series of orthogonal polynomials allows to express radiative quantities as a function of parameters that cannot be handled with usual symbolic Monte Carlo methods. In this work, the approach is illustrated with the phase function parameter: the radiative intensity is expressed as a function of the HenyeyGreenstein phase function asymmetry factor. Results show that the new SMC algorithm allows to estimate with a good accuracy the radiative intensity in all the space parameter.","PeriodicalId":413005,"journal":{"name":"Proceeding of Proceedings of the 9th International Symposium on Radiative Transfer, RAD-19","volume":"24 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceeding of Proceedings of the 9th International Symposium on Radiative Transfer, RAD-19","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1615/RAD-19.360","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
Abstract
A new Symbolic Monte Carlo (SMC) method based on series of orthogonal polynomials allows to express radiative quantities as a function of parameters that cannot be handled with usual symbolic Monte Carlo methods. In this work, the approach is illustrated with the phase function parameter: the radiative intensity is expressed as a function of the HenyeyGreenstein phase function asymmetry factor. Results show that the new SMC algorithm allows to estimate with a good accuracy the radiative intensity in all the space parameter.