{"title":"磁场和输运过程","authors":"P. Eggenberger","doi":"10.25518/0037-9565.9240","DOIUrl":null,"url":null,"abstract":"In this presentation, we briefly discuss how magnetic angular momentum transport in stellar radiative zones can be constrained by asteroseismic measurements. We focus on the internal rotational properties deduced from rotational splittings of solar-like oscillations and how they can be used to characterize angular momentum transport in stellar interiors.","PeriodicalId":35838,"journal":{"name":"Bulletin de la Societe Royale des Sciences de Liege","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2020-01-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Magnetic fields and transport processes\",\"authors\":\"P. Eggenberger\",\"doi\":\"10.25518/0037-9565.9240\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this presentation, we briefly discuss how magnetic angular momentum transport in stellar radiative zones can be constrained by asteroseismic measurements. We focus on the internal rotational properties deduced from rotational splittings of solar-like oscillations and how they can be used to characterize angular momentum transport in stellar interiors.\",\"PeriodicalId\":35838,\"journal\":{\"name\":\"Bulletin de la Societe Royale des Sciences de Liege\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-01-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Bulletin de la Societe Royale des Sciences de Liege\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.25518/0037-9565.9240\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"Multidisciplinary\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin de la Societe Royale des Sciences de Liege","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.25518/0037-9565.9240","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"Multidisciplinary","Score":null,"Total":0}
In this presentation, we briefly discuss how magnetic angular momentum transport in stellar radiative zones can be constrained by asteroseismic measurements. We focus on the internal rotational properties deduced from rotational splittings of solar-like oscillations and how they can be used to characterize angular momentum transport in stellar interiors.
期刊介绍：
The ‘Société Royale des Sciences de Liège" (hereafter the Society) regularly publishes in its ‘Bulletin" original scientific papers in the fields of astrophysics, biochemistry, biophysics, biology, chemistry, geology, mathematics, mineralogy or physics, following peer review approval.
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