磁场和输运过程

Q3 Multidisciplinary

Bulletin de la Societe Royale des Sciences de Liege Pub Date : 2020-01-14 DOI:10.25518/0037-9565.9240

P. Eggenberger

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引用次数: 0

摘要

在本演示中，我们简要讨论了恒星辐射区中的磁角动量传输如何受到星震测量的约束。我们专注于从类太阳振荡的旋转分裂中推导出的内部旋转特性，以及如何使用它们来表征恒星内部的角动量输运。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Magnetic fields and transport processes

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.

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来源期刊

Bulletin de la Societe Royale des Sciences de Liege Multidisciplinary-Multidisciplinary

CiteScore

0.90

自引率

0.00%

发文量

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.