地球物理和天体物理流体力学系列讲座——Tide and magnetic field of stars, exoplanets and exomoons

报告题目Tide and magnetic field of stars, exoplanets and exomoons

报告人魏 星 教授 (北京师范大学)

报告地点: 三楼大会议室

报告时间:2024年 4 月 17 日(周三) 上午10:00

腾讯会议: 254-480-149

报告摘要

I will report on my recent projects about tide and magnetic field of celestial bodies such as stars, exoplanets and exomoons. The projects are as follows. (1) stellar magnetic dynamo: field-rotation relation in anisotropic rotating turbulence; (2) stellar oblique rotator: why solar radiative zone is in uniform rotation; (3) stellar wave transmission: can internal waves transmit at the interface of radiative and convective zones; (4) magnetic tide: ohmic dissipation needs to be taken into account for orbital evolution; (5) tidal resonance: the resonance of tidal wave and orbital motion; (6) exoplanet's inflation: radius anomaly of hot Jupiters; (7) exomoon's retention: where to detect exomoons.

报告人简介

Xing Wei is professor at BNU. He studied BS at Tsinghua and PhD at Cambridge then worked at ETH, Gottingen, Princeton and SJTU before joining BNU.

http://www.ucar.shao.cas.cn/ppm/report/202404/t20240411_774096.html


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