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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