Ilonidis和他的同事通过日震学方法来了解太阳内部的活动。
Ilonidis and his colleagues plumbed the sun's inner workings with a method called time-distance helioseismology.
因此可以说类太阳振动的研究是传统的日震学与恒星结构和演化相结合的产物。
So, the study of solar-like oscillations came from helioseismology combine with the stellar structure and evolution.
本文着重讨论了流体和磁流体力学在日震学方面和恒星形成中吸积和外流这两方面的应用。
This paper focuses on the application of hydrodynamics and magnetohydrodynamics to solar oscillations and accretion process and outflow in star formation.
本文着重讨论了流体和磁流体力学在日震学方面和恒星形成中吸积和外流这两方面的应用。
This paper focuses on the application of hydrodynamics and magnetohydrodynamics to solar oscillations and accretion process and outflow in star formation.
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