文章基本信息

标题：Solar wind and its evolution
本地全文：下载
作者：Takeru K. Suzuki
期刊名称：Earth, Planets and Space
电子版ISSN：1880-5981
出版年度：2012
卷号：64
期号：2
页码：201-206
DOI：10.5047/eps.2011.04.012
出版社：Springer Verlag
摘要：By using our previous results of magnetohydrodynamical simulations for the solar wind from open flux tubes, I discuss how the solar wind in the past is different from the current solar wind.The simulations are performed in fixed one-dimensional super-radially open magnetic flux tubes by inputing various types of fluctuations from the photosphere, which automatically determines solar wind properties in a forward manner.The three important parameters which determine physical properties of the solar wind are surface fluctuation, magnetic field strengths, and the configuration of magnetic flux tubes.Adjusting these parameters to the sun at earlier times in a qualitative sense, I infer that the quasi-steady-state component of the solar wind in the past was denser and slightly slower if the effect of the magneto-centrifugal force is not significant.I also discuss effects of magneto-centrifugal force and roles of coronal mass ejections.
关键词：Atmosphere ;MHD ;planets ;solar corona ;solar wind ;waves