Magnetic fields of Sun-like stars

被引：0
|
作者：
Fares, Rim [1 ]
机构：
[1] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
来源：
MAGNETIC FIELDS THROUGHOUT STELLAR EVOLUTION | 2014年 / 302期
关键词：
stars: magnetic fields stars: activity stars: individual techniques: spectropolarimetry; ACTIVITY CYCLE; TAU BOOTIS; SPECTROPOLARIMETRIC OBSERVATIONS; DIFFERENTIAL ROTATION; MAIN-SEQUENCE; ACTIVE STARS; SOLAR-TYPE; DWARF; TOPOLOGIES; EMISSION;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Magnetic fields play an important role at all stages of stellar evolution, In Sun-like stars, they are generated in the outer convective layers. Studying the large-scale magnetic fields of these stars enlightens our understanding of the field properties and gives us observational constraints for the field generation models. In this review. 1 summarise the current observational picture of the large-scale magnetic fields of Sun-like stars, in particular solar-twins and planet host stars. I will discuss the observations of large-scale magnetic cycles, and compare these to the solar cycle.
引用
收藏
页码：180 / 189
页数：10
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