颜毅华,谭宝林.太阳物理研究与发展[J].中国科学院院刊,2012,(1):59-66.

太阳物理研究与发展

Research and Development of Solar Physics

颜毅华
中国科学院国家天文台中国科学院太阳活动重点实验室
Yan Yihua
Key Laboratory of Solar Activity,National Astronomical Observatories of CAS 100012 Beijing
谭宝林
中国科学院国家天文台中国科学院太阳活动重点实验室
Tan Baolin
Key Laboratory of Solar Activity,National Astronomical Observatories of CAS 100012 Beijing

         太阳;爆发;等离子体;日地环境

        the Sun;eruptive process;plasma;solar-terrestrial environment

        太阳是离地球最近的一颗恒星,也是人类可以进行具有一定空间分辨率地详细观测和研究的唯一恒星,在现代物理学和天文学的发展中扮演着重要的角色;同时,太阳为人类家园带来了温暖和光明,太阳的剧烈活动也对人类产生重大影响,探索太阳对现代社会的可持续发展具有极其重要的意义。本文简要介绍了太阳物理学的基本内容、研究方法,总结了过去半个多世纪太阳物理学研究所取得的主要成就,在此基础上对太阳物理学的前沿科学难题及未来发展前景进行了讨论。

        The Sun is the nearest star to our Earth.It is the only star which can be observed and investigated by us in some spatial resolutions.It plays an important role in the development of modern astrophysics and astronomy.Meanwhile,the Sun brings us the warmth and brightness and its intense activities also have a great effect on the terrestrial environment.It is extremely meaningful to explore the activities and revolutions of the Sun.This paper introduces the basic conceptions and the research methods of the solar physics,makes a brief summary of the main achievements during the past half century,and then discusses the key problems and the prospective on the frontier of solar physics.