| 注册
首页|期刊导航|天文学进展|恒星超级耀斑的研究进展

恒星超级耀斑的研究进展

雍浩然 林隽

天文学进展2024,Vol.42Issue(3):383-428,46.
天文学进展2024,Vol.42Issue(3):383-428,46.DOI:10.3969/j.issn.1000-8349.2024.03.01

恒星超级耀斑的研究进展

Advance in the Research of Stellar Superflares

雍浩然 1林隽2

作者信息

  • 1. 中国科学院 云南天文台,昆明 650216||中国科学院大学,北京 100049
  • 2. 中国科学院 云南天文台,昆明 650216||中国科学院大学,北京 100049||中国科学院 天文大科学研究中心,北京 100012||云南省太阳物理与空间目标监测重点实验室,昆明 650216
  • 折叠

摘要

Abstract

The Solar flare is one of the most violent eruptive phenomena in the Solar system,which releases energy up to 1025 J in tens of minutes.With the development of observational techniques,similar flare events have been observed on stars,with typical energy of 10 to 104 times that of Solar flares,which is known as the superflare.Studies of stellar superflares and their mechanisms are not only important for understanding the internal structure,evolution and magnetic activities of stars,but also for exploring the habitability and extraterrestrial life on exoplanets.A brief introduction is first given on Solar flares and the associated phenomena of magnetic activities,stellar magnetic field,and superflares of stars.Then,current detection methods and research results of stellar superflares are reviewed in terms of selection,energy evaluation,starspots,and the statistical relationships between the flare parameters and stellar parameters.Meanwhile,a comparison is made between theories of Solar flares and the related physical processes to explore their similarities and connections.Finally,a summary is made and the related further work is also discussed.

关键词

恒星耀斑/大样本/磁活动/太阳耀斑

Key words

stellar flares/large sample/magnetic activity/Solar flares

分类

天文与地球科学

引用本文复制引用

雍浩然,林隽..恒星超级耀斑的研究进展[J].天文学进展,2024,42(3):383-428,46.

基金项目

国家重点研发计划(2022YFF0503804) (2022YFF0503804)

国家自然科学基金(11933009) (11933009)

云南省"兴滇英才支持计划-云岭学者" ()

云南省"兴滇英才支持计划-科学家工作室(太阳物理研究)" (太阳物理研究)

天文学进展

OA北大核心CSTPCD

1000-8349

访问量4
|
下载量0
段落导航相关论文