中文核心期刊
CNKI期刊全文数据库
中国科学引文数据库(CSCD)源期刊
中国科技论文统计源期刊
万方数据知识服务平台
英国《科学文摘》(SA)
美国化学文摘(CA)
俄罗斯《文摘杂志》(AJ)
德国《天文学与天体物理学文摘》(AAA)
英国《中国天文学和天体物理学》(SCI收录)全文摘译期刊之一
《中国学术期刊文摘》
《中国物理文摘》
《中国天文学文摘》

Chinese Journal of Space Science ›› 2021, Vol. 41 ›› Issue (2): 183-210.doi: 10.11728/cjss2021.02.183

• Research Articles • Previous Articles     Next Articles

In Situ Detection of the Solar Eruption: Lay a Finger on the Sunormalsize

LIN Jun1,2,3, HUANG Shanjie1,3, LI Yan1, CHONG Xiaoyu4, ZHANG Shenyi5,6, LI Mingtao3,5, ZHANG Yiteng5, ZHOU Bin5, OUYANG Gaoxiang7, XIANG Lei7, DONG Liang1, JI Haisheng8, TIAN Hui9,10, SONG Hongqiang11, LIU Yu1,2,3, JIN Zhenyu1,2,3, FENG Jing4, ZHANG Hongbo12, ZHANG Xianguo5,6, ZHANG Weijie5,6, HUANG Min7, Lü Qunbo7, DENG Lei13, FU Huishan14, CHENG Xin15, WANG Min1   

  1. 1 Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216;
    2 Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012;
    3 University of Chinese Academy of Sciences, Beijing 100049;
    4 Kunming University of Science and Technology, Kunming 650031;
    5 National Space Science Center, Chinese Academy of Sciences, Beijing 100190;
    6 Beijing Key Laboratory of Space Environment Exploration, Beijing 100190;
    7 Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100094;
    8 Purple Mountain Observatories, Chinese Academy of Sciences, Nanjing 210008;
    9 School of Earth and Space Sciences, Peking University, Beijing 100871;
    10 Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing 100012;
    11 Institute of Space Sciences, Shandong University (Weihai), Shandong 264209;
    12 National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012;
    13 Innovation Academy for Microsatellites, Chinese Academy of Sciences, Shanghai 201203;
    14 School of Space and Environment, Beihang University, Beijing 100191;
    15 School of Astronomy and Space Science, Nanjing University, Nanjing 210093
  • Received:2021-02-12 Revised:2021-02-25 Online:2021-03-15 Published:2021-04-10

Abstract: This paper is to introduce a proposed deep space mission, which aims to perform in situ detection of the central structure, namely the magnetic reconnection current sheet, which drives the large scale eruption on a star. The main focus of this mission is on the fine physical characteristics of the large scale magnetic reconnection taking place on the Sun, our nearest star, revealing the secret of the most violent energy release process, also known as the solar storm, in the solar system. The scientific goal of this mission, magnetic reconnection, is a kernel process of energy conversion occurring in the magnetized plasma in the universe, and has long been a fairly important research topic or even research area in solar physics, space science, plasma physics, and the related fields. In situ detection enhances the spatial resolution of the instruments used on the Earth 5~20 times, will provide us extra-clear images of the Sun and the related information. We are thus able to study, to learn, and to understand the Sun on an unprecedented platform, and further resolve the long-standing puzzle in the solar community regarding the fine physical property of the kernel process driving the solar eruption, as well as that of the corona heating.

Key words: Solar eruption, Magnetic reconnection, In situ measurement, High thrust rocket, Thermal protection and isolation, Telecommunications in deep space

CLC Number: