2008年毕业于申慱sunbet官网入口天文学系，并获得申慱sunbet官网入口和巴黎十一大（Paris XI University）理学博士学位，同年赴英国伦敦大学学院（University College London）穆兰德空间科学实验室（Mullard Space Science Laboratory）博士后研究，2011年入职申慱sunbet官网入口天文与空间科学学院。研究领域为太阳物理和空间天文，课题涉及太阳高能粒子事件、日地空间中瞬变现象的研究，以及太阳空间探测设备的研发。先后主持国家自然科学基金青年、面上和重点项目，以及多项省部级科研项目。担任太阳Hα光谱探测与双超平台科学技术试验卫星（“羲和号”卫星）科学与应用系统总设计师、中国空间科学学会空间天文专业委员会副主任。

《空间天气学》，《日地空间环境探索》等。

Project 1: Chinese Hα Solar Explorer (CHASE)

The Chinese Hα Solar Explorer (CHASE), dubbed Xihe -- Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration (CNSA). The CHASE mission is designed to test a new satellite platform and conduct solar observations. The scientific payload of the CHASE mission is an Hα Imaging Spectrograph (HIS) which acquires spectroscopic observations at Hα (655.97 - 656.59 nm) and Fe I (656.78 - 657.06 nm) wavebands. A full-Sun scanning takes ~46 seconds, with a spectral sampling of 0.0024 nm and a spatial resolution of 1.2 arcsec. The science data are available to the community through the Solar Science Data Center of Nanjing University (SSDC-NJU, https://ssdc.nju.edu.cn).

Publications:

Focus Issue in ApJL: Focus on the early results from the Chinese Hα Solar Explorer (CHASE) mission, https://iopscience.iop.org/collections/Focus-on-Early-Results-from-CHASE

Li C., Tian H., Huang Y., New era of Chinese solar instruments, Sci China Tech Sci, 66, 1203, 2023

Li C., Fang C., Li Z., Ding M. D., Chen P. F., Qiu Y., et al. The Chinese Hα Solar Explorer (CHASE) mission: An overview, Sci. China-Phys. Mech. Astron., 65, 289602, 2022

Qiu Y., Rao S. H., Li C., Fang C., Ding M. D., Li Z., et al., Calibration procedures for the CHASE/HIS science data, Sci. China-Phys. Mech. Astron., 65, 289603, 2022

Zhang W., Cheng W. Q., You W., Chen X., Zhang J., Li C., Fang C., Levitated-body ultra-high pointing accuracy and stability satellite platform of the CHASE mission, Sci. China-Phys. Mech. Astron., 65, 289604, 2022

Liu Q., Tao H. J., Chen C. Z., et al., On the technologies of Hα Imaging Spectrograph for the CHASE mission, Sci. China-Phys. Mech. Astron., 65, 289605, 2022

Zhang W., Yang Y., You W., et al., Autonomous navigation method and technology implementation of high-precision solar spectral velocity measurement, Sci. China-Phys. Mech. Astron., 65, 289606, 2022

Li C., Fang C., Li Z., et al., Chinese Hα Solar Explorer (CHASE) -- a complementary space mission to the ASO-S, Research in Astronomy and Astrophysics, 19 (11), 165, 2019

Project 2：Solar energetic particles (SEPs)

SEPs, with energies from a few keV to several GeV, are produced by the release of magnetic energy on the Sun, notably flares and coronal mass ejections (CMEs). What I am interested is to clarify where and how SEPs are accelerated and to understand the processes of propagation for different species of SEPs.

Selected publications:

Li, T. M., Li, C., Ding, W. J., Chen, P. F., Particle-in-cell simulation of 3He enrichment in solar energetic particles, ApJ, 922, 50, 2021

Xu, Z. G., Li, C., Ding, M. D., Observations of a coronal shock wave and the production of solar energetic particles, ApJ, 840, 38, 2017

Li, C., Miroshnichenko, L. I., Sdobnov, V. E., Small ground-level enhancement of 6 January 2014: acceleration by CME-driven shock? Sol. Phys., 291, 975, 2016

Li, C., Miroshnichenko, L. I., Fang, C., Proton activity of the Sun in current solar cycle 24, RAA, 15, 1036, 2015

Li, C., Firoz, K. A., Sun, L. P., Miroshnichenko, L. I., Electron and proton acceleration during the first ground level enhancement event of solar cycle 24, ApJ, 770, 34, 2013

Li, C., Owen, S. J., Matthews, S. A., Dai, Y., Tang, Y. H., Major electron events and coronal magnetic configurations of the related solar active regions, ApJ Letters, 720, 36, 2010

Li, C., Dai, Y., Vial J.-C., et al., Solar source of energetic particles in interplanetary space during the 2006 December 13 event, A&A, 503, 1013, 2009

Li, C., Tang, Y. H., Dai, Y., Fang, C., Vial, J. -C., Flare magnetic reconnection and relativistic particles in the 2003 October 28 event, A&A, 472, 283, 2007

Li, C., Tang, Y. H., Dai, Y., Zong, W. G., Fang, C., The acceleration characteristics of solar energetic particles in the 2000 July 14 event, A&A, 461, 1115, 2007

Project 3: SOC processes in astrophysics

The power-law frequency distributions are ubiquitous in the Universe. Self-organized criticality (SOC) and turbulence are the two intrinsic physical processes during the energy release in a nonlinear dynamical system. Both of them can produce eruptive events with power laws. What I am interested is to understand the roles of SOC and turbulence in astrophysical eruptions.

Selected publications:

Li, C., Wang, W. B., Chen, P. F., Observations and simulations of self-organized criticality phenomena in astrophysics, Sci Sin-Phys Mech Astron, 52, 269501, 2022

Wang, W. B., Li, C., Tu, Z. L., Guo, J. H., Chen, P. F., Wang, F. Y., Avalanches of magnetic flux rope in the state of self-organized criticality, MNRAS, 512, 1567, 2022

Lei, W. H., Li, C., Chen, F., Zhong, S. J., Xu, Z. G., Chen, P. F., Do the solar flares originating from an individual active region follow a random process or a memory-dependent correlation? MNRAS, 494, 975, 2020

Li, C., Zhong, S. J., Xu, Z. G., et al., Waiting time distributions of solar and stellar flares: Poisson process or with memory?, MNRAS, 479, L139, 2018

Li, C. Z., Yang, J. H., Li, C., et al., Self-organized criticality of the solar eruptions during solar cycle 23 (in Chinese). Sci Sin-Phys Mech Astron, 2016, 46: 029501

Li, C., Zhong, S. J., Wang, L., Su, W., Fang, C., Waiting time distributions of solar energetic particle events modeled with a non-stationary Poisson process, ApJ Letters, 792, L26, 2014

学术发表文章

https://www.researchgate.net/profile/Chuan-Li-18

https://orcid.org/0000-0001-7693-4908