季索清
发布时间: 2024-05-08     文章作者:     访问次数: 4496




季索清



青年研究员/Associate Professor

2018年加州大学圣塔芭芭拉分校博士/Ph.D. (2018), University of California Santa Barbara

电话:

E-mailsqji@fudan.edu.cn

个人网站/Website中文   English 


主要经历:

2011.7 安徽建筑大学应用物理学学士

2013.5 马萨诸塞大学达特茅斯分校物理学硕士

2018.9 加州大学圣塔芭芭拉分校物理学博士

2018-2021 加州理工学院博士后费尔柴尔德学者

2021-2024 中国科学院上海天文台青年研究员

2024至今 复旦大学物理学系青年研究员


教学与研究领域:

星系的形成与演化:环星系介质,超新星与活动星系核反馈,宇宙射线,星系团;

天体物理流体动力学:湍流,磁流体动力学,流体与等离子体不稳定性;

计算天体物理



Suoqing Ji


Associate Professor

Ph.D. (2018), University of California Santa Barbara


Research Interests:

Galaxy formation and evolution: the circumgalactic medium, supernova and AGN feedback, cosmic rays, galaxy clusters;

Astrophysical fluid dynamics: turbulence, magnetohydrodynamics, fluid and plasma instabilities;

Computational astrophysics


Selected Publications:

1) Yang Yanhui, Ji Suoqing. “Radiative turbulent mixing layers at high Mach numbers.” MNRAS, 520(2), 2148-2162, 2023.

2) Ji Suoqing, Fuller Jim, Lecoanet Daniel. “Magnetohydrodynamic simulations of the Tayler instability in rotating stellar interiors.” MNRAS, 521(4), 5372-5383, 2023.

3) Ji Suoqing, Squire Jonathan, Hopkins Philip F. “Numerical study of cosmic ray confinement through dust resonant drag instabilities.” MNRAS, 513(1), 282-295, 2022.

4) Ji Suoqing, Chan TK, Hummels Cameron B, Hopkins Philip F, Stern Jonathan, Kereš Dušan, Quataert Eliot, Faucher-Giguère Claude-André, Murray Norman. “Properties of the circumgalactic medium in cosmic ray-dominated galaxy haloes.” MNRAS, 496(4), 4221-4238, 2020.

5) Ji Suoqing, Oh S Peng, Masterson Phillip. “Simulations of radiative turbulent mixing layers.” MNRAS, 487(1), 737-754, 2019.

6) Ji Suoqing, Oh S Peng, McCourt Michael. “The impact of magnetic fields on thermal instability.” MNRAS, 476(1), 852-867, 2018.

7) Ji Suoqing, Fisher Robert T, García-Berro Enrique, Tzeferacos Petros, Jordan George, Lee Dongwook, Lorén-Aguilar Pablo, Cremer Pascal, Behrends Jan. “The post-merger magnetized evolution of white dwarf binaries: the double-degenerate channel of sub-Chandrasekhar Type Ia super- novae and the formation of magnetized white dwarfs.” ApJ, 773(2), 136, 2013.






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