李文顯

2015年獲得復旦大學博士學位，2015年至2020年期間在瑞典隆德大學、瑞典馬爾默大學、美國國家大氣研究中心高山天文台從事博士後研究。於2021年1月入職中科院國家天文台工作至今。主要從事太陽磁場測量、原子結構計算、等離子體光譜診斷等方面的研究。承擔國家自然科學基金青年項目1項。 ^[1] 

1. W. Li, M. Li, K. Wang, T. Brage, R. Hutton, and E. Landi, A Theoretical Investigation of the Magnetic-field-induced Transition in Fe X, of Importance for Measuring Magnetic Field Strengths in the Solar Corona, Astrophys. J., 2021, 913:135.

2. W. Li, A. M. Amarsi, A. Papoulia, J. Ekman and P. Jonsson, Extended theoretical transition data in C I – IV, Monthly Notices of the Royal Astronomical Society, 2021, 502,3780-3799.

3. W. Li, H. Hartman, K. Wang, and P. Jonsson, Theoretical investigation of oscillator strengths and lifetimes in Ti II, Astronomy & Astrophysics, 2020, 643, A156.

4. W. Li, P. Rynkun, L. Radziūte, G. Gaigalas, B. Atalay, A. Papoulia, K. Wang, H. Hartman, J. Ekman, T. Brage, C. Y. Chen, and P. J？nsson, Multiconfiguration Dirac-Hartree-Fock Calculations of Landé g-factors for Ions of Astrophysical interests: B II, C I-IV, Al I-II, Si I-IV, P II, S II, Cl III, Ar IV, Ca I, Ti II, Zr III and Sn II, Astronomy & Astrophysics, 2020, 639, A25.

5. W. Li, J. Grumer, T. Brage, and P. Jonsson, Hfszeeman95—A program for computing weak and intermediate magnetic-field- and hyperfine-induced transition rates, Comput. Phys. Commun.,2020, 107211.

6. W. Li, R. Casini, S. Tomczyk, E. Landi Degl’Innocenti and B. Marsell, Laboratory test of scattering polarization models, Astrophys. J. Lett. 2018, 867:L22.

7. W. Li, R. Casini, T. del Pino Alemán and P. G. Judge, Solar Spectral Lines with Special Polarization Properties for the Calibration of Instrument Polarization,Astrophys. J. 2017, 848:82. ^[1]