太阳物理，原子物理
李文显，女，1989年出生，籍贯山东菏泽，中国科学院国家天文台研究员。2015年获得复旦大学博士学位，2015年至2020年期间在瑞典隆德大学、瑞典马尔默大学、美国国家大气研究中心高山天文台从事博士后研究。于2021年1月入职中科院国家天文台工作至今。主要从事太阳磁场测量、原子结构计算、等离子体光谱诊断等方面的研究。承担国家自然科学基金青年项目1项。
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.