2022
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  1. Zhang, M.; Feng, X. A Three-Order, Divergence-Free Scheme for the Simulation of Solar Wind. Universe 2022, 8,  371. https://doi.org/10.3390/universe8070371

  2. Liu X, Feng X, Lv J, Wang X and Zhang M (2022), Direct discontinuous Galerkin method for potential magnetic field solutions. Front. Astron. Space Sci. 9:1055969. doi: 10.3389/fspas.2022.1055969 [PDF]

  3. Liu et al., Implementation of the HLL-GRP solver for multidimensional ideal MHD simulations based on fifinite volume method, Journal of Computational Physics 473 (2023) 111687, https://doi.org/10.1016/j.jcp.2022.111687

  4. Liu et al., Numerical Research on the Effect of the Initial Parameters of CME Flux-rope Model on Simulation Results. III. Different Initial Energy of CMEs, The Astrophysical Journal, 940:11 (11pp), 2022, https://doi.org/10.3847/1538-4357/ac9b16

  5. Lu et al., Temporal and spatial response of Holocene temperature to solar activity, Quaternary International 613 (2022) 39–45, https://doi.org/10.1016/j.quaint.2021.09.006

  6. Shen et al., Propagation characteristics of coronal mass ejections (CMEs) in the corona and interplanetary space, Reviews of Modern Plasma Physics (2022) 6:8, https://doi.org/10.1007/s41614-022-00069-1

  7. Wang et al., Implicit Solar Coronal Magnetohydrodynamic (MHD) Modeling with a Low-dissipation Hybridized AUSM-HLL Riemann Solver, The Astrophysical Journal, 935:46 (20pp), 2022. https://doi.org/10.3847/1538-4357/ac78e0

  8. Wang et al., MHD Simulation of Homologous Eruptions from Solar Active Region 10930 Caused by Sunspot Rotation, The Astrophysical Journal, 938:61 (17pp), 2022. https://doi.org/10.3847/1538-4357/ac8d0e

  9. Zhang, W.; Zhao, X.; Feng, X.; Liu, C.; Xiang, N.; Li, Z.; Lu, W. Predicting the Daily 10.7-cm Solar Radio Flux Using the Long Short-Term Memory Method. Universe 2022, 8, 30. https://doi.org/10.3390/universe8010030

  10. ZHAO Xinhua, HE Jiansen, SHEN Chenglong, FENG Shiwei, JIANG Chaowei, LI Huichao, QIN Gang, LUO Xi. A Brief Review of Interplanetary Physics Research Progress in Mainland China during 2020– 2022.  Chinese Journal of Space Science, 2022, 42(4): 612-627. DOI:10.11728/cjss 2022.04.yg19 [PDF]

  11. Wang H P, Zhao J M, Lü J K, etal. 2022. A solenoidality-preserving variational reconstruction method and its application to solar coronal MHD modeling. ChineseJ. Geophys. (in Chinese), 65(8):2779-2795, doi: 10.6038/cjg2022P0818.  [PDF]

  12. LIU Chang, SHEN Fang, LIU Yousheng. Three-dimensional Numerical Simulation of Coronal Solar Wind (in Chinese).  Chinese Journal of Space Science, 2022, 42(1): 25-33. DOI:10.11728/cjss2022.01.201127102 [PDF]

  13. Ma M X, Shen F, Liu Y S. 2022. Simulation study on the propagation process of coronal mass ejection. Reviews of Geophysics and Planetary Physics, 53(4): 397-415. doi:10.19975/j.dqyxx.2021-064 [PDF]

  14. ZHANG Hanke, SHEN Fang. Application of Data Assimilation in Space Weather (in Chinese). Chinese Journal of Space Science, 2022, 42(3): 422-436. DOI:10.11728/cjss2022.03.210611069 [PDF]