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Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions
Lucas A. Tarr, N. Dylan Kee, Mark G. Linton, Peter W. Schuck and James E. Leake The Astrophysical Journal Supplement Series 270(2) 30 (2024) https://doi.org/10.3847/1538-4365/ad0e0c
Magnetic flux rope models and data-driven magnetohydrodynamic simulations of solar eruptions
Yang Guo, Jinhan Guo, Yiwei Ni, Chun Xia, Ze Zhong, Mingde Ding, Pengfei Chen and Rony Keppens Reviews of Modern Plasma Physics 8(1) (2024) https://doi.org/10.1007/s41614-024-00167-2
MHD Simulations of the Solar Corona to Determine the Conditions for Large Solar Flares and the Acceleration of Cosmic Rays during Them
Helium abundance and speed difference between helium ions and protons in the solar wind from coronal holes, active regions, and quiet Sun
Hui Fu, Maria S Madjarska, Bo Li, Lidong Xia and Zhenghua Huang Monthly Notices of the Royal Astronomical Society 478(2) 1884 (2018) https://doi.org/10.1093/mnras/sty1211
Investigating the Magnetic Imprints of Major Solar Eruptions with SDO/HMI High-cadence Vector Magnetograms
Xudong 旭东 Sun 孙, J. Todd Hoeksema, Yang 扬 Liu 刘, Maria Kazachenko and Ruizhu 瑞竹 Chen 陈 The Astrophysical Journal 839(1) 67 (2017) https://doi.org/10.3847/1538-4357/aa69c1
Testing the Accuracy of Data-driven MHD Simulations of Active Region Evolution