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Evolution of Coronal Mass Ejections in Different Data-Driven Solar Wind Conditions
Nishtha Sachdeva, Zhenguang Huang, Gabor Toth +3
Numerical models of the solar wind and coronal mass ejections (CMEs) utilize photospheric magnetic field observations to prescribe the inner boundary conditions for the plasma solu…
One Year in the Life of Young Suns: Data Constrained Corona-Wind Model of kappa1 Ceti
Vladimir S. Airapetian, Meng Jin, Theresa Lueftinger +5
The young magnetically active solar-like stars are efficient generators of ionizing radiation in the form of X-ray and Extreme UV (EUV) flux, stellar wind and eruptive events. Thes…
Obtaining Potential Field Solution with Spherical Harmonics and Finite Differences
Gabor Toth, Bart van der Holst, Zhenguang Huang
Potential magnetic field solutions can be obtained based on the synoptic magnetograms of the Sun. Traditionally, a spherical harmonics decomposition of the magnetogram is used to c…