22 citations as recorded by crossref.

1. Comparative analyses of current three-dimensional numerical solar wind models S. Wu & M. Dryer https://doi.org/10.1007/s11430-015-5062-1
2. Implicit predictor–corrector central finite difference scheme for the equations of magnetohydrodynamic simulations T. Tsai et al. https://doi.org/10.1016/j.cpc.2015.05.001
3. Comparison of astrospheres around cool and hot stars K. Scherer et al. https://doi.org/10.1088/1742-6596/767/1/012024
4. Shock structures of astrospheres K. Scherer et al. https://doi.org/10.1051/0004-6361/201526137
5. THREE-DIMENSIONAL SOLARWINDMODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID X. Feng et al. https://doi.org/10.1088/0004-637X/723/1/300
6. Tests of a new code that simulates the evolution of solar winds and CMEs F. Guzmán & L. Mendoza Mendoza https://doi.org/10.1088/1742-6596/2307/1/012020
7. CAFE-AMR: a computational MHD solar physics simulation tool that uses AMR R. Ochoa-Armenta & F. Guzmán https://doi.org/10.1093/mnras/stad2342
8. The CRONOS Code for Astrophysical Magnetohydrodynamics R. Kissmann et al. https://doi.org/10.3847/1538-4365/aabe75
9. Using a 3‐D spherical plasmoid to interpret the Sun‐to‐Earth propagation of the 4 November 1997 coronal mass ejection event Y. Zhou et al. https://doi.org/10.1029/2010JA016380
10. SIP-CESE MHD model of solar wind with adaptive mesh refinement of hexahedral meshes X. Feng et al. https://doi.org/10.1016/j.cpc.2014.03.027
11. Simulation of the Unusual Solar Minimum with 3D SIP-CESE MHD Model by Comparison with Multi-Satellite Observations L. Yang et al. https://doi.org/10.1007/s11207-011-9785-7
12. Magnetic clouds in the solar wind: a numerical assessment of analytical models G. Dalakishvili et al. https://doi.org/10.1051/0004-6361/201015468
13. A HYBRID SOLAR WIND MODEL OF THE CESE+HLL METHOD WITH A YIN-YANG OVERSET GRID AND AN AMR GRID X. Feng et al. https://doi.org/10.1088/0004-637X/734/1/50
14. Nanodust dynamics during a coronal mass ejection A. Czechowski & J. Kleimann https://doi.org/10.5194/angeo-35-1033-2017
15. 4π Models of CMEs and ICMEs (Invited Review) J. Kleimann https://doi.org/10.1007/s11207-012-9994-8
16. Alfvén wave solar model (AWSoM): proton temperature anisotropy and solar wind acceleration X. Meng et al. https://doi.org/10.1093/mnras/stv2249
17. A multi-GPU finite volume solver for magnetohydrodynamics-based solar wind simulations Y. Wang et al. https://doi.org/10.1016/j.cpc.2018.12.003
18. MHD simulation of the inner‐heliospheric magnetic field T. Wiengarten et al. https://doi.org/10.1029/2012JA018089
19. Cosmic rays in astrospheres K. Scherer et al. https://doi.org/10.1051/0004-6361/201425091
20. COSMIC RAY TRANSPORT IN HELIOSPHERIC MAGNETIC STRUCTURES. I. MODELING BACKGROUND SOLAR WIND USING THE CRONOS MAGNETOHYDRODYNAMIC CODE T. Wiengarten et al. https://doi.org/10.1088/0004-637X/788/1/80
21. GENERALIZED MULTI-POLYTROPIC RANKINE–HUGONIOT RELATIONS AND THE ENTROPY CONDITION K. Scherer et al. https://doi.org/10.3847/1538-4357/833/1/38
22. IMPLEMENTING TURBULENCE TRANSPORT IN THE CRONOS FRAMEWORK AND APPLICATION TO THE PROPAGATION OF CMEs T. Wiengarten et al. https://doi.org/10.1088/0004-637X/805/2/155