Toward a Quantitative Model for Simulation and Forecast of Solar Energetic Particle Production during Gradual Events. I. Magnetohydrodynamic Background Coupled to the SEP Model von Borovikov, D, Sokolov, I.V, Roussev, I.I, Taktakishvili, A, Gombosi, T.I

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Observational evidence of CMEs interacting in the inner heliosphere as inferred from MHD simulations von Lugaz, N., Manchester IV, W.B., Roussev, I.I., Gombosi, T.I.

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Solution-adaptive magnetohydrodynamics for space plasmas: Sun-to-Earth simulations von Gombosi, T.I., Powell, K.G., De Zeeuw, D.L., Clauer, C.R., Hansen, K.C., Manchester, W.B., Ridley, A.J., Roussev, I.I., Sokolov, I.V., Stout, Q.F., Toth, G.

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Magnetic reconnection during eruptive magnetic flux ropes von Mei, Z.X, Keppens, Rony, Roussev, I.I, Lin, J

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Numerical modeling of interplanetary coronal mass ejections and comparison with heliospheric images von Lugaz, N., Roussev, I.I.

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Magnetic Field Configuration Models and Reconstruction Methods for Interplanetary Coronal Mass Ejections von Al-Haddad, N, Nieves-Chinchilla, T, Savani, N.P, Moestl, C, Marubashi, K, Hidalgo, M.A, Roussev, I.I, Poedts, Stefaan, Farrugia, C.J

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On the internal structure of the magnetic field in magnetic clouds and interplanetary coronal mass ejections: writhe versus twist von Al-Haddad, N, Roussev, I.I, Moestl, C, Jacobs, Carla, Lugaz, N, Poedts, Stefaan, Farrugia, C.J

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THE INTERNAL STRUCTURE OF CORONAL MASS EJECTIONS: ARE ALL REGULAR MAGNETIC CLOUDS FLUX ROPES? von Jacobs, C, Roussev, I.I, Lugaz, N, Poedts, S

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Validation of a global 3D heliospheric model with observations for the May 12, 1997 CME event von Cohen, O., Sokolov, I.V., Roussev, I.I., Lugaz, N., Manchester, W.B., Gombosi, T.I., Arge, C.N.

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A TVD principle and conservative TVD schemes for adaptive Cartesian grids von Sokolov, I.V., Powell, K.G., Gombosi, T.I., Roussev, I.I.

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