Development and application of three-dimensional time-dependent magnetohydrodynamic numerical model

Statistics – Applications

Scientific paper

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Aerospace Environments, Applications Programs (Computers), Magnetohydrodynamics, Mathematical Models, Solar Wind, Space Plasmas, Weather Forecasting, Solar Activity Effects, Steady Flow, Thermal Conductivity, Time Dependence, Unsteady Flow

Scientific paper

Modifications and implementations to the steady, three-dimensional MHD solar wind model (STDSOL) and to the unsteady, three-dimensional MHD solar wind model (UTDSOL) are completed. These models are appropriate for steady and time-dependent simulations of interplanetary disturbances between 18 solar radii and 1 AU. Example computations for both steady and transient cases were made to examine the capabilities of these models. In addition to two MHD models, a transient one-dimensional hydrodynamic transonic numeric model (TOH) was completed. The model is capable of simulating solar wind expansions through the hydrodynamic critical point. Example computations were performed for thermally-conductive solar wind between the solar surface and 1 AU.

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