Abstract:The heliospheric structure ranging from the solar surface to the earth's orbit is self-consistently reproduced from a time-stationary three-dimensional (3D) magnetohydrodynamic (MHD) simulation. The simulation model incorporates gravity, Coriolis, and centrifugal forces into the momentum equation, and coronal heating and fieldaligned thermal conduction into the energy equation. The heating term in the present model has its peak at 2.8 solar radius (R s ) and exponentially falls to zero at greater distance from… Show more
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