A storage process of the magnetic energy results from the unsteady plasma flow field in the space active regions and stellar atmosphere

Computer Science

Scientific paper

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Flow Distribution, Magnetohydrodynamic Flow, Magnetohydrodynamics, Stellar Atmospheres, Magnetic Fields, Unsteady Flow

Scientific paper

In the discussion about the energy storage by a pure azimuthal motion in
the active regions of solar and stellar atmosphere we consider the
unsteady poloidal flow field and the unsteady coupling process between
the magnetic field and both the toroidal and the poloidal velocity
components.

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