Computer Science
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spme.rept.....l&link_type=abstract
Unknown
Computer Science
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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