The origin of running penumbral waves

Details The origin of running penumbral waves The origin of running penumbral waves

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184p..49g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Aug. 1978, p. 49P-52P.

Astronomy and Astrophysics

Astronomy

7

Magnetohydrodynamic Waves, Penumbras, Solar Magnetic Field, Sunspots, Traveling Waves, Wave Propagation, Boussinesq Approximation, Convection, Navier-Stokes Equation, Rayleigh Number, Standing Waves, Time Dependence, Wave Fronts

Scientific paper

Numerical experiments on axisymmetric convection with a magnetic field
display solutions in which steady convection concentrates the field into
a strong central rope. Subsequently, oscillations develop within the
rope; this process models the formation of a sunspot with running
penumbral waves.

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