Physics
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...61...23r&link_type=abstract
Solar Physics, vol. 61, Feb. 1979, p. 23-34.
Physics
28
Magnetic Flux, Solar Granulation, Solar Magnetic Field, Solar Physics, Spicules, Atmospheric Physics, Magnetic Effects, Solar Corona
Scientific paper
It is proposed that spicules are the direct result of a resonant buffeting of the sides of an intense (kilogauss) slender flux tube by turbulent granular motions. For a critical wave speed, the granular motion drives a high-speed flow along the axis of the tube. This effect is illustrated by considering in detail a flux tube embedded in a uniform compressible atmosphere, thereby modeling the development of the 'seedflow' in the photosphere that eventually manifests itself in the chromosphere as the spicule.
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