Other
Scientific paper
Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...68..275p&link_type=abstract
Solar Physics, vol. 68, Dec. 1980, p. 275-278.
Other
3
Gas Dynamics, Inviscid Flow, Ionized Gases, Isothermal Flow, One Dimensional Flow, Solar Atmosphere, Spicules, Lines Of Force, Pressure Gradients, Solar Magnetic Field
Scientific paper
A one-dimensional model of nonviscous gas in isothermal flow is considered, using the theory of Abramovich (1976). A mechanism of spicule flow is proposed which successfully explains the observed spicule height. The model further predicts inhomogeneities in the magnetic field topology, and in the direction and magnitude of the velocity flow.
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