Sunspots and the physics of magnetic flux tubes. V - Mutual hydrodynamic forces between neighboring tubes

Details Sunspots and the physics of magnetic flux tubes. V - Mutual hydrodynamic forces between neighboring tubes Sunspots and the physics of magnetic flux tubes. V - Mutual hydrodynamic forces between neighboring tubes

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231..270p&link_type=abstract

Astrophysical Journal, Part 1, vol. 231, July 1, 1979, p. 270-276.

Physics

22

Circular Cylinders, Hydrodynamics, Magnetic Flux, Solar Magnetic Field, Sunspots, Ideal Fluids, Solar Physics, Stellar Models

Scientific paper

The mutual hydrodynamic forces between parallel cylinders in a moving fluid are illustrated through several formal examples. Parallel tubes in a uniform flow are attracted or repelled depending on whether they are side by side or one ahead of the other, respectively. A pulsating or undulating tube attracts all other neighboring tubes toward itself. These hydrodynamic effects suggest that the separate flux tubes beneath the sunspots exert significant attractive forces on each other.

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