On the magnetic and velocity field geometry of simple sunspots

Details On the magnetic and velocity field geometry of simple sunspots On the magnetic and velocity field geometry of simple sunspots

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...403..780t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 403, no. 2, p. 780-796.

Astronomy and Astrophysics

Astrophysics

170

Solar Magnetic Field, Sunspots, Velocity Distribution, Charge Coupled Devices, Correlation Coefficients, Flow Distribution, Lorentz Force, Magnetic Field Configurations, Penumbras

Scientific paper

It is presently shown that a simple sunspot model with azimuthal variations in inclination, but lacking azimuthal field-strength variations, is free from azimuthal Lorentz forces. The meridional currents arising from the inclination variations are parallel to the field lines, suggesting that a cylindrically symmetric magnetostatic sunspot model can be perturbed into one with azimuthal variations in inclination with adjustment of the meridional force balance.

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