Basic geometrical properties of the velocity and magnetic field in sunspots

Details Basic geometrical properties of the velocity and magnetic field in sunspots Basic geometrical properties of the velocity and magnetic field in sunspots

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...149..291b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 149, no. 2, Aug. 1985, p. 291-294.

Astronomy and Astrophysics

Astrophysics

9

Flow Velocity, Magnetic Field Configurations, Magnetohydrodynamic Flow, Solar Magnetic Field, Sunspots, Differential Equations, Photosphere, Solar Activity

Scientific paper

The predominant horizontality of the velocity vector and the anticorrelation of velocity and magnetic field, which are characteristics of field distributions in solar active regions, are presently explained in terms of a simple model that takes into account the physical conditions at the photosphere in active regions. Attention is given to the coupling between magnetic field and velocity regions.

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