Physics
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...80s&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Sept.-Oct. 1986, p. 80-84. In Russian.
Physics
3
Force-Free Magnetic Fields, Magnetostatics, Solar Magnetic Field, Fine Structure, Magnetic Field Configurations, Magnetic Flux, Multipolar Fields
Scientific paper
A magnetostatic model based on the axisymmetric solution for a linear force-free field is proposed which explains the existence of certain small-scale (not greater than 10 to the 7th cm) solar magnetic elements. These elements are characterized by a magnetic field strength not greater than about 1 Tl, the quantization of H, a sharp concentration of the field toward the axis, a multipolar H profile, and a high vertical gradient of H (about -1 mTl/km).
Lozitskii V. G.
Solovev Alexander
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