Small-scale structure of solar magnetic fields

Details Small-scale structure of solar magnetic fields Small-scale structure of solar magnetic fields

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...28l&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Jan.-Feb. 1986, p. 28-35. In Russian.

Computer Science

2

Fine Structure, Photosphere, Solar Magnetic Field, Line Spectra, Polarization Characteristics, Solar Flares, Stellar Structure, Zeeman Effect

Scientific paper

Zeeman spectrograms of photospheric magnetic fields of three active regions (Nos. 113, 123, and 216) and magnetic fields in a 2B flare are analyzed. Nonsunspot magnetic fields are found to have two spatially unresolved components: a quasi-homogeneous vertical component with strengths less than about 1 T and a multipolar component with strengths less than about 0.1 T. The total magnetic fluxes of these components are approximately the same; the components are closely connected, and could belong to small-scale flux ropes.

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