The problem of superstrong magnetic fields in the solar atmosphere

Details The problem of superstrong magnetic fields in the solar atmosphere The problem of superstrong magnetic fields in the solar atmosphere

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kfnt....9...23l&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 9, no. 3, p. 23-32.

Physics

5

Line Spectra, Magnetic Flux, Solar Atmosphere, Solar Magnetic Field, Zeeman Effect, Magnesium, Metallicity

Scientific paper

New and old observational data on the existence of magnetic fields over 0.5 T are analyzed. Three new effects have been detected from observations of the flare on June 16, 1989: (1) nontypical splitting of emission in the lines Mg I 517.27 and 518.36 nm; (2) local extremum of bisector splitting for (rj +/- rv) profiles in H-alpha, Hr-gamma, and H-epsilon; and (3) evidence of the Zeeman effect in nonsplit line Fe I 543.45 nm. The first effect corresponds to field strengths of 0.4-0.7 T by direct measurements; the second and the third ones to 4-5 T.

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