Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..500l&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Aug. 1982, p. 500-505) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, July-Aug.
Astronomy and Astrophysics
Astronomy
3
Brightness Distribution, Magnetic Flux, Solar Flares, Solar Magnetic Field, Solar Spectra, Spectrum Analysis, Iron, Line Spectra, Magnetic Signatures, Zeeman Effect
Scientific paper
Analysis of a spectrum of the 1981 July 26 solar flare indicates that the 'magnetic transients' recently detected with a videomagnetograph at the Big Bear Solar Observatory more likely represent brightness effects than magnetic phenomena. Direct measurements of the Zeeman splitting in the 5233, 5324, 5447, 5587 Fe I lines show that in this flare the field strength reached 3000 gauss.
Lozitskaia N. I.
Lozitskii V. G.
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