Physics
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11..176z&link_type=abstract
Chinese Journal of Space Science (ISSN 0254-6124), vol. 11, no. 3, p. 176-186.
Physics
1
Magnetic Field Configurations, Magnetic Flux, Magnetic Signatures, Short Wave Radiation, Solar Magnetic Field, Polarity, Solar Activity
Scientific paper
The magnetograms of the longitudinal field in 18 activity regions for April-December, 1988 are analyzed. Some magnetic precursors of the flares causing strong short wave fade-out (SWF flares) are distinguished from the magnetograms of the longitudinal field. They are: (1) emergence of the magnetic flux in a magnetic area with the opposite polarity, with an intensity larger than or equal to 160G; (2) incorporation of the magnetic fluxes with similar polarity; (3) invasion of a magnetic flux with opposite polarity; and (4) a sharp increase in the magnetic intensity. There is a close relation between the SWF flares and the magnetic precursors.
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