Physics
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..112..387s&link_type=abstract
Solar Physics, Volume 112, Issue 2, pp.387-390
Physics
Scientific paper
An analysis of the data of Achong and Stahl (1984) discloses discrete intervals which differ significantly in SID flare incidence and the proportion of complex sunspot groups present. This supports the alternative interpretation of Sawyer et al. (1985) in respect of the strong dependence of SID flare production on complex magnetic class (see Abstr. 40.073.048).
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