SID flare production is independent of Mt. Wilson magnetic class

Details SID flare production is independent of Mt. Wilson magnetic class SID flare production is independent of Mt. Wilson magnetic class

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...92..259a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 92, May 1984, p. 259-269.

Physics

3

Solar Flares, Solar Magnetic Field, Solar Terrestrial Interactions, Sudden Ionospheric Disturbances, Sunspots, Frequency Distribution, Magnetic Field Configurations, Poisson Density Functions, Statistical Distributions

Scientific paper

The authors have analyzed the observed frequency distributions of SID flare days for the different sunspot magnetic classes, taking flare days as well as 'no flare' days into account. They find that there is no significant difference between any observed distribution for a specific magnetic class, and the Poisson random theoretical distribution, computed for that class.

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