Do Solar Flares Exhibit an Interval-size Relationship?

Details Do Solar Flares Exhibit an Interval-size Relationship? Do Solar Flares Exhibit an Interval-size Relationship?

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..191..381w&link_type=abstract

Solar Physics, v. 191, Issue 2, p. 381-389 (2000).

Physics

18

Scientific paper

Some models for flare statistics predict or assume that there is a relationship between the times between flares and the energy of flares. This question is examined observationally using the WATCH solar X-ray burst catalogue. A rank correlation test applied to the data finds strong evidence for a correlation between the time since the last event, t_b, and the size (peak count rate) of an event, and for a correlation between the time to the next event, t_a, and the size of an event. A more sophisticated statistical test, taking into account a probable bias in event selection, does not support the hypothesis that event size depends on t_b or t_a.

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