Self-Organized Criticality in Solar and Stellar Flares: Are Extreme Events Scale-Free ?
arXiv:1906.05840 · doi:10.3847/1538-4357/ab29f4
Abstract
We search for outliers in extreme events of statistical size distributions of astrophysical data sets, motivated by the {\sl Dragon-King hypothesis} of Sornette (2009), which suggests that the most extreme events in a statistical distribution may belong to a different population, and thus may be generated by a different phyiscal mechanism, in contrast to the strict power law behavior of {\sl self-organized criticality (SOC)} models. Identifying such disparate outliers is important for space weather predictions. Possible physical mechanisms to produce such outliers could be generated by sympathetic flaring. However, we find that Dragon-King events are not common in solar and stellar flares, identified in 4 out of 25 solar and stellar flare data sets only. Consequently, small, large, and extreme flares are essentially scale-free and can be modeled with a single physical mechanism. In very large data sets ($N \gapprox 10^4$) we find significant deviations from ideal power laws in almost all data sets. Neverthess, the fitted power law slopes constrain physcial scaling laws in terms of flare areas and volumes, which have the highest nonlinearity in their scaling laws.
6 Figures
References in corpus (7)
- Power-law distributions in empirical data
- Toward Reliable Benchmarking of Solar Flare Forecasting Methods
- Dragon-kings: mechanisms, statistical methods and empirical evidence
- 25 Years of Self-Organized Criticality: Solar and Astrophysics
- Driving major solar flares and eruptions: a review
- Global Energetics of Solar Flares: V. Energy Closure in Flares and Coronal Mass Ejections
- Global Energetics of Solar Flares: I. Magnetic Energies
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