In the tested avalanche models for solar flares, the power-law flare size distribution is carried by power-law transition rates between energy states, not by the distribution of active region energies.
J., Caspi, A., Cohen, C
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Energy Balance in Avalanche Models for Solar Flares
In the tested avalanche models for solar flares, the power-law flare size distribution is carried by power-law transition rates between energy states, not by the distribution of active region energies.