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Effects of Temperature Bias on Nanoflare Statistics
Statistics of solar flares, microflares, and nanoflares have been gathered over an energy range of some 8 orders of magnitude, over -10 32 ergs. Frequency distributions of flare energies are always determined in a 24doi:10.1086/339451 fatcat:lzbphwkjqzcijat46pql3xo4yu