Effects of Temperature Bias on Nanoflare Statistics

Markus J. Aschwanden, Paul Charbonneau
2002 Astrophysical Journal  
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 24
doi:10.1086/339451 fatcat:lzbphwkjqzcijat46pql3xo4yu