Peak gamma-ray intensity of solar flares.
Details
" 'The cumulative distribution of the peak gamma-ray intensity of solar flares. The observations were made between 1980 and 1989 by the instrument known as the Hard X-Ray Burst Spectrometer aboard the Solar Maximum Mission satellite launched in 1980. The spectrometer used a CsI scintillation detector to measure gamma-rays from solar flare... The data are from the NASA Goddard Space Flight Center, umbra.nascom.nasa.gov/smm/hxrbs.html.' Quoted from: Newman, M. (2005). Power laws, Pareto distributions and Zipf’s law. Contemporary Physics, 46(5), 323–351. https://doi.org/10.1080/00107510500052444"