Mass Composition of Ultrahigh-Energy Cosmic Rays, According to Data from the Pierre Auger Collaboration (A Statistical Investigation Using the Copula Function)статья
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Дата последнего поиска статьи во внешних источниках: 19 сентября 2015 г.
Аннотация:The mass composition of cosmic rays with ultrahigh energies (2 × 10^18 – 5 × 10^19 eV) is studied using the publicly accessible data of the Pierre Auger Collaboration as of January 1, 2014. Employing tools for describing intrinsic relations inside multidimensional distribution (the Copula function) at 3 × 10^18 – 3 × 10^19 eV, the investigation reveals a mass composition weight of a complex nature.