Speaker
Dr
Alexander Karelin
(NRNU MEPhI)
Description
The study of a large-scale anisotropy was done for the hadronic component of cosmic rays in the energy range 1 – 20 TeV/n using the data of the PAMELA experiment. However the statistics available was low to carry out its direct measurement. But the amplitude and phase of anisotropy can be obtained under an assumption that it exists and has a dipole form. The uncertainties of these values can be obtained by two different ways. The approaches of these uncertainty estimations are discussed in this work.
Primary author
Dr
Alexander Karelin
(NRNU MEPhI)
