Speaker
Dr.
Victor Shutenko
(National Research Nuclear University (MEPhI))
Description
Investigations of cosmic rays on the surface of the Earth allow to derive information of applied character on the conditions of the interplanetary magnetic field and of the geomagnetic field. For this purpose, it is necessary to collate the trajectories of the particles detected in the ground detector to trajectories of primary cosmic rays in the heliosphere. This problem is solved by means of various back-tracking methods. In this work, one of such methods is presented.
Primary author
Dr.
Victor Shutenko
(National Research Nuclear University (MEPhI))
