Speaker
Mr
Petr Gololobov
(ShICRA of SB RAS)
Description
In this work the dynamics of tensor anisotropy of cosmic rays during the passage of large-scale disturbances of the solar wind for the 22-24 solar cycles is studied. The information on the anisotropy was obtained using a global survey method by data of the worldwide neutron monitor network. For the analysis of the obtained results the data on the interplanetary magnetic field state and solar wind parameters are used.
| Registration number following "ICRC2015-I/" | 0264 |
|---|---|
| Collaboration | -- not specified -- |
Author
Mr
Petr Gololobov
(ShICRA of SB RAS)
Co-authors
Prof.
Germogen Krymsky
(ShICRA of SB RAS)
Dr
Prokopii Krivoshapkin
(ShICRA of SB RAS)
Dr
Sardaana Gerasimova
(ShICRA of SB RAS)
Dr
Vladislav Grigoryev
(ShICRA of SB RAS)
