Speaker
Igor Petrov
(Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy)
Description
Radio emission at Yakutsk Array registers at frequency 32 MHz and radio antennas co-located with scintillation and Cherenkov detectors of Yakutsk Array. The co-location with particle detectors brings as a profit the reconstruction of fundamental air shower parameters, such as shower axis, energy and arrival direction (azimuthal and zenith angles).
The paper presents data obtained in the new series of measurements of Yakutsk Radio Array in the period 2009-2013 years. We analyze individual showers and reconstruct Xmax by slope of radio LDF. Obtained results of Xmax are compared with results of other arrays.
| Registration number following "ICRC2015-I/" | 273 |
|---|---|
| Collaboration | -- not specified -- |
Author
Igor Petrov
(Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy)
Co-authors
Stanislav Knurenko
(Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy)
Dr
Zim Petrov
(Yu.G. Shafer Institute of cosmophysical research and aeronomy)
